of Characteristics planetary candidates observed by Kepler, II: Analysis
of the first four months of data
William J. Borucki0,1, David G. Koch1, Gibor Basri2, Natalie Batalha3, Timothy M. Brown5,
Stephen T. Bryson1, Douglas Caldwell6, Jrgen Christensen-Dalsgaard7, William D. Cochran8,
Edna DeVore6, Edward W. Dunham9, Thomas N. Gautier III11, John C. Geary10, Ronald
Gilliland12, Alan Gould13, Steve B. Howell14, Jon M. Jenkins6, David W. Latham10, Jack J.
Lissauer1, Geoffrey W. Marcy2, Jason Rowe1, Dimitar Sasselov10, Alan Boss4, David
Charbonneau10, David Ciardi22, Laurance Doyle6, Andrea K. Dupree10, Eric B. Ford16, Jonathan
Fortney17, Matthew J. Holman10, Sara Seager18, Jason H. Steffen19, Jill Tarter6, William F.
Welsh20, Christopher Allen21, Lars A. Buchhave10, Jessie L. Christiansen6, Bruce D. Clarke6,
Santanu Das23, Jean-Michel Dsert10, Michael Endl8, Daniel Fabrycky17, Francois Fressin10,
Michael Haas1, Elliott Horch24, Andrew Howard2, Howard Isaacson2, Hans Kjeldsen7, Jeffery
Kolodziejczak25, Craig Kulesa15, Jie Li6, Philip W. Lucas28, Pavel Machalek6, Donald
McCarthy15, Phillip MacQueen8, Sren Meibom10,, Thibaut Miquel27Andrej Prsa26, Samuel N.
Quinn10,Elisa V. Quintana6, Darin Ragozzine10, William Sherry14, Avi Shporer5, Peter
Tenenbaum6, Guillermo Torres10, Joseph D. Twicken6, Jeffrey Van Cleve6, and Lucianne
Walkowicz2
1
NASA Ames Research Center, Moffett Field, CA 94035, USA
2
University of California, Berkeley, CA, 94720, USA
3
San Jose State University, San Jose, CA, 95192, USA
4
Carnegie Institution of Washington, Washington, DC 20015 USA
5
Las Cumbres Observatory Global Telescope, Goleta, CA 93117, USA
6
SETI Institute, Mountain View, CA, 94043, USA
7
Aarhus University, Aarhus, Denmark
8
McDonald Observatory, University of Texas at Austin, Austin, TX, 78712, USA
9
Lowell Observatory, Flagstaff, AZ, 86001, USA
10
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, 02138, USA
11
Jet Propulsion Laboratory, Calif. Institute of Technology, Pasadena, CA, 91109, USA
12
Space Telescope Science Institute, Baltimore, MD, 21218, USA
13
Lawrence Hall of Science, Berkeley, CA 94720, USA
14
NOAO, Tucson, AZ 85719 USA
15
University of Arizona, Steward Observatory, Tucson, AZ 85721, USA
16
Univ. of Florida, Gainesville, FL, 32611 USA
17
Univ. of Calif., Santa Cruz, CA 95064 USA
18
MIT, Cambridge, MA 02139 USA
19
Fermilab, Batavia, IL 60510 USA
20
San Diego State Univ., San Diego, CA 92182 USA
21
Orbital Sciences Corp., Mountain View, CA 94043 USA
22
Exoplanet Science Institute/Caltech, Pasadena, CA 91125 USA
23
University Affiliated Research Center, University of California, Santa Cruz, CA 95064 USA
24
Southern Connecticut State University, New Haven, CT 06515 USA
25
MSFC, Huntsville, AL 35805 USA
26
Villanova University, Villanova, PA 19085 USA
27
CNES, Toulouse, France
28
Centre for Astrophysics Research, Science & Technology Research
Institute, University of Hertfordshire, Hatfield, UK
0
Correspondence should be addressed to: William Borucki, [e-mail]
1
Abstract. On 1 February 2011 the Kepler Mission released data for 156,453 stars observed from
the beginning of the science observations on 2 May through 16 September 2009. There are 1235
planetary candidates with transit like signatures detected in this period. These are associated with
997 host stars. Distributions of the characteristics of the planetary candidates are separated into
five class-sizes; 68 candidates of approximately Earth-size (Rp < 1.25 R!), 288 super-Earth size
(1.25 R! < Rp < 2 R!), 662 Neptune-size (2 R!, < Rp < 6 R!), 165 Jupiter-size (6 R! < Rp < 15
R!), and 19 up to twice the size of Jupiter (15 R! < Rp < 22 R!). In the temperature range
appropriate for the habitable zone, 54 candidates are found with sizes ranging from Earth-size to
larger than that of Jupiter. Six are less than twice the size of the Earth. Over 74% of the planetary
candidates are smaller than Neptune. The observed number versus size distribution of planetary
candidates increases to a peak at two to three times Earth-size and then declines inversely
proportional to area of the candidate. Our current best estimates of the intrinsic frequencies of
planetary candidates, after correcting for geometric and sensitivity biases, are 5.4% for Earth-size
candidates, 6.8% for super-Earth size candidates, 19.3% for Neptune-size candidates, 2.4% for
Jupiter-size candidates, and 0.15% for very-large candidates; a total of 0.341 candidates per star.
Multi-candidate, transiting systems are frequent; 17% of the host stars have multi-candidate
systems, and 33.9% of all the candidates are part of multi-candidate systems.
Keywords: Exoplanets, Kepler Mission
1. Introduction
Kepler is a Discovery-class mission designed to determine the frequency of Earth-size planets in
and near the habitable zone (HZ) of solar-type stars. Details of the Kepler Mission and instrument
can be found in Koch et al. (2010a), Jenkins et al. (2010c), and Caldwell et al. (2010). All data
through 16 September 2009 are now available through the Multi-Mission Archive (MAST1) at the
Space Telescope Science Institute for analysis by the community.
Based on the first 43 days of data, five exoplanets with sizes between 0.37 and 1.6 Jupiter radii
and orbital periods from 3.2 to 4.9 days were recognized and then confirmed by radial velocity
observations during the 2009 observing season (Borucki et al. 2010, Koch et al. 2010b, Dunham
et al. 2010, Jenkins et al. 2010a, and Latham et al. 2010). Ten more planets orbiting a total of 3
stars have subsequently been announced (Holman et al., 2010, Torres et al. 2011, Batalha et al.
2011, Lissauer et al. 2011a).
Because of great improvements to the data-processing pipeline, many more candidates are much
more visible than in the data used for the papers published in early 2010. When Keplers first
major exoplanet data release occurred on 15 June 2010, 706 targets stars had candidate
exoplanets (Borucki et al. 2011). In this data release we identify 997 stars with a total of 1235
planetary candidates that show transit-like signatures in the first 132 days of data. A list of false
positive events found in the released data is also included in Table 4 with a brief note explaining
the reason for classification as a false positive. All false positives are also archived at the MAST.
A total of 1202 planetary candidates are discussed herein.
1
http://archive.stsci.edu/Kepler/data_search/search.php
2
The algorithm that searches for patterns of planetary transits also finds stars with multiple planet
candidates. A separate paper presents an analysis of five of these candidates (Steffen et al. 2010).
Data and search techniques capable of finding planetary transits are also very sensitive to
eclipsing binary (EB) stars, and indeed the number of EBs discovered with Kepler exceeds the
number of planetary candidates. With more study, some of the current planetary candidates might
also be shown to be EBs and some planetary candidates or planets might be discovered orbiting
some of the EBs. Prsa et al. (2011) present a list of EBs with their basic system parameters that
have been detected in these early data.
2. Description of the Data
Data for all stars are recorded at a cadence of one per 29.4244 minutes (hereafter, long cadence,
or LC). Data for a subset of up to 512 stars are also recorded at a cadence of one per 58.85
seconds (hereafter, short cadence or SC), sufficient to conduct asteroseismic observations needed
for measurements of the stars sizes, masses, and ages. The results presented here are based only
on LC data. For a full discussion of the LC data and their reduction, see Jenkins et al. (2010b,
2010c). See Gilliland et al. (2010) for a discussion of the SC data.
The results discussed in this paper are based on three data segments; the first segment (labeled
Q0) started JD 2544953.53 and ended on 2454963.25 and was taken during commissioning
operations; the second data segment (labeled Q1) taken at the beginning of science operations that
started on JD 2454964.50 and finished on JD 2454997.99 and a third segment (labeled Q2)
starting on JD 2455002.51 and finishing on JD 2455091.48. The durations of the segments are;
9.7, 33.5, and 89.0 days, respectively. The observations span a total period of 137.95 days
including the gaps. A total of 156,097 LC targets in Q1 and 166247 LC and 1492 SC targets were
observed in Q2. The stars observed in Q2 were mainly a superset of those observed in Q1. These
data have been processed with Science Operations Center (SOC) pipeline version 6.2 and
archived at the MAST. Originally, the bulk of these data were scheduled for release on 15 June
2011, but the exoplanet targets are being released early, so 165470 LC and 1478 SC targets will
be publically available to the public on 1 February 2011. The remaining few targets have a
proprietary user other than the Kepler science team (e.g., guest observers). Data for these targets
will become public by 15 June 2011. The current release date and the proprietary owner for each
target are posted at MAST as soon as the data enter the archive, which occurs about four months
after data acquisition for the quarter in question is complete.
The results reported here are for the LC observations of 153,196 stars observed during Q2. Other
stars were giants or super-giants, did not have valid parameter values, or were in some way
inappropriate to the discussion of the exoplanet search. The enlarged set of stars observed in Q2
included most of the stars observed in Q1and additional stars due to the more efficient use of the
available pixels. The selected stars are primarily main sequence dwarfs chosen from the Kepler
Input Catalog27 (KIC). Targets were chosen to maximize the number that were both bright and
small enough to show detectable transit signals for small planets in and near the habitable zone
(HZ) (Gould et al. 2003, Batalha et al. 2010a). Most stars were in the Kepler magnitude range 9 <
Kp < 16. The Kepler passband covers both the V and R photometric passbands (Figure 1 in Koch
et al. 2010a). See the discussion in Batalha et al. (2010b).
27
http://archive.stsci.edu/Kepler/Kepler_fov/search.php
3
2.1 Noise Sources in the Data
The Kepler photometric data contain a wide variety of both random and systematic noise sources.
These sources and others are discussed in Jenkins et al. (2010b) and Caldwell et al. (2010). Work
is underway to improve the mitigation and flagging of the affected data. Stellar variability over
the periods similar to transit durations is also a major source of noise.
Because of the complexity of the various small effects that are important to the quality of the
Kepler data, prospective users of Kepler data are strongly urged to study the data release notes
(available at the MAST) for the data sets they intend to use. Note that the Kepler data analysis
pipeline was designed to perform differential photometry to detect planetary transits, so other
uses of the data products require caution.
2.2 Distinguishing Planetary Candidates from False Positive Events
The search for planets starts with a search of the time series of each star for a pattern that exceeds
a detection threshold commensurate with a non-random event. Observed patterns of transits
consistent with those from a planet transiting its host star are labeled planetary candidates. (In a
few cases, a single drop in brightness that had a high SNR and was of the form of a transit was
sufficient to identify a planetary candidate.) Those that were at one time considered to be
planetary candidates but subsequently failed some consistency test are labeled false positives.
After passing all consistency tests described below, and only after a review of all the evidence by
the entire Kepler Science Team, does the candidate become a confirmed or validated exoplanet.
Steps such as high-precision radial velocity (RV) measurements (Borucki et al. 2010, Koch et al.
2010b, Dunham et al. 2010, Jenkins et al. 2010a, and Latham et al. 2010), or transit timing
variations (Holman et al 2010, Lissauer et al. 2011a) are used when practical. When such
methods cannot be used to confirm an exoplanet, an extensive analysis of spacecraft and groundbased data may allow validation of an exoplanet by showing that the planetary interpretation is at
least 100 times as probable as a false positive (Torres et al. 2011, Lissauer et al. 2011a). This
paper does not attempt to promote the candidates discussed herein to validated or confirmed
exoplanets, but rather documents the full set of current candidates and the many levels of steps
toward eventual validation, or in some cases, rejection as a planet that have been taken.
There are two general causes of false positive events in the Kepler data that must be evaluated
and excluded before a candidate planet can be considered a valid discovery: 1) statistical
fluctuations or systematic variations in the time series, and 2) astrophysical phenomena that
produce similar signals. A sufficiently high detection threshold (i.e., 7.1 !) was chosen such that
the totality of data from Q0 thru Q5 (end date JD 2455371.170) provides an expectation of fewer
than one false positive event due to statistical fluctuations over the ensemble of all stars for entire
mission duration. Similarly, systematic variations in the data have been interpreted in a
conservative manner and should result in false positives only rarely. However, astrophysical
phenomena that produce transit-like signals are common.
2.2.1 Search for False Positives in the Output of the Data Pipeline
The Transiting Planet Search (TPS) pipeline searches through each systematic error-corrected
flux time series for periodic sequences of negative pulses corresponding to transit signatures. The
approach is a wavelet-based, adaptive matched filter that characterizes the power spectral density
(PSD) of the background process yielding the observed light curve and uses this time-variable
PSD estimate to realize a pre-whitening filter and whiten the light curve (Jenkins 2002, Jenkins et
al. 2010c,d). TPS then convolves a transit waveform, whitened by the same pre-whitening filter
as the data, with the whitened data to obtain a time series of single event statistics. These
represent the likelihood that a transit of that duration is present at each time step. The single event
statistics are combined into multiple event statistics by folding them at trial orbital periods
4
ranging from 0.5 days to as long as one quarter (~93 days) of a spacecraft year. Every quarter
year, the spacecraft must be rotated 90 degrees to keep the solar panels pointed at the Sun. This
rotation put the images of the stars on a different set of detectors and resets the photometric
values. Automated identification of candidates with periods longer than one quarter will be done
by the pipeline in the coming months, but is currently done by ad hoc methods. The ad hoc
methods produced many of the Kepler-Object-of-Interests (KOI) with numbers larger than 1000,
but might cause a bias against candidates with periods longer than one quarter. For a more
comprehensive discussion of the data analysis, see Wu et al (2010) and Batalha et al (2010b).
After automatic identification with TPS or ad hoc detection of longer period candidates, the light
curves of potential planet candidates were modeled and examined by eye to determine the gross
viability of the candidate. If the potential candidate was not an obvious variable star or eclipsing
binary showing significant ellipsoidal variation the candidate was elevated to Kepler Object of
Interest (KOI) status, given a KOI number (see section 3.1) and was subjected to tests described
in the next paragraphs. After passing these tests, the KOI is forwarded to the Follow-up
Observation Program (FOP) for various types of observations and additional analysis. See the
discussion in Gautier et al. (2010) and Bryson et al. (2011).
Using these estimates and information about the star from the KIC, tests are performed to search
for a difference in even- and odd-numbered event depths. If a significant difference exists, this
suggests that a comparable-brightness EB has been found for which the true period is twice the
period initially determined due to the presence of primary and secondary eclipses. Similarly, a
search is conducted for evidence of a secondary eclipse or a possible planetary occultation
roughly halfway between the potential transits. If a secondary eclipse is seen, then this could
indicate that the system is an EB with the period assumed. However, the possibility of a selfluminous planet (as with HAT-P-7; Borucki et al. 2009) must be considered before dismissing a
candidate as a false positive.
Many false positives due to background eclipsing binaries (BGEBs) are not detected by the
pipeline techniques described above, for example if their secondary transit signals are so weak
that they are lost in the noise. The term eclipsing binaries, as distinct from BGEBs, are
gravitationally-bound, multi-star targets and are usually detected by the secondary eclipse or RV
observations. To detect BGEBs, a very sensitive validation technique is used on all candidates to
determine the relative position of the image centroid during and outside of the transit epoch. The
shift in the centroid position of the target star measured in and out of the transits must be
consistent with that predicted from the fluxes and locations of the target and nearby stars. (See
Bryson et al. 2011.) In particular, a post-processing examination uses an average difference image
formed by subtracting the pixels during transit from the pixels out of transit. A pixel response
function fit to this difference image provides a direct sub-pixel measurement of the transit source
location on the sky (Torres et al. 2011). When the measured position of the transit source does not
coincide with the target star the most common cause will be a BGEB false positive, although for
strongly blended targets in the direct image further analysis is necessary to support this rejection.
This analysis of centroid motion is capable of identifying BGEBs as close as about 1 arcsecond
to the target star in favorable circumstances, even with Kepler's 4-arcsecond pixel scale.
Centroid analysis is conducted for each candidate that is unsaturated in the Kepler observations
and follow-up observations by AO and speckle imaging of the area near the target star are carried
out for many candidates. adaptive optics (AO) observations in the infrared were conducted at the
5-m at Palomar Observatory and the 6.5 m at the MMT with ARIES; speckle observations were
obtained at the WIYN 3.5m telescope. However, the area behind and immediately surrounding
the star, can conceal a BGEB that could imitate a candidate signature. The area that could conceal
5
an EB varies with brightness of the target star because of photon noise limitations to AO and
speckle searches, but is of order 1 square arc sec. Model estimates of the a priori probability that
an EB is present in the magnitude range that could mimic the transit signal range from 10-6 to 10-4.
Thus the estimated number of target star locations that might have an EB too close to the star to
be detected by AO or speckle imaging is 0.1 to 10 based on observations of 150,000 stars.
A much more comprehensive and intensive analysis has been done for the candidates listed here
than was done for the data released in June 2010 (Borucki et al. 2011). Consequently the fraction
of the candidates that are false positives in the active candidate list should be substantially smaller
than the earlier estimate.
2.2.2 Estimate of false positive rate
While many of the candidates have been vetted through the steps described above, the process of
determining the residual false positive fraction for Kepler candidates at various stages in the
validation process has not proceeded far enough to make good quantitative statements about the
expected true planet fraction, or reliability, of the released list. However, we can make rough
estimates of the quality of the vetting that the KOIs have had. Several groups of KOIs in Table 2
are distinguished by the FOP ranking flag. These groups have had different levels of scrutiny for
false positives and will therefore have different expectations for reliability.
KOIs with ranking of 1 are validated and published planets with expected reliability above 98%.
We are reluctant to state a higher reliability since unforeseen issues have led to retractions of
apparently well-established planets in other planet detection programs.
KOIs with rankings of 2 and 3 have been subject to thorough analysis of their light curves to look
for signs of eclipsing binary origin, analysis of centroid motion to detect BGEBs confused with
their target stars, and varying degrees of spectroscopic and imaging follow-up observation from
ground and space based observatories. These analyses and follow-up observations are generally
sufficient to eliminate many stellar mass objects at or near the location of the target star as the
source of the transit signal. A ranking of 2 means that none of the results argued against the
planet interpretation. A ranking of 3 means that some of the results were suspicious enough to
warrant caution but did not unambiguously rule out the planet interpretation. The criteria are
subjective and are not meant to be quantitative. The main sources of unreliability, false positives
among the rank 2 and 3 KOIs are likely to be from BGEBs with angular separation from the
target star too small to be detected by our centroid motion analysis, grazing eclipses in binary
systems, and eclipsing stars in hierarchical multiple systems where transits by stellar companions
and giant planets dilute the light of other system components. Note that spectroscopy, even at low
signal-to-noise such as the reconnaissance spectra we are pursuing, easily rules out grazing
eclipsing binaries, as they would show RV variations of tens of km/s. However, those KOIs in
Table 2 without a flag=1 in the FOP column did not have such spectroscopy, leaving open the
possibility of such grazing eclipsing binaries.
For bright unsaturated stars with Kp " 11.5 and transit depths strong enough to provide overall
detection significances of 20! and more, the minimum angular separation for the current centroid
motion analysis is about 1 arcsec. This limit becomes significantly larger for fainter stars and/or
low-amplitude transit signals associated with smaller planets. For these signal levels, the transit
significance of ~10! supports a centroid motion analysis constraint on the inner detection limit of
about 3 arcsec. These minimum detection angles of 1 to 3 arcsecs are quoted as 3! angles beyond
which high confidence of discriminating against BGEBs exists. High resolution imaging provided
additional reduction of the effective the minimum detection angle for about 100 of the rank 2
6
KOIs. We expect 10% of the BGEBs to remain in the rank 2 list. KOIs were given a rank of 3
when the centroid motion analysis or follow-up spectroscopy was ambiguous so that the KOI
could not be definitely declared a false positive. We estimate that as many as 30% false positives
could remain among the rank 3 KOIs.
About 12% of star systems in the solar neighborhood are found to be triple, or of higher
multiplicity, hierarchical systems (Raghavan et al. 2010), so a similar fraction is expected to
appear in the Kepler target list. Only a small percentage of the hierarchical systems will produce
eclipses that are seen by Kepler and many of these signals can be identified as binary star eclipses
by examination of their light curves. From the rare occurrence rate of EBs and the also rare
occurrence rate of triple star systems, the fraction of KOIs that are triple-star systems with an EB
is expected to be less than 5%.
A potentially more frequent type of misidentification in a hierarchical system is a planet transiting
in a binary system. If the double nature of the star system is not identified, dilution of the
planetary transit by the second star will result in miscalculation of the planet size. Raghavan et
al. (2010) give the binary star system fraction as 34%, but little is yet known about the frequency
of planets in binary systems and, again, only a small fraction of planets in binary systems will
transit because the orbital planes of the planets are expected to be coplanar with the orbital plane
of the stars. Adopting Raghavan et al.'s occurrence rate of binary stars, and assuming that the
typical number of planets per star system doesn't depend on the multiplicity of the system, we
expect that up to 34% of the KOIs represent planets of larger radius than indicated in Table 2.
The distribution of the amounts of dilution cannot be easily determined as it depends on two
effects, namely the distribution of the ratio of star brightnesses and the distribution of planet sizes
that transit one (or the other) of the two stars in the binary system. Estimating these planet-transit
effects in binary systems requires knowledge of the systematic dependence of planet size on
orbital distance, a chicken-and-egg problem that we cannot easily resolve at present. For binaries
in which the transiting planet orbits the primary star, the dilution will be less than 50% flux. But
for binaries in which the transiting object (planet or star) orbits the fainter secondary star, the
transiting object's radius can be arbitrarily larger than that stated in Table 2.
Considering all sources of remaining false positives we expect the list of rank 2 KOIs to be >80%
reliable and the rank 3 list to be >60% reliable. A careful assessment of false positive scenarios,
especially background and gravitationally bound eclipsing binaries and planets, suggests that 90%
to 95% of the Kepler planet candidates are indeed true planets (Morton & Johnson 2011). This
agrees with our best estimates.
Rank 4 KOIs have had scant examination of their light curves and no follow-up observation and
were therefore subject only to centroid motion analysis. We expect the reliability of rank 4 KOIs
to be similar to that of rank 3.
2.2.3 Development of a model to estimate the probability of an EB near the position of a
candidate.
Low-mass planets, especially those in long-period orbits within the habitable zone, have low
amplitude RV signal levels that are often too small to be confirmed by current Doppler
observation capabilities. Consequently, validation must be accomplished by the series of steps
outlined above. An estimate is also made of the probability that an EB is present that is too near
the target star to detect by AO, speckle imaging, or centroid motion. The area number density
(number per solid angle) of EBs is calculated based on the assumption that the number of EBs to
the number of background stars is constant near the position of each target star. Because the area
7
number density varies rapidly with Galactic latitude and because the Kepler field-of-view (FOV)
covers over 10 of latitude, predictions of the EB density also vary greatly over the FOV.
Consequently, a model was constructed to estimate the probability per square arcsec that an EB is
present in the magnitude range that would provide a signal with an amplitude similar to that of
the candidate and at the position of each target star. The model is based on the fraction of stars
observed by Kepler to be binary (Prsa et al. 2011), and it uses the number and magnitude
distributions of stars from the Besancon model after correction from the V band to the Kepler
passband. The value of the probability that there is a BGEB at the location of the target star is
listed in Table 2 for each candidate.
3. Results
The characteristics of the host stars and the candidates are summarized in Tables 1 and 2,
respectively. A total of 1235 KOIs were found in the Q0 through Q2 data. Table 3 provides short
notes on many of these KOIs. Table 4 lists the 511 candidates considered to be false positives;
comments are included. The false positives have been removed from the list of candidates in
Table 2 and are not used in the distributions discussed here. The 15 candidates with a diameter
over twice that of Jupiter, and thus larger than late M dwarf stars, were also removed from
discussion. This leaves a total of 1235 -18 single-transit candidates -15 candidates greater than
twice the size of Jupiter = 1202 candidates for consideration in this discussion.
To provide the most accurate predictions for future observations, the values for the epoch and
orbital period given in Table 2 are derived from all data currently available to the Kepler team;
i.e., data obtained through Q5 (from JD 2455276.481 through JD 2455371.170) were used. For
some candidates, reconnaissance spectra were taken with moderate exposures to look for doubleand single-lined binaries. They are most useful in finding outliers for the stellar temperatures and
log g listed in the KIC. Adaptive optics and speckle observations were taken to check for the
presence of faint nearby stars that could be BGEBs or that could dilute the signal level. Flags also
indicate the particularly interesting candidates for which radial velocity (RV) measurements of
extremely high precision (~ 2 m/s) or high precision (~ 10 m/s) observations were obtained. The
last column of Table 2 indicates whether a note is available about that candidate in Table 3. For
consistency, all values of the stellar parameters are derived from the KIC.
3.1 Naming Convention
To avoid confusion in naming the target stars, host stars, planetary candidates, and
confirmed/validated planets, the following naming convention has been used. Kepler stars are
referred to as KIC NNNNNNN (with a space between the KIC and the number), where the
integer refers to the ID in the Kepler Input Catalog archived at MAST. Confirmed planets are
named Kepler followed by a hyphen, a number for the planetary system, and a letter designating
the first, second, etc. confirmed planet as b, c, etc., for example Kepler-4b. Candidates are
labeled Kepler Object of Interest (KOI) followed by a decimal number. The two digits beyond
the decimal provide identification of the candidates when more than one is found for a given star,
e.g., KOI NNN.01, KOI NNN.02, KOI NNN.03, etc. For example KOI 377.03, the third transit
candidate identified around star KOI 377, became Kepler-9d after validation as a planet (Torres et
al. 2011). KOI numbers are always cross-referenced to a KIC ID. For a multi-candidate system
these digits beyond the decimal indicate the order in which the candidates were identified by the
analysis pipelines and are not necessarily in order of orbital period. It should be noted that the
KOI list is not contiguous and not all integers have an associated KOI.
8
3.2 Statistical Properties of Planet Candidates
We conducted a statistical analysis of the 1202 candidates to investigate the general trends and
initial indications of the characteristics of the planetary candidates. The list of candidates was
augmented with known planets in the field of view. In particular, TrES-2, HAT-P7b, HAT-P11b,
(Kepler-1b, -2b, -3b, respectively), Kepler-4b-8b (Borucki et al. 2010, Koch et al. 2010b,
Dunham et al. 2010, Latham et al. 2010, and Jenkins et al. 2010). Kepler-9bcd (Holman et al.
2010, Torres et al. 2011), Kepler-10b (Batalha et al. 2011), and Kepler-11b-g (Lissauer et al.
2011a) were included. However one candidate identified by a guest observer (KOI 824.01) is
included in the list of candidates but is not used in the graphs and statistics because it wasnt in
the range of parameters chosen for the search. As noted above, not all candidates appearing in
Table 2 were used in the statistical analysis or in the graphical associations shown in the figures:
specifically, candidates greater than twice the size of Jupiter, those that showed only one transit in
the Q0/Q2 data but no others in the succeeding observations, and those orbiting stars larger than
10 solar radii or with temperatures in excess of 9500 K were excluded. Comparisons are limited
to orbital periods of " 138 days. The figures are indicative of the properties and associations of
candidates with various parameters, but are not meant to be definitive.
The readers are cautioned that the sample is affected by many poorly quantified biases. Obviously
some of the released candidates could be false positives, but other characteristics such as stellar
radius, magnitude, noise spectrum, and analysis protocols can all play significant roles in the
statistical results. Nevertheless, the large number of candidates provides interesting, albeit
tentative, associations with stellar properties. No correction is made to the frequency plots due to
the linearly decreasing probability of a second transit occurring during the Q0 through Q2 period.
This correction is not needed because data for following quarters were used to calculate the
epochs and periods for all candidates that showed at least one transit in the Q0 through Q2 period
and at least one in the subsequent observations.. In the figures below, the distributions of various
parameters are plotted and compared with values in the literature and those selected from the
Extrasolar Planets Encyclopedia2 (EPE; values as of 7 December 2010). We consulted the
literature to identify those planets discovered by the RV method and excluded those discovered
by the transit method. This step avoids biasing the RV-discovered planets with the short-period
planets that are often found by the transit method.
The results discussed here are primarily based on the observations of stars with Kp < 16, with
effective temperature below 9500 K, and with size less than ten times the solar radius. The latter
condition is imposed because the photometric precision is insufficient to find Jupiter-size and
smaller planets orbiting stars with 100 times the area of the Sun. Stellar parameters are based on
KIC data. The function of the KIC was to provide a target sample with a high fraction of dwarf
stars that are suitable for transit work, and to provide a first estimate of stellar parameters that is
intended to be refined spectroscopically for KOI targets at a later time. Although postidentification reconnaissance spectroscopic observations have been made for more than half of
the stars with candidates, it is important to recognize that some of the characteristics listed for the
stars are still uncertain, especially surface gravity (i.e., log g) and metallicity ([M/H]). The errors
in the stellar diameters can reach 25%, with proportional changes to the estimated diameter of the
candidates.
In Figure 1, the stellar distributions of magnitude and effective temperature are given for
reference. In later figures, the association of the candidates with these properties is examined.
2
Extrasolar Planet Encyclopedia; http://exoplanet.eu/
9
Figure 1. Distributions of effective temperature and magnitude for the stars observed during Q2 and
considered in this study. Bin size for left panel is 500 K. The bin size for right hand panel is one magnitude
from 6 to 9 and 0.25 mag from 9 to 16.5.
It is clear from the left panel in Figure 1 that most of the stars monitored by Kepler have
temperatures between 4000 and 6500 K; they are mostly late F, G and K spectral types. Because
of their faintness, only 2510 stars cooler than 4000 K (i.e., dwarf stars of spectral type M) were
monitored. Although cooler stars are more abundant, hotter stars are the most frequently seen for
a magnitude-limited survey of dwarfs.
The selection of target stars was purposefully skewed to enhance the detectability of Earth-size
planets by choosing those stars with an effective temperature and magnitude that maximized the
transit signal-to-noise ratio (SNR) (Batalha et al. 2010b). The step decrease seen in the right hand
panel of Figure 1 at Kepler magnitude (Kp) equal 14.0 and the turnover near Kp = 15.5, seen in
the right hand panel of figure 1, are due to the selection of only those stars in the FOV that are
bright enough and small enough to show terrestrial-size planets. After all available bright dwarf
stars were chosen for the target list, many target slots remained, but only stars fainter than Kp=14
were available (Batalha et al. 2010b). From the fainter stars the smallest stars are given
preference. At the lower left of the right hand chart, the bin size has been increased to show the
small number of candidates brighter than Kp = 9. In the following figures, the bias introduced by
the selection of stellar size- and magnitude distributions must always be considered.
10
Figure 2. Size distribution of the number of Kepler candidates vs. planet radius (Rp) (upper panel). The
logarithm of the number of candidates is presented in the lower panel to better show the tail of the
distribution. Bin sizes in both panels are 1 R!.
As noted in Borucki et al. (2011), the results shown in Figure 2 imply that small candidate planets
are much more common than large candidate planets. Of the 1202 candidates considered for the
analysis, 74% are smaller than Neptune (Rp= 3.8 R!). Table 6 shows the observed distribution and
the definition of sizes used throughout the paper for these 1202 candidates.
The dashed curve in both panels of Figure 2 represents a 1/(Rp-2 dependence of the number of
candidates on candidate radius; i.e., dN/dr scales as
for 2R! <Rp <15 R!. The data shown
here are restricted to orbital periods " 138 days. Because it is much easier to detect larger
candidates than smaller ones, this result implies that the frequency of candidates decreases with
the area of the candidate, assuming that the false positive rate, completeness, and other biases are
independent of candidate size for candidates larger than 2 Earth radii. However, the current
survey is not complete, especially for the fainter stars, smallest candidates, and long orbital
periods, and further observations could influence the distribution.
11
Figure 3. Candidate size versus orbital period, semi-major axis, stellar temperature, and candidate
equilibrium temperature3. Uncertainties in candidate size are mostly due to the uncertainty in stellar sizes,
i.e., approximately 25%. Horizontal lines mark ratios of candidate sizes for Earth-size, Neptune-size , and
Jupiter-size relative to Earth-size.
Figure 3 presents scatter plots showing the observed relative size of individual candidates versus
orbital period, semi-major axis, stellar temperature, and candidate temperature. The values on the
abcissa are limited to show only the most populous range. Outliers can be found in Table 2. The
upper left panel shows a concentration (in log-log space) of candidates for orbital periods
between 3 and 30 days and sizes between 1 and 4 R!. The upper right panel shows a similar
concentration. Both of them show a nearly empty area to the lower right that likely represents the
lack of small candidates caused by the lower detectability of small candidates in long period
orbits.
All panels in Figure 3 show a scarcity of candidates with radius Rp smaller than 1 R!. The paucity
of small candidates at even the shortest orbital periods could be due to incompleteness for the
smaller signals, coupled with analysis of only a portion of the eventually expected Kepler data,
and higher than expected noise levels. These effects could mask a real dependence of number on
size. The modestly higher noise levels than those anticipated are thought to follow primarily from
an underestimate of intrinsic stellar noise and are the topic of an on-going study.
3
Teq was derived by assuming an even distribution of heat from the day to night side of the
planet(e.g., a planet with an atmosphere or a planet with rotation period shorter than the orbital period)
and the planet and star actas blackbodies in equilibrium; \begin{equation}\label{eq:teq}
T_{eq}=T_* (R_*/2a)^{1/2} [f(1-A_B)]^{1/4}, \end{equation} where $T_*$ and $R_*$ are the
effective temperature and radius of the host star, the planet at distance $a$ with a Bond albedo of $A_B$
and $f$ is a proxy for atmospheric thermal circulation. The Bond albedo, $A_B$, is the fraction of total
power incident on a body scattered back into space which we assume to be 30\% and $f=1$ indicates full
thermal circulation.
12
Figure 4 expands that portion of the lower right panel to emphasize those candidates with
estimated radiative equilibrium temperatures in the range of liquid water at a pressure of 1 bar.
Figure 4. Candidate sizes and estimated radiative equilibrium temperatures (Teq) centered on the habitable
zone temperature range. The dotted lines bracket the range of temperatures allowing water to exist as a
liquid at one atmosphere of pressure. Uncertainties are discussed in the text.
The habitable zone (HZ) is often defined to be that region around a star where a rocky planet with
an Earth-like atmosphere could have a surface temperature between the freezing point and boiling
point of water, or analogously the region receiving roughly the same insolation as the Earth from
the Sun (Kasting et al.1993, Rampino and Caldeira 1994, Heath et al. 1999, Joshi 2003, Tarter et
al. 2007). The surface temperature range for habitable zones is likely to include radiative
equilibrium temperatures well below 273 K because of warming by any atmosphere that might be
present. For example, the greenhouse effect raises the Earths surface temperature by 33 K and
that of Venus by approximately 500 K. Further, the spectral characteristics of the stellar flux vary
strongly with Teff and affect both the atmospheric composition and the chemistry of
photosynthesis (Heath et al. 1999, Segura et al. 2005). Consequently, Figure 4 shows
temperatures well below the freezing point of water. The vertical lines at 183 and 307 K delineate
the radiative temperature range for which the surface temperature of a rocky planet with an
atmosphere similar to that of the Earth is expected to be within the freezing and boiling point of
water (Jim Kasting, private communication, 2/28/2011).
The calculated equilibrium temperatures shown in Figure 4 are for grey-body spheres without
atmospheres. The calculations assume a Bond albedo of 0.3, emissivity of 0.9, and a uniform
surface temperature. The uncertainty in the computed equilibrium temperatures is approximately
13
22% (see Appendix) because of uncertainties in the stellar size, mass, and temperature as well as
the planetary albedo. For planets with an atmosphere, the surface temperature would be higher
than the radiative equilibrium temperature.
Within this temperature range, there are 54 candidates are present with sizes ranging from Earthsize to larger than that of Jupiter. Table 5 lists the candidates in the HZ. The detection of Earthsize candidates depends on the signal level, which in turn depends on the size of the candidate
relative to the size of the star, the number of transits observed, and the combined noise of the star
and the instrument. It is important to recognize that the size of the star is generally not well
characterized until spectroscopic studies and analysis are completed. In particular, some of the
cooler stars could be nearly double the size shown in Table 1 and that some of the candidates
could prove to be false positives.
As can be seen in Table 5, there are two candidates with Rp < 1.5 R! (KOI 314.02 and KOI
326.01) present in the list. The uncertainty in the sizes of these candidates is approximately 25%
to 35% due to the uncertainty in size of stars and of the transit depth.
The predicted semi-amplitudes of the RV signals for small candidates such as KOI 314.02 and
326.01 are 1.2 m/s and 0.5 m/s, respectively. These RV amplitudes follow from assuming a
circular orbit and a density of 5.5 g/cm3 for both candidates. RV semi-amplitudes of 1.0 m/s are at
the very limit of what might currently be possible to detect with the largest telescopes and best
spectrometers. In principle, RV amplitudes under 1 m/s could be detected, but there are many
impediments to achieving such precision including the surface velocity fields (turbulence) and
spots on the rotating surface. In addition, stars with one transiting planet may well harbor
multiple additional planets that do not transit, causing additional RV variations. Moreover, these
two stars have V-band magnitudes of 14, making it very difficult to acquire sufficient photons in
a high resolution spectrum to achieve the required Doppler precision. Of course, for all of these
small planets RV measurements can place firm upper limits to their masses and densities.
Table 6. Number of Candidates versus Size.
Candidate Label
Candidate Size
Number of
( R !)
Candidates plus
known planets
Earth-size
Rp "1.25
68
super-Earth-size
1.25 < Rp " 2.0
288
Neptune-size
2.0 < Rp " 6.0
662
Jupiter-size
6.0 < Rp " 15
165
very-Large-size
15.0 < Rp " 22.4
19
Not considered
Rp > 22.4
15
14
Figure 5. Upper panel: Historgrams of the observed number of candidates vs. linear intervals in the semimajor axis. The dashed line shows the relative effect of geometricical probability of alignment Lower
panel: The number of candidates vs. logarithmic intervals of the semi-major axis. Bin size is 0.02 AU in
the upper panel and 0.1 in the lower panel.
In Figure 5, the dependence of the number of candidates on the semi-major axis is examined. For
a less than 0.04 AU, it is evident that the distribution is severely truncated. As is evident in
Figure 5, this feature is present in each of the candidate size groups. In the upper panel of Figure
5, an analytic curve shows the expected reduction in the number in each interval due to the
decreasing geometrical probability that orbits are aligned with the line-of-sight. It has been
scaled over the range of semi-major axis from 0.04 to 0.5 AU, corresponding to orbital periods
from 3 days to 138 days for a solar-mass star. The fit is fair-to-poor implying that the intrinsic
distribution is not constant with semi-major axis after a correction only for the alignment
probability.
15
Figure 6. Number of candidates vs orbital period for several choices of candidate size. Bin size is 2 days.
Refer to Table 6 for the definition of each size category.
The panels in Figure 6 show that the period distribution of Neptune-size candidates has a less
steep slope compared to Jupiter-size candidates in the period range from one week to one month.
Because of the large numbers in both samples and the ease of detecting such large candidates, the
difference in the dependence of number on semi-major axis is likely to be real. All show maxima
in the number of candidates for orbital periods between 2 to 5 days for all sizes and a narrow dip
at periods shorter than two days. (The small number of very-Large candidates might be the
reason for the lack of a local minimum at the shortest orbital periods.) However these objects are
as large as late M-dwarf stars and it is unclear what type of object they represent. Determination
of their masses with RV techniques is clearly warranted because the results would not only
provide masses, but densities as well when combined with the transit results.
16
Figure 7. Number of observed candidates versus semi-major axis for four candidate size ranges. As defined
in Table 6, Earth-size refers to Rp < 1.25 R!, super-Earth-size to 1.25 R! < Rp < 2 R!, Neptune-size to 2
R!, < Rp < 6 R!, and Jupiter-size refers to 6 R! < Rp < 15 R!. Bin size for the semi-major axis is 0.04
AU.
A breakout of the number of candidates versus semi-major axis is shown in Figure 7 using the
definition for size in Table 6. Earth-size candidates and some of the super-Earth-size
candidates are expected to be rocky type planets without a hydrogen-helium atmosphere.
Neptune-size candidates could be similar to Neptune and the ice giants in composition. All size
classes show a rise in the number of candidates for decreasing semi-major axis until a value of
0.04 AU and then a steep drop. The drop off in the number of Earth-size candidates for semimajor axes greater than 0.2AU is due at least in part to the decreasing probability of a favorable
geometrical alignment and the difficulty of detecting small planets when only a few transits are
available.
17
Figure 8. (Upper panel) Observed period distribution of Kepler planet candidates with orbital periods
less than 125 days, uncorrected for observational selection effects. (Lower panel) Period distribution over
the same range for RV-discovered planets listed in the Extrasolar Planet Encyclopedia (EPE) as of 7 Dec
2010 exclusive of Kepler planets. Bin size is 2 days.
Figure 8 compares the orbital period distribution of the Kepler planet candidates with the planets
discovered by the RV method (as reported by the EPE.) Both detection methods show a
prominent peak in the numbers for periods between two and four days and a large drop in the
number for shorter periods. There are several references in the literature to the pile-up of giant
planet orbital periods near 3 days (e.g. Santos and Mayor 2003). It is suggestive of a process that
allows planets migrating inward to synchronize their orbital period with the rotation period of the
star, raise tides of sufficient strength that enough momentum is transferred to the planet to halt its
migration. Later, the star becomes sufficiently luminous that the dust and gas of the accretion disk
are expelled leaving the planet in a stable, but short-period orbit. The cause of the much larger
relative decrease seen in the RV-discovered planets compared to that seen in the Kepler results is
not understood.
The planetary candidates observed at shorter distances could represent those that did not come
into synchronism with the star, but stopped short of entering the stars atmosphere because a
coincidence with the dissipation of the accretion disk. They could also represent a continued
migration of the body into the star.
18
Figure 9. Observed distribution of candidate sizes for four ranges of orbital period, uncorrected for
selection effects. Panels 2, 3, & 4 compare the distributions for longer periods with that of the shortest
period range. Bin size is 2 R!.
Except for the peak between 2 to 4 R!, Figure 9 shows that the number of short-period (< 3 days)
candidates is nearly independent of candidate size through 16 R!. However, small candidates are
more numerous than large ones for longer orbital periods. This distribution suggests that shortperiod candidates might represent a different population than the populations at larger orbital
periods and semi-major axes. In particular, they might represent rocky planets and the remnant
cores of ice giants and gas giant planets that have lost their atmospheres. To confirm that this
population is distinct from that of longer-period candidates will require a future investigation of
the comparison of the mass-radius relationships of the populations.
19
Figure 10. Observed frequencies, uncorrected for selection effects, of candidates for five size ranges
defined in Table 6 as a function of Kepler magnitude. The error bars represent only the Poisson noise
associated with the number of events in each bin, and the upper bar represents a single event if no events
are observed.
In Figure 10, the observed frequency of candidates in each magnitude bin has been simply
calculated from the number of candidates in each bin divided by the total number of stars
20
monitored in each bin. The number of stars brighter than Kp = 9.0 or fainter than Kp = 16.0 in the
current list is so small that the count is not shown.
The panels for Earth-size and super-Earth size candidates are consistent with a decrease in the
observed frequency with increasing magnitude for magnitudes larger than Kp=11, and are
indicative of difficulty in detecting small candidates around faint stars. Near-constant values of
observed frequencies of the Neptune-size and larger candidates would be expected if the survey
were mostly complete for the large candidates and for the orbital periods reported here and if the
distribution of stellar types is independent of apparent magnitude. However, almost all M-dwarf
stars in the Kepler FOV have Kp>14. Therefore if the frequency of large candidates around Mdwarfs is different than for other spectral types, then near-constant frequencies of Neptune- and
larger-size candidates should not be expected. Perhaps the apparent decrease with increasing
magnitude is due to this cause.
An examination of the upper left panel of Figure 10 indicates that several Earth-size candidates
must be present in the 15th to 16th magnitude bin. The noise properties of the instrument are such
that only the smallest stars or small stars with short-period candidates can appear in this bin. To
get a measure of the variation of the observed frequency distributions with magnitude when the
transit amplitude is held nearly constant, the distributions for five ranges of the ratio Rp /R* are
displayed in Figure 11.
21
Figure 11. Frequency distribution (not corrected for selection effects) for 5 ranges of the ratio of the radius
of the candidate to that of the host star versus magnitude.
The five ratios shown in Figure 11 are appropriate for Earth-size, super-Earth-size, Neptune-size,
Jupiter-size, and very-Large-size candidates transiting stars of radius R!= 1 R!, where the
subscript ! signifies solar values. An examination of the upper left hand panel shows no
candidates are found for the 15 to 16 magnitude range. The Earth-size candidates around faint
stars (Kp>15) shown in the upper left panel of Figure 10 orbit small stars and have a planet-star
radius ratio greater than 0.0115. Thus they no longer appear in the upper left panel of Figure 11.
The observed frequency distributions show a steeper decrease with increasing magnitude for the
small Rp/R* shown in the two upper panels. The panels in the second row again show a nearly
constant frequency with magnitude implying that such signal levels are readily detected over the
magnitude range of interest. Contrary to what might be expected, a nearly constant frequency
with magnitude is not seen for the largest ratio-range. This result is not understood.
22
Figure 12. Observed number of candidates for various candidate sizes vs. stellar effective temperature,
uncorrected for selection effects. Bin size is 500K. Refer to Table 6 for the definition of each size
category.
The number of candidates is a maximum for stars with temperatures between 5000 and 6000 K,
i.e., G-type dwarfs (Figure 12). This result should be expected because the selection process
explicitly emphasized these stars and because G-type stars are a large component of magnitudelimited surveys of dwarfs at the magnitudes of interest to the Kepler Mission.
To reduce the bias associated with the large fraction of K, G, and F type stars, the number of
candidates in each bin was normalized to the number of star in the bin and frequencies calculated
as a function of stellar temperature. However, because of the narrow-width temperature bins,
many of the bins have a very small number of candidates which cause the frequencies to vary
widely due to small-number statistics. To increase the number in each bin and reduce the large
variations associated with small-number statistics, the bins in Figure 13 are twice as large as those
in Figure 12.
23
Figure 13. Measured frequency of candidates versus stellar temperature. The error bars shown with the
distributions represents only that portion of the uncertainty due to Poisson noise. Bin size is 1000 K. Refer
to Table 6 for the definition of each size category.
In Figure 13, a comparison of the frequencies of super-Earth-size and Neptune-size candidates
shows an indication that candidates are preferentially found around stars cooler than 4000K. A
similar distribution is also found for Earth-size candidates, but because of the very small number
of candidates in that bin (i.e., 2), the maximum is not statistically significant. Main sequence stars
with temperatures between 3000 K and 4000 K are classified as M-dwarfs. Giant and super-giant
late K spectral-type stars are both more massive and larger than the M-dwarfs but have similar
temperatures. A check of the KIC showed that none of the candidates were associated with log g
less than 4.2; i.e., they are associated with dwarfs, not giants. Because M-dwarfs are much
smaller than earlier spectral types, the amplitudes of the transits generated by small planets are
substantially larger than those generated by hotter stars. This fact introduces a strong bias that
will be considered in the next section.
4. Completeness Estimate
Although the primary purpose of the paper is to summarize the results of the observations and to
act as a guide to content of the tables, a model was developed to provide a first estimate of the
intrinsic frequency of planetary candidates. The intrinsic frequency of planetary candidates is
24
used here to mean the observed number of candidates per number of target stars that must be
observed to produce the observed number of candidates in the specified bins of semi-major axis a
and candidate size R when all selection effects are applied. The bin limits used for a are evenly
spaced from 0.0 to 0.5 AU with a spacing of 0.02 AU. The bin limits for the planetary candidate
size-classes are: Earth-size (0.5 " R < 1.25 R!), super-Earth-size (1.25 " R< 2.0 R!), Neptunesize (2.0" R <6.0 R!), Jupiter-size (6.0 " R < 15.0R! ), and very-Large-size (15.0 " R < 22.4 R!).
It should be noted that the calculation of the intrinsic frequency is equivalent to ratio of the
measured number of candidates divided by the expected number of candidates based on the
ensemble of stars that are observed.
For every candidate in a #a #R bin, each of the 156,000 target stars was examined to determine if
a planet orbiting it with the same size as the candidate and having the same a could be detected
during the Q0 through Q2 observation period. The number of target stars needed to produce a
minimum of two transits in the period of interest with a signal $7 ! was tabulated for each bin.
(There is no need for three transits because confirmation as a planet is not considered here.) The
actual period simulated is longer than the 138 days of the Q0 through Q2 period because the
search for planetary candidates used data obtained during later periods to obtain accurate values
of the epoch and period, as discussed earlier.
Inputs to the model include the observed noise for 3, 6, and 12-hour bins averaged over one
quarter of data (Q3) for each target star and the target stars size, mass, and magnitude, as well as
the values of the size and semi-major axis of each candidate in the #a #R bin. We also undertook
an independent analysis that used the observed noise for 3-hour bins averaged over the Q3 data.
Since the properties of the noises are not Gaussian, this serves as a check on our results.
The model computes the duration of the transits from the size and mass of the star at the specified
value of the semi-major axis. The value of the noise for each target star is interpolated to the
computed transit duration based on the values of the noise measured for 3, 6, and 12 hour
samples. This a very important correction because for 80%of the stars, the variation of CDPP
with the duration of the transit does not vary with the reciprocal of the square root of the time, but
is less than that expected from a Poisson-distribution . The signal level is computed from the
square of the ratio of the candidate size to the size of the target star. This value is then divided by
the interpolated noise value to get the estimated single-transit SNR. The total SNR is based on the
single-transit SNR multiplied by the square root of number of transits that occur during the
observation period. A correction is made for the loss of transits (and consequently, the reduction
in the total SNR) due to the monthly and quarterly interruptions of observations. The probability
of a recognized detection event is then computed from the value of the total SNR and a threshold
level of 7!. In particular, if the total SNR is 7.0, then the transit pattern will be recognized 50% of
the time while if the total SNR was estimated to be 8.0, then the transit pattern would be
recognized 84% of the time. The value of this probability p1 is tabulated and then an adjustment
is made for the probability that the planets orbit is correctly aligned to the line-of-sight p2. The
value of p2 is based on the size of the target star and the semi-major axis specified for the
candidate. The product of these probabilities pnc is the probability that the target star n could have
produced the observed candidate c.
The probability pnc is computed for each of the 156,000 stars and then summed to yield the
estimated number of target stars
that could have produced a detectable signal consistent
with candidates semi-major axis a and size R. (Subscripts designate candidate c, semi-major
axis value a, candidate size R.) This procedure is repeated for each candidate in the #a #R
bin.
25
The sum of the number of candidates of size-class k in a bin (a, #a, R, #R) is designated Sa,R,k.
The size-class k (k=1 to 5) represents Earth-size, super-Earth-size, Neptune-size, Jupiter-size,
and very-large size planetary candidates, respectively.
After a value of
has been computed for each candidate in the bin, the median value
of
is computed and used to estimate the frequencies:
Eq. 1
For each size-class, the sum of the frequencies over a and R is the estimate of the frequency for
that size-class:
Eq. 2
The summation for each size-class is done only for those bins that have at least 2 planetary
candidates and a minimum of 10 target stars. These choices help to reduce the impact of outlier
values.
The uncertainties in the results are quite large because the calculated number of stars
for
the observed number of candidates Sa,R,k is a sensitive function of the position of each planetary
candidate inside of the #a #Rr bin and because the number of candidates in each bin is often
small. In particular, estimated frequencies based on the sum of the individual frequencies in each
bin are very different than the estimates obtained by dividing the number of observed candidates
by the average number of expected planets. Therefore medians are used instead of averages to
reduce the effects of outliers.
To provide an estimate of the dispersion Da,R,k of the estimated frequencies for each bin, the
relative error associated with the number of candidates used in the estimate of the frequency is
added in quadrature to the variance due to the dispersion of the values of
.
Da,R,k =
where
,
Eq. 3
Eq. 4
It is important to note that the estimated frequencies calculated by the model are based upon the
number of candidates found in the data. In turn, the number and size distributions depend on both
the results from the analysis pipeline and a manual inspection of the results of the pipeline
product. The current version of the analysis pipeline provides threshold crossing events and
checks that those data are consistent with an astrophysical process. However, it does not yet have
the capability to stitch together quarterly records. Thus the number of candidates discussed here is
based on a combination of pipeline results, manual inspection, and an ad hoc program that does
not use the more comprehensive detrending that is done in the pipeline, but does allow a longer
period of data to be examined. In some cases, the candidates in the Q0-Q2 data were not
discovered until the Q3 and Q5 data were examined. As discussed later, the procedure is designed
26
to quickly find candidates that can be followed up, but is not well controlled for the purpose of
the model calculations. Consequently, the results must be considered very preliminary.
Table 7 presents an example of the calculated intrinsic frequencies, number of planetary
candidates, mean value of the number of target stars, and dispersion values for the range of a
from 0.01 to 0.50 AU for Earth-size candidates. The results for the all class-sizes are plotted in
Figure 14.
Table 7. Intrinsic Frequency of Earth-size Candidates (Simulation of 1.0 year of observations)
Results for Earth-size Candidates !
----- a (AU) -----!
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Relative
Dispersion
"#''+(+*!
"#'),(%,!
"#'")($&!
"#,(&,'(!
"#,')++*!
"#,&((++!
"#')(*%)!
$!
"!
"#&(),'!
"!
"!
"!
"!
"!
"!
"!
"!
"!
"!
"!
"!
"!
"!
"!
"!
The estimated intrinsic frequencies summed over semi-major axis are 0.054, 0.068, 0.193, 0.024,
and 0.0015 for Earth-, super-Earth-, Neptune-, Jupiter- and very-Large-size planetary candidates,
respectively. The sum over all values of the semi-major axis is 0.341. This value is interpreted to
27
mean that the average number of candidates per star with semi-major axes less than 0.5 AU is
0.341 with a very large uncertainty.
When the model is run to simulate a six-month period, the results are very similar for candidates
Neptune-size and larger, but the frequencies of super-Earth and Earth-size candidates are
increased by 3 for Earth-size candidates and 2 for super-Earth size candidates. The uncertainty in
the predictions will decrease as the mission duration increases and the number of transits and
resulting SNR increase.
Figure 14. Comparisons of the logarithms of intrinsic frequencies log(Frequency) to
observations log(# of Observations) as a function of semi-major axis for five size-classes. Red
symbols (circles) denote intrinsic frequencies and use the scales on the left vertical axes. Blue
symbols (diamonds) denote the number of observations and use the scales on the right vertical
axes. Values of the observations are shown if at least one event is found in a bin. To reduce the
effect of outliers, values for the intrinsic frequencies are shown only when at least two candidates
are found in the bin. Frequencies are based on 0.02 AU bins.
All the panels in Figure 14 show a large increase in intrinsic frequency with semi-major axis from
the 0.00 to approximately 0.07 AU and then show a negative or near-zero slope at larger values of
the semi-major axis. (The variation of intrinsic frequency for the very-Large candidates is too
noisy to characterize.) The result for the Jupiter-size candidates shows a nearly constant value
with semi-major axis. The peak in the intrinsic frequencies for the three smallest class-sizes is
located in the bin to the immediate right of the peak in the observations.
In Figure 15, the dependence of the intrinsic frequencies on the stellar temperature is examined.
Note that these results subsume the entire range of semi-major axis just discussed.
28
Figure 15. Logarithm of the mean number of candidates per star, as a function of stellar
effective temperature, after implementing the sensitivity correction described in Section 4. The
bins along the x-axis span 3000-4000K, 4000-5000K, 5000-6000K, 6000-7000K, with each bin
labeled by the central value for each bin.
The results shown in Figure 15 indicate that once adjustments are made for the increased
sensitivity to small planets orbiting small stars as opposed to Sun-like stars, the higher frequency
of Earth-size candidates orbiting the coolest stars seen in Figure 13 disappears. However, the
peak for super-Earth-size and Neptune size is still prominent and it is also clear that the Jupitersize and very-Large candidates are much more frequent around hotter than they are for the cooler
M- and K-type stars.
An examination of the panel in Figure 15 for the frequency dependence of Neptune-sized
candidates, suggests a negative correlation with temperature. The linear correlation coefficient
has a value of -0.95 with 95% confidence limits for the coefficient between -0.995 and -0.57.
Although the intrinsic frequencies of Jupiter-sized and very-large-sized candidates also suggest a
correlation with stellar effective temperature, because of the small number of data points, no
formal estimation can be obtained for their correlation coefficients nor those for the Earth-size
and super-Earth size candidates.
One of the surprising results shown in Figure 15 is the dip in the intrinsic frequency of Earth-size
and super-Earth-size candidates orbiting stars with temperatures near 4500K, i.e., K-type stars. A
careful inspection of the lower-left panel of Figure 3also shows a paucity of candidates for
temperatures between 4000 and 5000K. The large values of the dispersion shown in Figure 15
indicate that the result should be interpreted with caution.
29
It should be noted that the values for the intrinsic frequencies in Table 7 and in Figures 14 and 15
must be considered preliminary estimates. These values will be lowered when more false positive
events are recognized and removed, but they could also increase; the precision of the data is
assumed to improve as the square root of the number of measurements in transit. If, however, the
performance of the data does not achieve this ideal case, then fewer stars are being searched than
assumed here. Thus, the inherent frequency would be higher than shown in Table 7 and
associated figures. Furthermore, throughout the mission we will continue to make improvements
to the data analysis pipeline. As the capability of the system to recognize small candidates
improves, and more candidates in the data discussed here will be discovered. A significant
improvement is expected in mid-year when the capability to stitch together quarters of
observations becomes operational.
It is interesting to compare these results with those of Howard et al. 2010 for planets with periods
" 50 days discovered by RV. For planet masses 3 - 10 M! (super-Earth-mass), they get
approximately 10.7% to 11.8% while the present calculation for candidates with comparable
periods days and super-Earth size gives 7.0%. For 10 - 30 M!, Howard et al. obtain 5.8 - 6.5%
while the Kepler results for Neptune-size candidates predict 19.0%. The agreement is satisfactory
given the many uncertainties involved in the estimates.
5. Overview of Multi-planet Systems
A total 170 target stars with multiple planet candidates have been detected among the 997 host
stars in Kepler data. There are 115 stars with exactly two candidates, 45 with exactly three
candidates, 8 stars with exactly 4 candidates, 1 star with 5, and 1 with 6 candidates. For these
figures all candidates are included, whether they are validated planets or not. The fraction of host
stars that have multi-candidate systems is 0.17 and the fraction of the candidates that are part of
multi-candidate systems is 0.339, i.e., 408 among 1202 candidates. Because all the candidates
discussed here show two or more transits, accurate orbital periods and epochs are available in
Table 2.
30
Figure 16. Observed distributions of planetary candidates in multi-planet candidate systems. Bin sizes for
the upper two panels and the lower panel are 2 days, 1 R! , and 1000 K, respectively. Refer to Table 6 for
the definition of each size category.
Comparisons of the distributions presented in Figure 16 with previous figures show that they are
similar to those for the ensemble of all candidates. The number versus orbital period is very much
like that seen in Figure 6; a lack of candidates with orbital periods less than 2 days, a maxima
near 4 days, and a gradual reduction in the number with orbital period. The number versus
candidate size in Figure 16 is quite similar to that in Figure 2. The peak in the frequency with
stellar temperature for cool stars is also repeated. However, the distributions displayed in the two
scatter plots in the middle panel of Figure 16 show that the size versus orbital period and semimajor axis are different from those in Figure 3. In particular, both of the distributions shown in
Figure 16 display a lack of giant planets for close-in/short-period orbits compared to the
distributions in Figure 3. There is a clear paucity of giant planets in the observed multi-candidate
and multi-planet systems (see Latham et al. 2011 for details). This result is consistent with radial
velocity surveys which indicate short-period giant planets are significantly less common in
multiple planet systems (Wright et al. 2009).
31
An unusual candidate KOI# 961.02, shows up in second row, left hand panel of Figure 16. It has
a period of 0.45 days, a semi-major axis of 0.01 AU, and a size 28% larger than Jupiter. So far it
has passed all vetting tests and will be on the list to get an RV confirmation.
Multiple planet candidate systems, as well as the single-planet candidate systems, could harbor
additional planets that do not transit, or have not yet been recognized as such, and therefore are
not seen in these data. Such planets might be detectable via transit timing variations (TTVs) of
the transiting planets after several years of Kepler photometry (Agol et al. 2005, Holman and
Murray 2005, Holman et al. 2010). A preliminary analysis of transit times of planetary
candidates based on data up to and including quarter 2 provides hints that ~65 KOIs may already
exhibit transit timing variations. A statistical analysis of these and many other marginal TTV
signals has been submitted (Ford et al. 2011). Papers with TTV confirmation of three systems are
already published (Holman et al. 2010; Lissauer et al. 2011a) or in preparation (Cochran et al.
2011). Ford et al. (2011) predicts that Kepler will confirm (or reject) at least ~12 systems with
multiple transiting planet candidates via TTVs.
It is important to note that it is possible, though unlikely, for light from more than one
background eclipsing binary star system to be within the photometric aperture, producing an
apparent multi-planet transit signal in the light curve. While Latham et al. 2011 and Lissauer et al.
2011b present several arguments showing that candidates in multiples are more likely to be true
planets, a thorough analysis of each system and a check of background binaries are required
before any discovery can be claimed. Approximately 34% of Kepler candidates are part of multicandidate systems. The corresponding fraction of RV planets in multi-planet systems is 30%
based on the Extrasolar Planets Encyclopedia. The fraction of stars with multiple known planets
or candidates is 17% for the Kepler sample and about 12% for the RV sample. Given the various
limitations of these two observing techniques, these numbers are consistent. While an exhaustive
study remains to be done, Lissauer et al. (2011b) investigated the dynamical attributes of Kepler
multi-candidate systems and also suggest that nearly coplanar planetary systems might be
common.
6. Summary and Conclusions
Distributions of the characteristics of 1202 planetary candidates have been given. These include
number and frequency distributions with orbital size and period, stellar temperature and
magnitude. These distributions are separated into five class-sizes; 68 candidates of approximately
Earth-size (Rp < 1.25 R!), 288 super-Earth size (1.25 R! < Rp < 2 R!), 662 Neptune-size (2 R!, <
Rp < 6 R!), 165 Jupiter-size (6 R! < Rp < 15 R!), and 19 up to twice the size of Jupiter (15 R! <
Rp < 22 R!). Over the temperature range appropriate for the habitable zone, 54 candidates are
found with sizes ranging from Earth-size to larger than that of Jupiter. Six planetary candidates
in the habitable zone are less than twice the size of the Earth.
Over 74% of the planetary candidates are smaller than Neptune. The observed number versus size
distribution of planetary candidates increases to a peak at two to three times Earth-size and then
declines inversely proportional to area of the candidate. For candidate sizes greater than 2 R!, t he
dependence of the number of candidates on the candidate radius is proportional to the reciprocal
of the square of the inverse radius on candidate radius.
However, there is a prominent decrease in the number of candidates with size in all class-sizes for
semi-major axes smaller than 0.07 AU and for orbital periods less than 3 days. A group of
32
candidates with orbital periods less 3 days is identified that appears distinctly different from those
with longer periods in that the size distribution of candidates with short orbital periods is nearly
constant with candidate size.
The intrinsic frequencies of super-Earth-size and Neptune-size candidates show maxima for the
coolest stars. Both Earth-size and super-Earth-size candidates show minima for stars with
temperatures near 4500K. Jupiter-size and very-Large-size candidates show much higher
frequencies for hotter stars than for those cooler than 5500K.
The analysis of the first four months of Kepler observations is the first to estimate the frequency
of small candidates (Earth-size, super-Earth-size, and Neptune-size) based on a uniform set of
observations with the capability of detecting small candidates. After correcting for geometric and
sensitivity biases, we find intrinsic frequencies of 5.4% for Earth-size candidates, 6.8% for superEarth size candidates, 19.3% for Neptune-size candidates, and 2.4% for Jupiter-size candidates.
Multi-candidate, transiting systems are frequent; 17% of the host stars have multi-candidate
systems, and 33.9% of all the candidates are part of multi-candidate systems.
There is also evidence for 34 candidates with sizes between 1.3 and 4.5 times that of Jupiter. The
nature of these candidates is unclear. Those that are between 1.3 and 2.0 times the size of Jupiter
are included in tables and figures presented in this paper because of the possibility that they are
very inflated planetary objects, but the 15 larger than twice the size of Jupiter were omitted from
the discussion because it is more likely that they are stellar objects or that the estimated size of
the host star is much smaller than listed in the KIC.
In the coming years, many of these candidates are expected to be reclassified as exoplanets as the
validation effort proceeds. The number of candidates is so large that the Kepler team must be
selective in its follow up program and will devote the majority of its efforts to the detection and
validation of the smallest candidates and to those with orbital periods appropriate for the
habitable zone and those amenable to follow up. Many candidates will be left to future work or
for follow up by the community. The release of the Q0 through Q1 data and the early release of
the Q2 data and the descriptions of the candidates with accurate positions, magnitudes, epochs,
and periods should help the community to confirm and validate many of these candidates.
The data released here should also provide to the community a more comprehensive source of
data and distributions needed for further developments of the theories of planet structure and
planetary systems. These results have concentrated upon discovery of candidates, and initial
levels of validations sufficient to cull out many false positives. Future studies by the Kepler
science team will include efforts to robustly quantify the completeness of these candidate lists
through simulation studies, and provide more refined confidence levels on probabilities of
candidates being planets. Discovery of additional candidates will of course continue and reduce
incompleteness for weak signals whether those follow from small planets, long orbital periods, or
faint stars.
The Kepler Mission was designed to determine the frequency of extrasolar planets, the
distributions of their characteristics, and their association with host star characteristics. The
present results are an important milestone toward the accomplishment of Kepler's goals.
Acknowledgements
33
Kepler was competitively selected as the tenth Discovery mission. Funding for this mission is
provided by NASAs Science Mission Directorate. Some of the data presented herein were
obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the
California Institute of Technology, the University of California, and the National Aeronautics and
Space Administration. The Keck Observatory was made possible by the generous financial
support of the W. M. Keck Foundation. We sincerely thank Andrew Gould for his timely,
thorough, and very helpful review of this paper. The authors would like to thank the many people
who gave so generously of their time to make this Mission a success.
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35
36
Table 1.
Host Star Characteristics
All parameters are from the Kepler Input Catalog (KIC) except where Teff Flag = 1 indicates that no parameters were
available in the KIC. In which case Teff, log(g) and R are derived as noted.
Key:
KOI
Kepler Object of Interest number
KIC
Kepler Input Catalogue Identifier
Kp
Kepler magnitude
CDPP
6 hr Combined Differential Photometric Precision from Quarter 3
RA
Right Ascension (J2000)
Dec
Declination (J2000)
Teff
Effective Temperature of host star as reported in the KIC. If Teff Flag = 1, then Teff , log(g), R
are
derived using KIC J-K colour and linear interpolation of luminosity class V stellar properties of
Schmidt-Kaler (1982).
log(g)
Surface gravity reported by KIC. If Teff Flag = 1, then log(g) is based on J-K interpolation.
R
Stellar radius reported by KIC. If Teff Flag = 1, then R is based on J-K interpolation.
M
Stellar mass derived from log(g) and stellar radius.
KOI
11446443
10666592
10748390
3861595
8554498
11853905
6922244
5812701
9941662
10874614
8191672
11804465
9631995
6521045
8866102
8845026
10905239
9527334
6056992
11554435
7051180
3544595
6850504
11904151
7199397
10187017
2571238
Kp
CDPP
RA
DEC
Teff
log(g)
R
M
[mag]
1
2
3
4
5
7
10
12
13
17
18
20
22
41
42
44
46
49
51
63
64
69
70
72
75
82
84
KIC
[ppm]
[Hr]
[Deg]
[K]
[cgs]
[Rsun]
[Msun]
11.338
10.463
9.147
11.432
11.665
12.211
13.563
11.353
9.958
13.000
13.369
13.438
13.435
11.000
9.364
13.483
13.770
13.704
13.761
11.582
13.143
9.931
12.498
10.961
10.775
11.492
11.898
14
21.9
97.8
126
20.2
71.2
58.6
82
10.4
38.6
63.9
46.8
63.5
32.7
41.6
324
52.1
142
461
171
119
11.1
73.7
44.2
27.6
59.6
50.9
19.12056
19.48315
19.84729
19.62377
19.31598
19.04102
18.75254
19.83025
19.13141
19.78915
19.96047
19.08290
18.84198
19.42573
18.87671
20.01012
18.88370
19.48327
19.72792
19.28175
19.76737
19.42789
19.17987
19.04529
19.43315
18.76552
19.36139
49.3164
47.9695
48.0809
38.9474
44.6474
50.1358
42.4511
41.0110
46.8684
48.2399
44.0351
50.0404
46.3234
41.9903
45.1398
45.0896
48.3552
46.1648
41.3324
49.5482
42.5474
38.6724
42.3387
50.2413
42.7285
47.2080
37.8518
5713
6577
4628
6054
5766
5701
6164
6419
8848
5724
5816
6012
5859
5692
6035
5490
5562
5848
3240
5533
5128
5480
5342
5491
5718
4727
5347
4.14
4.32
4.53
4.41
4.04
4.35
4.44
4.26
3.93
4.47
4.46
4.47
4.53
4.51
4.22
4.48
4.48
4.45
4.90
4.40
3.94
4.43
4.72
4.47
4.40
3.96
4.58
1.50
1.34
0.76
1.08
1.73
1.16
1.05
1.32
2.44
0.91
0.95
1.01
0.94
0.95
1.37
0.88
0.89
0.97
0.27
1.07
1.94
1.03
0.70
0.98
1.08
1.86
0.84
1.14
1.36
0.71
1.11
1.18
1.08
1.12
1.17
1.83
0.91
0.95
1.09
1.07
1.06
1.14
0.85
0.87
0.97
0.21
1.05
1.19
1.04
0.95
1.03
1.08
1.14
0.98
Teff
Flag
1
1
1
1
1
1
1
1
37
85
87
89
92
94
97
98
99
100
102
103
104
105
107
108
110
111
112
113
115
116
117
118
119
122
123
124
127
128
131
135
137
138
139
141
142
144
148
149
150
151
152
153
155
156
157
159
161
5866724
10593626
8056665
7941200
6462863
5780885
10264660
8505215
4055765
8456679
2444412
10318874
8711794
11250587
4914423
9450647
6678383
10984090
2306756
9579641
8395660
10875245
3531558
9471974
8349582
5094751
11086270
8359498
11359879
7778437
9818381
8644288
8506766
8559644
12105051
5446285
4180280
5735762
3835670
7626506
2307199
8394721
12252424
8030148
10925104
6541920
8972058
5084942
11.018
11.664
11.642
11.667
12.205
12.885
12.128
12.960
12.598
12.566
12.593
12.895
12.870
12.702
12.287
12.663
12.596
12.772
12.394
12.791
12.882
12.487
12.377
12.654
12.346
12.365
12.935
13.938
13.758
13.797
13.958
13.549
13.960
13.492
13.687
13.113
13.698
13.040
13.397
13.771
14.000
13.914
13.461
13.494
13.738
13.709
13.431
13.341
41.6
32.5
28.4
34
35.6
46.7
43.8
115
31.2
78.7
42.4
33.6
58.4
30.5
43.7
32.5
44.7
36.7
59.4
71.9
55.1
41.6
31.7
46.5
48.6
41.1
261
70.7
239
266
54.7
55
68.4
74.6
87.2
122
95.1
86.8
75.8
104
108
89.6
76.3
142
111
78.6
81.1
19.24591
19.28117
19.98808
18.89165
19.82220
19.23877
19.18059
19.69562
19.41186
19.98032
19.44556
18.74632
19.92914
19.65568
19.26564
18.97038
19.17364
19.70991
19.48492
19.19249
20.05760
19.80188
19.15752
19.63728
18.96550
19.35951
19.52861
19.30720
19.74671
19.93984
19.01606
19.87196
19.72939
19.44355
19.20255
19.40987
19.76829
19.94261
19.10867
19.79873
19.49165
20.03448
19.19986
19.48810
19.60809
19.80767
19.84746
19.13678
41.1512
47.8845
43.8143
43.7882
41.8911
41.0898
47.3331
44.5311
39.1995
44.4358
37.7516
47.4971
44.8579
48.9824
40.0645
46.0638
42.1668
48.4956
37.6716
46.2762
44.3376
48.2086
38.6496
46.0623
44.3980
40.2849
48.6028
44.3454
49.1401
43.4976
46.6683
44.7463
44.5784
44.6883
50.6516
40.6694
39.2498
40.9490
38.9456
43.2098
37.6310
44.3816
50.9443
43.8812
48.3495
41.9091
45.2619
40.2116
6006
5606
7490
5850
6090
5944
6659
4951
6440
5919
5493
4411
5450
5816
5872
6344
5853
5839
5362
6202
5980
5725
5605
5380
5569
5897
6076
5570
5718
6244
5953
5289
6772
5921
5277
5361
4724
5063
6059
5538
6028
6187
4647
5651
4450
5675
5823
4768
4.07
4.36
3.90
4.28
4.08
4.27
3.92
4.33
3.69
3.90
4.63
4.56
3.96
4.46
4.36
4.35
4.46
4.31
4.34
4.25
3.96
4.47
4.49
4.44
4.58
4.29
4.25
4.53
4.18
4.40
4.51
4.25
4.12
4.56
4.60
4.68
4.00
4.51
4.23
4.29
4.40
4.54
4.41
4.18
4.54
4.47
4.31
4.04
1.66
1.14
2.24
1.26
1.66
1.29
2.08
1.11
2.79
2.08
0.80
0.73
1.88
1.01
1.15
1.18
1.02
1.22
1.15
1.34
1.91
1.00
0.97
1.00
0.86
1.25
1.32
0.92
1.43
1.10
0.95
1.27
1.62
0.90
0.81
0.74
1.75
0.89
1.35
1.23
1.09
0.94
0.95
1.42
0.76
1.00
1.22
1.66
1.19
1.07
1.45
1.11
1.20
1.12
1.31
0.97
1.39
1.24
1.00
0.71
1.19
1.08
1.10
1.14
1.08
1.11
1.04
1.15
1.22
1.07
1.05
1.02
1.03
1.11
1.14
1.04
1.13
1.13
1.08
1.05
1.26
1.07
0.97
0.96
1.11
0.94
1.14
1.08
1.11
1.10
0.85
1.12
0.73
1.06
1.10
1.09
38
162
163
165
166
167
168
171
172
173
174
176
177
179
180
183
186
187
188
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195
196
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199
200
201
202
203
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214
216
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219
220
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222
223
225
8107380
6851425
9527915
2441495
11666881
11512246
7831264
8692861
11402995
10810838
6442377
6803202
9663113
9573539
9651668
12019440
7023960
5357901
11391018
5771719
5972334
7950644
10799735
10904857
11502867
9410930
2987027
10019708
6046540
6849046
7877496
10619192
9305831
7046804
5728139
3762468
10723750
10656508
6300348
11046458
6152974
9595827
6305192
7132798
3937519
4249725
4545187
5801571
13.837
13.536
13.938
13.575
13.273
13.438
13.717
13.749
13.844
13.779
13.432
13.182
13.955
13.024
14.290
14.952
14.857
14.741
14.388
14.137
14.991
14.221
14.904
14.804
14.835
14.465
14.018
14.879
14.412
14.014
14.309
14.141
14.678
14.518
14.463
14.996
14.274
14.989
14.858
14.256
14.711
15.127
14.153
14.236
14.622
14.735
14.708
14.784
66.9
75.8
82.9
78.4
66.5
73.8
79.7
79.6
57
64.5
56.9
52.8
57.8
70.7
343
128
103
82.9
88.8
416
134
82.7
96.7
561
284
84.4
267
94.4
82.1
70.3
141
760
202
104
134
962
74.9
105
114
164
707
235
57.9
98.9
181
139
270
19.67759
19.20451
19.49913
19.40146
19.63093
19.61460
19.64947
19.55073
19.46047
19.78819
19.44312
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18.95962
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18.99200
18.97659
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18.86441
19.29564
19.63422
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19.66838
19.53950
19.14204
19.07402
19.89302
20.00682
19.69978
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19.68717
19.25287
19.19802
19.74265
19.90833
19.94754
19.65770
19.81427
19.72976
19.06205
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19.07747
19.66089
43.9630
42.3554
46.1962
37.7698
49.7650
49.4792
43.5368
44.8689
49.2621
48.1076
41.8847
42.2370
46.3287
46.2491
46.3912
50.4701
42.5509
40.5677
49.2670
41.0150
41.2220
43.7049
48.1953
48.3451
49.4734
45.9816
38.1844
46.9560
41.3555
42.3502
43.6810
47.8150
45.7621
42.5379
40.9773
38.8816
48.0402
47.9721
41.6032
48.5775
41.4248
46.2859
41.6640
42.6589
39.0981
39.3391
39.6780
41.0747
5632
5151
4956
5216
6285
5877
6287
5603
5752
4654
6340
5620
5827
5549
5722
5826
5768
5087
4787
5425
5495
5936
5883
5883
5604
5585
4907
6214
5774
5491
5912
5634
5287
5060
5771
6094
6221
6072
5843
5322
5086
5504
5347
5388
5176
4353
5128
6037
4.45
4.37
4.76
4.24
4.60
3.97
4.41
4.80
4.52
4.54
4.49
4.39
4.42
4.62
4.71
4.56
4.70
4.73
4.50
4.23
4.52
4.46
4.47
4.63
4.50
4.51
4.38
4.60
4.69
4.45
4.44
4.49
4.48
4.57
4.35
4.59
4.48
4.41
4.54
4.44
4.31
4.72
4.73
4.87
4.69
4.71
4.66
4.55
1.01
1.08
0.64
1.28
0.87
1.88
1.10
0.66
0.94
0.80
1.00
1.10
1.07
0.82
0.74
0.89
0.75
0.67
0.86
1.33
0.92
1.01
1.01
0.82
0.96
0.94
1.03
0.87
0.76
1.00
1.04
0.97
0.95
0.83
1.16
0.88
1.01
1.09
0.92
1.00
1.16
0.71
0.70
0.59
0.72
0.58
0.74
0.92
1.06
1.00
0.85
1.04
1.10
1.21
1.13
0.98
1.06
0.80
1.12
1.07
1.08
1.01
1.02
1.06
1.03
0.89
0.86
1.08
1.02
1.09
1.08
1.05
1.05
1.04
0.94
1.09
1.03
1.04
1.09
1.05
0.99
0.93
1.09
1.08
1.11
1.11
1.07
1.01
1.00
0.98
0.95
0.92
0.92
0.64
0.92
1.08
39
226
227
229
232
234
235
237
238
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240
241
242
244
245
246
247
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249
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285
5959753
6185476
3847907
4833421
8491277
8107225
8041216
7219825
6383785
8026752
11288051
3642741
4349452
8478994
11295426
11852982
5364071
9390653
9757613
10489206
11187837
11752906
5794240
7021681
11548140
5514383
11231334
8292840
5383248
11807274
10514430
12024120
3425851
7670943
6528464
9451706
3102384
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10586004
11133306
11401755
12314973
4141376
4143755
5088536
5695396
6021275
6196457
14.817
14.267
14.720
14.247
14.283
14.353
14.176
14.061
14.762
14.982
14.139
14.747
10.734
9.710
10.000
14.216
15.264
14.486
15.473
14.752
15.613
15.254
15.979
15.108
15.373
10.868
9.890
10.500
10.297
10.421
10.821
11.994
10.560
10.927
11.411
11.485
11.457
11.390
11.696
11.854
11.866
11.684
11.072
11.947
11.529
11.525
11.818
11.565
149
156
114
64.8
112
100
97.5
58.9
171
215
88.3
404
15.8
22.6
36.3
130
232
123
296
322
238
320
357
216
1996
43
115
24.5
39
30.6
39.4
36
23.4
22.6
26.7
35.5
23.1
26.9
35.2
22.8
42.1
70.9
23.1
36.1
42.6
37.1
25.5
48.1
19.44273
18.95680
19.38439
19.40746
19.35721
19.67400
19.73009
19.79991
19.81344
19.40534
19.11685
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41.2410
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44.5188
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49.0649
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50.1468
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48.8226
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40.7198
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44.2085
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50.0337
47.7744
50.4090
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43.3784
41.9008
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38.2288
43.9802
47.8486
48.7062
49.2318
51.0135
39.2119
39.2443
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5043
4043
5608
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5735
5041
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5437
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3804
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3933
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6023
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5848
6152
6435
5699
5900
5679
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5822
4.89
4.54
4.37
4.68
4.36
4.65
4.53
4.44
4.54
4.60
4.85
4.51
4.37
4.48
4.41
4.56
4.53
4.42
4.51
4.58
4.60
4.57
4.54
4.48
4.17
4.10
4.17
4.37
3.96
4.24
4.33
4.38
4.51
4.12
4.48
4.47
4.76
4.37
4.46
4.36
4.45
4.27
4.22
3.89
4.43
3.99
4.13
4.45
0.54
0.67
1.12
0.77
1.15
0.74
0.92
1.05
0.92
0.86
0.57
0.93
1.14
0.87
1.06
0.60
0.67
0.73
0.68
0.59
0.58
0.62
0.65
0.73
1.10
1.61
1.48
1.13
1.89
1.35
1.17
1.13
0.79
1.58
0.90
1.01
0.68
1.14
0.95
1.15
0.97
1.30
1.39
2.08
1.01
1.82
1.54
0.96
0.84
0.57
1.07
1.04
1.09
0.90
1.05
1.10
1.08
1.07
0.85
1.02
1.10
0.83
1.07
0.48
0.55
0.51
0.55
0.49
0.49
0.52
0.53
0.58
0.65
1.18
1.18
1.09
1.20
1.15
1.07
1.11
0.73
1.20
0.88
1.10
0.97
1.11
0.94
1.11
0.97
1.14
1.18
1.23
0.99
1.19
1.16
0.95
1
1
1
1
1
1
1
1
1
40
288
289
291
292
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295
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297
298
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302
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344
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349
350
351
9592705
10386922
10933561
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11259686
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13.928
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13.936
13.448
13.763
13.057
13.338
13.203
13.400
13.340
13.524
13.933
13.586
13.387
13.804
27.8
46.2
54.8
51
61.5
56.1
43.7
41.9
47.1
95.6
53.3
63.5
35.5
52.6
59.4
74.7
59.1
58.1
40.8
50.9
201
58.6
60.5
64.2
80.1
32.2
34.7
89
189
45.3
85.9
64.2
45.6
219
65.7
83.5
108
88.4
372
114
79.1
68.9
82.8
105
115
52.3
66
88.2
19.58110
18.86304
19.81853
19.15511
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18.98260
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43.3333
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4.15
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4.14
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4.35
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4.32
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4.26
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4.18
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4.34
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1.04
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1.29
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1.10
1.30
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1.17
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1.53
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0.70
1.27
0.27
1.02
1.31
0.59
0.71
1.05
1.54
0.91
1.36
0.77
2.15
1.16
1.02
1.16
1.51
1.04
1.28
1.14
1.12
0.94
1.01
0.94
1.01
1.11
1.08
1.01
1.09
1.13
0.84
1.19
1.13
1.24
1.03
1.21
0.92
1.07
1.11
1.17
1.04
1.01
0.53
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1.07
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1.06
0.21
1.11
1.11
0.91
0.99
1.13
1.20
1.06
1.02
1.05
1.23
1.05
1.07
1.08
1.05
0.96
0.96
1.08
1.09
1.09
1
1
1
1
1
1
1
1
41
352
353
354
355
356
360
361
364
365
366
367
368
369
370
371
372
373
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375
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384
385
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392
393
398
401
403
408
409
410
412
413
415
416
417
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419
420
421
422
423
425
426
427
11521793
11566064
11568987
11621223
11624249
12107021
12404954
7296438
11623629
3545478
4815520
6603043
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12356617
3323887
2446113
3353050
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5862
6007
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45
620
622
623
624
625
626
627
628
629
632
633
635
638
639
640
641
644
645
647
649
650
652
654
655
657
658
659
660
661
662
663
664
665
666
667
670
671
672
673
674
676
678
679
680
682
683
684
685
11773022
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385
153
33.3
141
104
62.2
86
82.7
122
65.5
63.5
170
121
87.7
69.3
146
69.9
60.6
48.1
57.8
83.8
166
101
48.3
109
119
55.3
59.9
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57.3
74.8
55.3
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65.9
847
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1
1
1
46
686
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688
689
691
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693
694
695
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700
701
703
704
707
708
709
710
711
712
714
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717
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719
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721
722
723
725
728
730
732
733
734
735
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740
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46.1
134
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48
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870
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890
891
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893
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901
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903
904
905
906
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912
913
914
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918
920
921
922
923
924
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50
926
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929
931
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937
938
939
940
941
942
943
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128
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30.8
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1
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0.96
0.56
52
1142
1144
1145
1146
1148
1149
1150
1151
1152
1159
1160
1161
1162
1163
1164
1165
1166
1168
1169
1170
1175
1176
1177
1187
1192
1193
1198
1199
1201
1202
1203
1204
1205
1207
1208
1210
1212
1214
1215
1216
1218
1219
1220
1221
1222
1226
1227
1230
8288947
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201
84.8
106
178
71.7
136
53.7
44.1
621
159
352
113
45.7
163
188
85.7
128
70.3
49.5
118
63.7
362
861
193
86.6
146
257
183
388
434
210
243
143
172
65.8
122
201
107
60.9
67.9
64
126
54
56.9
75.2
139
401
127
19.16516
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1.46
1
53
1236
1238
1240
1241
1242
1244
1245
1246
1257
1258
1261
1264
1266
1268
1270
1273
1275
1276
1278
1279
1281
1282
1283
1285
1288
1298
1299
1300
1301
1302
1303
1304
1305
1306
1307
1308
1309
1310
1311
1312
1314
1315
1316
1325
1328
1329
1335
1336
6677841
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124
113
99.9
104
48.4
91.1
69.6
104
104
256
118
216
189
94.4
118
118
78.4
105
129
71.2
93.6
42
23
147
129
338
94.7
161
118
114
203
193
198
97.7
75.2
77.5
94.3
51.1
101
68.9
57
32.8
222
206
190
135
184
19.15941
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1.29
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0.94
1.20
1.09
1
1
54
1337
1338
1339
1341
1342
1344
1353
1355
1360
1361
1363
1364
1366
1367
1369
1370
1372
1375
1376
1377
1378
1379
1382
1385
1387
1391
1395
1396
1401
1402
1403
1404
1405
1406
1407
1408
1409
1410
1412
1413
1419
1422
1423
1424
1425
1426
1427
1428
4243911
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4650674
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14.232
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14.631
169
173
125
119
110
57.1
113
210
287
149
271
219
179
159
124
154
120
52.5
75.4
85.8
51.1
51.9
576
215
92
152
301
305
114
184
214
280
178
103
179
166
119
137
67.7
99.9
299
300
235
137
198
76.1
229
105
19.04116
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0.85
1
1
1
55
1429
1430
1432
1433
1434
1435
1436
1437
1438
1439
1440
1441
1442
1444
1445
1448
1452
1459
1463
1465
1468
1472
1474
1475
1476
1477
1478
1480
1486
1488
1489
1494
1495
1498
1499
1501
1502
1503
1505
1506
1507
1508
1510
1511
1512
1515
1516
1517
11030711
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15.531
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14.271
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14.056
12.849
15.451
15.135
12.521
13.949
12.320
15.418
13.630
15.692
12.328
14.245
15.262
15.061
13.005
15.937
15.792
15.917
12.450
15.887
15.505
15.623
15.554
15.858
15.430
15.776
14.480
15.835
15.202
14.827
15.695
14.982
15.259
15.689
15.929
15.106
14.880
14.390
14.829
14.683
162
212
170
203
167
77.7
152
179
74.6
44.6
131
132
52.7
92.2
44.2
1365
440
484
48.2
179
276
103
70.4
292
299
36.3
310
170
212
205
139
188
92.1
269
140
134
213
177
198
208
275
128
155
121
155
117
19.49010
18.86932
18.88046
19.13713
18.90032
19.68591
18.93220
18.98978
19.55255
19.39012
19.53896
19.64535
19.06909
19.82611
18.92912
19.32035
19.55210
19.14288
19.21724
19.07663
19.92150
19.64216
19.69453
19.82869
19.39028
19.17693
19.25658
19.11612
19.62113
19.49026
19.21578
19.69714
19.84430
19.00381
19.84829
19.34149
19.41541
19.15235
18.82423
19.29497
19.69350
19.63514
19.67228
19.69450
19.12583
18.87570
19.76021
19.66379
48.5111
48.8254
48.5805
49.0460
49.4510
48.5997
49.2330
49.6924
48.8116
48.5213
48.5754
49.1402
49.6145
48.5607
49.1103
46.4917
43.0558
46.5081
43.3765
49.8675
46.6503
43.4005
51.1848
39.8478
51.2228
43.5057
51.2091
43.1901
43.6293
46.2263
46.6059
50.0772
43.2490
46.3207
43.5274
43.0856
50.5670
51.2500
46.6752
50.9941
50.4786
43.3682
50.1146
43.6056
50.3771
43.6571
51.2713
43.0143
5595
4502
5675
5560
4731
5744
5616
5791
5596
5967
5970
5575
5469
6101
6336
5658
6834
4060
6020
5619
5635
5455
6498
4097
5275
5346
5441
4948
5688
4984
5014
4559
5661
5941
5264
4659
5034
5356
5701
5582
5881
5695
4772
5520
5068
4103
6092
5815
4.58
4.60
4.65
4.83
4.47
4.70
4.52
4.46
4.43
4.31
4.68
4.43
4.24
4.25
4.36
4.36
4.10
4.40
4.38
4.85
4.44
4.92
4.08
4.59
4.52
4.71
4.73
4.74
4.62
4.51
4.61
4.54
4.50
4.67
4.38
4.51
4.64
4.90
4.54
4.62
4.54
4.93
4.79
4.61
4.70
4.57
4.56
4.43
0.87
0.71
0.80
0.63
0.89
0.75
0.93
1.01
1.04
1.22
0.77
1.04
1.30
1.33
1.18
1.14
1.66
0.84
1.09
0.62
1.02
0.56
1.68
0.63
0.90
0.71
0.70
0.65
0.83
0.88
0.78
0.78
0.95
0.78
1.07
0.83
0.75
0.56
0.92
0.82
0.92
0.56
0.59
0.83
0.70
0.66
0.90
1.06
1.03
0.73
1.03
0.97
0.86
1.03
1.05
1.07
1.06
1.12
1.05
1.06
1.08
1.14
1.14
1.08
1.27
0.65
1.05
0.98
1.06
0.93
1.23
0.56
0.98
0.95
0.97
0.85
1.04
0.92
0.91
0.77
1.05
1.05
1.01
0.82
0.90
0.91
1.05
1.02
1.07
0.97
0.77
1.01
0.90
0.58
1.09
1.08
1
56
1518
1519
1520
1521
1522
1523
1525
1526
1527
1528
1529
1530
1531
1532
1533
1534
1535
1536
1537
1540
1541
1543
1546
1549
1553
1557
1560
1561
1564
1569
1573
1574
1576
1577
1581
1582
1583
1584
1585
1586
1587
1588
1589
1590
1591
1593
1595
1596
7549209
7663405
9765975
9818462
12266636
9850893
7869917
9824805
7768451
7691260
9821454
11954842
11764462
11656246
7808587
4741126
11669125
12159249
9872292
5649956
4840513
5270698
5475431
8053552
7951018
5371776
8046659
4940438
5184584
8009350
5031857
10028792
5299459
12506770
7939330
4918309
12602568
9941066
5470739
10022908
9932970
5617854
5301750
5542466
10028140
5289854
10006581
10027323
15.219
15.369
14.516
14.817
14.264
14.673
12.082
15.216
14.879
14.083
14.307
13.029
13.069
12.841
13.939
13.470
13.046
12.710
11.740
15.559
15.189
14.985
14.456
15.135
15.182
14.840
15.042
15.549
15.287
15.587
14.373
14.600
14.072
15.988
15.481
15.402
15.068
15.961
15.401
14.940
15.700
14.699
14.764
15.674
15.372
15.809
14.904
15.157
117
154
85.8
128
106
134
77.1
135
94.1
73.3
77.3
43.9
54.7
48.9
60.1
51.5
41.8
47.6
31.3
759
705
953
177
155
122
222
111
252
127
240
115
85.3
152
270
200
132
135
321
217
169
254
145
160
255
173
182
128
162
19.82009
18.89855
19.32394
19.01975
19.72044
19.91534
18.79808
19.26617
19.77809
19.64333
19.13597
19.09558
19.50563
19.24410
19.08478
19.33939
19.70141
19.43115
18.76411
19.94022
19.54634
19.36316
19.90091
19.93706
19.22905
19.62945
19.82798
19.73556
19.40559
18.87531
19.78974
19.86113
19.85301
19.28604
18.82928
19.34191
19.37246
19.10569
19.83217
19.74515
18.77459
19.41020
19.88347
19.62432
19.84932
19.71901
19.31545
19.83399
43.1419
43.3838
46.5227
46.6034
50.9098
46.6887
43.6728
46.6708
43.4984
43.3356
46.6401
50.3003
49.9232
49.7372
43.5952
39.8170
49.7386
50.7595
46.7899
40.8493
39.9073
40.4429
40.6396
43.8972
43.7635
40.5576
43.8766
40.0196
40.3553
43.8882
40.1386
46.9651
40.4177
51.4089
43.7345
40.0218
51.6958
46.8709
40.6808
46.9990
46.8142
40.8875
40.4961
40.7209
46.9419
40.4396
46.9538
46.9613
5563
4994
5235
4962
5609
5207
6680
6011
5470
5087
6074
5973
5811
6225
6122
6193
5924
5848
6063
5390
6164
5821
5505
5401
5942
4783
5620
5659
5709
4639
5838
5537
5445
4165
5301
5384
5619
4147
5514
4692
5007
4106
5755
4830
5130
5676
5669
4656
4.57
4.68
4.51
4.42
4.41
4.37
4.24
4.69
4.24
4.95
4.53
4.41
4.41
4.31
4.43
4.42
4.33
4.41
4.37
4.53
4.53
4.54
4.97
4.36
4.52
4.25
4.39
4.48
4.92
4.61
4.57
4.58
4.35
4.61
4.57
4.80
4.63
4.52
4.66
4.70
4.54
4.58
4.42
4.50
4.97
4.54
4.52
4.39
0.88
0.71
0.91
0.99
1.07
1.08
1.38
0.77
1.31
0.51
0.94
1.08
1.07
1.24
1.07
1.09
1.19
1.08
1.12
0.90
0.95
0.92
0.52
1.12
0.95
1.22
1.09
0.98
0.56
0.72
0.89
0.85
1.13
0.62
0.85
0.64
0.82
0.72
0.78
0.65
0.85
0.64
1.06
0.88
0.49
0.91
0.94
0.99
1.03
0.88
0.98
0.95
1.06
1.01
1.20
1.05
1.08
0.84
1.09
1.10
1.08
1.14
1.11
1.12
1.11
1.09
1.07
1.00
1.10
1.06
0.93
1.04
1.08
0.96
1.07
1.06
0.97
0.77
1.06
1.02
1.05
0.58
0.98
0.94
1.03
0.62
1.00
0.77
0.93
0.57
1.08
0.88
0.84
1.05
1.05
0.87
1
57
1597
1598
1599
1601
1602
1603
1605
1606
1608
1609
5039228
10004738
5474613
5438757
4860678
5177104
5009189
9886661
10055126
5009743
12.681
14.279
14.802
14.659
14.943
14.429
14.832
13.984
13.797
13.956
94.7
107
119
108
173
96.4
123
76
74.4
62.5
19.89126
19.25596
19.89159
19.25140
19.85313
19.25486
19.41592
19.33674
18.80409
19.42704
40.1734
46.9867
40.6184
40.6642
39.9214
40.3891
40.1635
46.7134
47.0855
40.1255
6178
5565
5627
5502
5596
5995
5680
5377
6030
6063
4.36
4.52
4.48
4.60
4.58
4.67
4.33
4.57
4.39
4.45
1.17
0.93
0.98
0.83
0.87
0.79
1.17
0.85
1.12
1.03
1.14
1.04
1.05
1.01
1.03
1.06
1.08
0.99
1.11
1.10
1
58
Table 2
List of Planetary Candidates and their Characteristics
Key:
KOI
Dur
Depth
SNR
t0, t0_unc
Period, P_unc
a/R*, a/R*_unc
r/R*, r/R*_unc
b, b_unc
Rp
a
Teq
EB prob
V
FOP
N
KOI
Dur
[h]
Depth
[ppm]
Kepler Object of Interest number indicates that this KOI was detected on the basis of a single transit with the period derived
from the transit duration and stellar radius.
Transit duration, first contact to last contact
Transit depth at center of transit
Total SNR of all transits detected. SNR=Depth/(Std*sqrt(N)) where Std is the standard deviation of all data outside of transits
(Q0 through Q5) and N is the total number of measurements inside of all transits.
Time of a transit center based on a linear fit to all observed transits and its uncertainty
Average interval between transits based on a linear fit to all observed transits and uncertainty
Ratioofsemi-majoraxistostellarradiusassumingzeroeccentricity,aparameterderivedfromthelightcurve,anduncertainty
Note: For planets in non-circular orbits, a/R* is the scaled planet-star separation at the time of transit.
Ratio of planet radius to stellar radius and uncertainty
Impact parameter of the transit and uncertainty. Note, there is a strong co-variance between b and a/R*
Radius of planet in units of REarth=6378km
Semi-major axis of orbit based on Newtons generalization of Keplers third law and the stellar mass in Appendix1.
Equilibrium temperature of the planet (see main text and Appendix 5 for discussion)
Probability of background eclipsing binary confused with planets host star (see text for discussion)
Vetting flag
1
Confirmed and published planet
2
Strong probability candidate, cleanly passes tests that were applied
3
Moderate probability candidate, not all tests cleanly passed but no definite test failures
4
Insufficient follow-up to perform full suite of vetting tests
Follow-up observation description (to be revised)
1
Reconnaissance spectra taken
2
Adaptive optics observations taken
3
Speckle observations taken
4
10m/s RV spectra taken
5
2m/s RV spectra taken
NoObs No observations yet taken
Notes flag. A 1 indicates a note on this KOI or its host star in Appendix3.
SNR
t0
[BJD2454900]
t0_unc
Period
[days]
P_unc
a/R*
a/R*_unc
r/R*
r/R*_unc
b
b_unc
Rp
[REarth]
a
[AU]
Teq
[K]
EBprob
V FOP
N
59
1.01 1.7952
2.01 3.9107
3.01 2.3607
4.01 2.3866
5.01 2.0326
7.01 3.6234
10.01 3.2860
12.01 7.4343
13.01 3.2029
17.01 3.9011
18.01 4.6271
20.01 4.7062
22.01 4.3233
41.01 6.3192
42.01 4.4845
44.01 14.0968
46.01 3.8313
49.01 3.6652
51.01 3.3759
63.01 2.9910
64.01 1.6811
69.01 2.8948
70.01 3.7978
70.02 2.4785
70.03 7.2380
70.04 2.7697
72.01 1.8200
72.02 6.8565
75.01 17.4137
82.01 4.1390
82.02 3.2778
84.01 3.4186
85.01 4.0746
85.02 3.2040
85.03 4.2219
87.01 7.5747
89.01 10.4048
89.02 7.4240
92.01 3.7259
94.01 7.0052
94.02 5.3435
14174
6716
4197
1193
951
741
9390
9253
4644
10738
7239
16726
10570
224
251
2758
1347
1113
25812
4100
1223
269
1027
375
793
74
184
461
1275
981
248
692
326
99
103
481
372
377
703
5674
749
2062 55.76258
2413 54.35781
328 57.81227
136
90.5261
263
65.9735
231 56.61126
237 54.11809
604 79.59772
1147 53.56498
724 54.48575
496 55.90127
2001 104.00835
1098 110.24939
44
55.9589
34
114.235
67
93.395
145
103.931
17
108.99
275 66.93528
97 110.8421
132 90.54051
138 67.92512
135 71.60857
58
67.5005
34
97.729
15
68.93
101 64.57364
74
71.676
165
89.9691
102
67.7519
31
67.0745
141 68.99092
117
65.0392
53
66.5008
34
70.9924
38
66.6987
35
83.587
22
222.855
39
70.4508
382 65.74223
34
71.0084
0.00004
0.00005
0.00033
0.00055
0.00025
0.00041
0.00062
0.00038
0.00012
0.00007
0.00022
0.00006
0.00011
0.0042
0.018
0.013
0.00083
0.0053
0.00052
0.0015
0.00046
0.00069
0.00081
0.0011
0.01
0.0055
0.0007
0.0021
0.0019
0.0014
0.0044
0.00073
0.0012
0.0019
0.0035
0.0033
0.012
0.005
0.0042
0.00047
0.0051
2.4706131
2.2047355
4.8878177
3.84937
4.7803247
3.213682
3.522297
17.855038
1.7635892
3.2347003
3.548461
4.4379643
7.8914455
12.81521
17.8328
66.5126
3.487714
8.31393
10.431147
9.434152
1.9510939
4.726745
10.854042
3.696125
77.609
6.09852
0.8374958
45.29491
105.8885
16.14583
10.312
9.287047
5.859965
2.15488
8.13119
289.8605
84.6763
107.5
65.7008
22.34094
10.42361
0.0000004
0.0000004
0.0000089
0.000014
0.0000058
0.000011
0.00008
0.000038
0.0000014
0.0000012
0.000033
0.0000013
0.0000059
0.00029
0.0022
0.007
0.000028
0.00041
0.00002
0.000098
0.0000057
0.000018
0.000039
0.000017
0.0063
0.00014
0.0000042
0.00069
0.0014
0.00012
0.00026
0.00003
0.000039
0.000018
0.00012
0.0047
0.0075
0.0097
0.0019
0.00065
0.00022
8.519
4.152
16.1
10
7.3
3.94
8.15
19.9
4.51
6.9639
6.7257
8.0762
15.471
15.67
21.8612
17.3
7.241
19
21.1
27.57
4.4
12.706
20
6.2
83.39
16
3.609
35
47.1
18.3
13
21.25
7.7
4.5
7
311.1
56
48
56
24.3
13.73
0.082
0.041
9.1
24
2.2
0.56
0.34
0.025
0.2
0.0036
0.0047
0.0038
0.013
0.24
0.0027
1.2
0.044
1.1
6.3
0.63
1.3
0.084
18
9.6
0.99
95
0.035
38
2.3
6.7
30
0.15
5.7
1.3
15
5
156
14
17
4
0.76
0.12429
0.07931
0.0577
0.034
0.03707
0.02911
0.09138
0.0874
0.07695
0.09467
0.0788
0.11678
0.09222
0.01353
0.01721
0.0782
0.03279
0.0266
0.16271
0.0566
0.04
0.01465
0.0297
0.0209
0.02575
0.0079
0.01211
0.0214
0.0362
0.0337
0.0182
0.02349
0.0179
0.00923
0.0111
0.01956
0.018
0.02241
0.03169
0.07
0.022
0.00029
0.00012
0.0073
0.015
0.0002
0.00069
0.00071
0.0001
0.00043
0.00004
0.00005
0.00004
0.00006
0.00019
0.0013
0.00016
0.0014
0.00076
0.001
0.00034
0.00008
0.0054
0.0055
0.00033
0.0087
0.00009
0.0042
0.0012
0.0025
0.0083
0.00013
0.0022
0.00013
0.0039
0.00033
0.01
0.00061
0.00074
0.0024
0.051
0.816
0.51
0.29
0.7
0.91
0.86
0.53
0.0003
0.26
0.0001
0.0001
0.0271
0.001
0.6978
0.83
0.0021
0.03
0.56
0.025
0.84
0
0.49
0.85
0.198
0.4
0.029
0.73
0.01
0.85
0.86
0.0009
0.73
0.277
0.88
0.02
0.5
0.86
0.89
0.39
0.201
0.067
0.1
0.86
1.4
0.27
0.23
0.21
0.24
0.01
0.17
0.072
0.17
0.036
0.25
0.014
1
0.78
0.035
2.7
0.027
0.84
0.23
0.38
0.92
0.69
0.083
0.81
0.066
1.7
0.26
0.27
0.45
0.081
20.3
11.6
4.8
4.0
7.0
3.7
10.5
12.6
20.5
9.4
8.2
12.8
9.4
1.4
2.6
7.5
3.2
2.8
4.8
6.6
8.5
1.6
2.3
1.6
2.0
0.6
1.3
2.3
4.3
6.8
3.7
2.2
3.2
1.7
2.0
2.4
4.4
5.5
4.4
12.6
4.0
0.037
0.037
0.05
0.05
0.059
0.044
0.047
0.141
0.035
0.041
0.045
0.054
0.079
0.109
0.14
0.304
0.043
0.079
0.056
0.089
0.032
0.056
0.094
0.046
0.35
0.064
0.018
0.252
0.449
0.131
0.097
0.086
0.067
0.035
0.084
0.877
0.427
0.501
0.33
0.165
0.099
1603
1743
796
1242
1376
1290
1287
868
3257
1192
1180
1145
890
741
834
412
1117
906
314
844
1760
1036
643
919
333
779
1790
478
391
786
914
737
1318
1823
1177
282
756
698
505
851
1099
1.4E-06
2.4E-06
2.0E-06
9.5E-06
6.5E-06
9.4E-06
1.8E-06
1.6E-05
3.3E-05
4.8E-06
5.3E-06
3.6E-05
6.1E-06
1.1E-05
3.4E-05
5.3E-06
4.3E-05
1.7E-05
2.3E-05
1.9E-05
3.4E-05
1.0E-05
8.1E-06
5.6E-06
8.8E-06
4.2E-05
2.4E-05
1.2E-05
6.2E-05
5.4E-05
8.0E-06
2.2E-05
8.8E-05
1
1
1
3
3
1
1
3
2
1
1
2
2
2
2
2
2
2
3
2
3
3
2
2
2
2
1
2
2
2
2
2
2
4
4
2
2
2
2
2
2
NoObs
2,3
1
1
1
1
1
1
1
1
1
1
1
1,2,3
1,2,3
1,2,3,4
1,3
1
1
1
3
1,2,3,4
1
1
1
1
1,2,3
1,3
1,2,3
1,2,3
1,2
1
1,2,3,4,5
1,2,3,4,5
1,2,3
1,2,3,4
1,2
1,2,3
1
1,2,3
1,2,3
1,3
60
94.03 9.0070
97.01 5.5128
98.01 6.8561
99.01 19.7865
100.01 4.5162
102.01 2.4232
103.01 3.4297
104.01 1.2727
105.01 2.3693
107.01 4.8694
108.01 4.5210
110.01 3.9364
111.01 4.5716
111.02 5.7168
111.04 7.5697
112.01 6.3832
112.02 2.5592
113.01 4.6696
115.01 2.9014
115.02 2.7875
116.01 3.5494
116.02 6.7062
117.01 6.1280
117.02 4.0855
117.03 3.3490
117.04 4.1670
118.01 5.7166
119.01 11.2962
122.01 3.9263
123.01 3.6301
123.02 6.4510
124.01 3.8682
124.02 5.0544
127.01 2.9074
128.01 3.5022
131.01 4.6736
135.01 2.7842
137.01 3.5437
137.02 3.7766
137.03 2.0761
138.01 6.1103
1929
53
7396 1275
2299 478
1803
72
1506
95
933 240
800
72
1174
68
1082 114
463
91
505
79
522
98
506
84
456
65
636
38
756
67
118
24
1038
21
595
96
192
28
471
43
601
44
397
68
117
29
113
33
43
8.8
259
36
1579 144
509
89
293
66
365
65
223
32
352
39
11637 1078
11241 1191
6925 458
7916 766
2354 155
3279 297
269
38
7085 245
94.2397
67.27602
71.08749
73.0486
74.1515
68.05961
74.3331
67.99798
69.6502
67.0215
75.1762
68.2136
70.6135
65.7105
359.3572
118.1798
66.9837
87.3183
66.1414
72.0079
69.2763
84.9344
71.7751
71.6097
66.5106
70.838
71.6798
74.9125
64.9714
55.9766
70.5763
70.1234
75.822
67.02957
69.32863
66.17565
65.41537
68.40567
61.15248
66.5071
73.7648
0.0044
0.00013
0.00048
0.0019
0.0016
0.00042
0.0015
0.0007
0.0014
0.0015
0.0016
0.0013
0.0015
0.0022
0.0047
0.0018
0.0036
0.0041
0.0011
0.0042
0.003
0.0044
0.003
0.0052
0.0039
0.014
0.0044
0.0016
0.0013
0.0017
0.0024
0.0039
0.0038
0.0001
0.00024
0.00071
0.00014
0.00078
0.00045
0.0022
0.0019
90.5323
4.8854906
6.790119
817
9.966512
1.7351339
14.91155
2.508091
8.98092
7.257003
15.96534
9.94075
11.427514
23.6686
103.5112
51.07943
3.709209
300
5.412245
7.12575
13.57096
43.8448
14.74942
4.90134
3.17985
7.9572
24.99348
49.18381
11.522904
6.481654
21.22222
12.69116
31.71954
3.5787781
4.9427813
5.014177
3.0241018
7.641577
14.859006
3.50472
48.93807
0.0017
0.0000024
0.000019
12
0.000092
0.0000041
0.00013
0.000013
0.000096
0.000062
0.00016
0.000079
0.000074
0.00022
0.0066
0.00063
0.000057
0.000032
0.00017
0.00023
0.0013
0.00025
0.00015
0.000052
0.00051
0.0006
0.00044
0.000062
0.000047
0.00023
0.00029
0.00071
0.000002
0.000002
0.000021
0.0000017
0.000023
0.000025
0.000029
0.00058
84.7
7.8838
8.004903
327.4
7.8
4
36.15
16
12.2
11.608
22
13
14
28
108
40
6
167
13
11
21
54.1
8.8
5
3.9
11.11552
17
34.44916
22.89
11
19
14
28
10.33
12.11
8.885
8.998787
17.82
19.3
8
37
4.5
0.0076
0.000022
4.9
2.3
1.8
0.44
11
3.6
0.094
28
12
14
40
2
29
20
50
19
41
42
0.84
3
13
9.8
0.00071
22
0.00031
0.21
14
25
32
46
0.01
0.93
0.017
0.000005
0.11
2.1
26
11
0.0382
0.07784
0.0534
0.03768
0.04475
0.0303
0.02642
0.035
0.0394
0.01932
0.0211
0.0229
0.0222
0.0203
0.02271
0.0276
0.0128
0.066
0.0231
0.0151
0.0227
0.02306
0.0219
0.0121
0.0118
0.0062
0.0172
0.035
0.02023
0.0166
0.0183
0.0161
0.0196
0.09665
0.10066
0.07492
0.0795
0.04345
0.0616
0.0167
0.09401
0.0016
0.00007
0.0094
0.00052
0.0024
0.00024
0.0048
0.00059
0.00014
0.0047
0.0034
0.0038
0.0052
0.00038
0.0033
0.0079
0.021
0.006
0.0088
0.0078
0.00033
0.0012
0.0052
0.0048
0.0036
0.018
0.00016
0.0039
0.0042
0.0057
0.005
0.00007
0.00052
0.00012
0.0074
0.00022
0.0013
0.0093
0.00057
0.006
0.0001
0.88
0.76
0.025
0.45
0.91
0.009
0.6
0.74
0.72
0.5
0.018
0.78
0.9
1.02
0.5
0.9
0.8
0.021
0.89
0.87
0.8
0.6594
0.86
0.0009
0.0038
0.6
0.7
0.85
0.84
0.0038
0.58
0.0008
0.0089
0.027
0.84
0.8
0.82
0.076
0.26
0.52
0.027
0.86
0.27
0.017
1.1
0.76
0.82
1.2
0.071
0.63
1
0.31
1.2
1.2
1.1
0.025
0.32
0.98
1
0.68
1.1
1
0.95
0.84
0.16
0.02
0.21
1.3
0.25
6.9
11.0
12.1
4.6
13.6
6.9
2.3
2.8
8.1
2.1
2.7
2.9
2.5
2.3
2.5
3.7
1.7
8.3
3.4
2.2
4.7
4.8
2.4
1.3
1.3
0.7
1.8
3.9
1.9
2.3
2.5
2.3
2.8
9.7
15.7
9.0
8.3
6.0
8.6
2.3
16.6
0.419
0.059
0.077
1.693
0.101
0.03
0.119
0.032
0.09
0.075
0.128
0.095
0.102
0.166
0.443
0.279
0.048
0.888
0.063
0.076
0.119
0.26
0.12
0.058
0.043
0.08
0.17
0.264
0.101
0.071
0.155
0.111
0.205
0.046
0.059
0.06
0.042
0.077
0.12
0.046
0.282
534
1226
1528
177
1493
2175
628
927
1100
943
777
985
814
638
391
539
1300
269
1260
1147
1057
715
729
1048
1217
892
590
462
716
1091
739
926
681
1098
1240
1181
1250
949
760
1228
716
4.5E-05
1.3E-05
9.0E-06
4.2E-05
3.1E-05
5.8E-05
4.8E-05
8.4E-06
4.4E-05
2.6E-05
3.0E-05
1.5E-05
2.1E-05
2.1E-05
2.2E-05
1.9E-05
1.6E-05
2.1E-05
8.1E-05
7.9E-05
4.4E-05
6.1E-05
5.8E-05
3.0E-05
2.3E-05
1.3E-05
3.6E-05
3.4E-05
2.5E-05
2.2E-05
1.4E-05
1.1E-05
9.3E-06
6.2E-05
4.8E-05
-
2
1
2
3
3
2
2
2
2
2
2
2
2
2
2
3
4
2
2
2
2
2
2
3
3
4
2
3
2
2
2
2
2
2
2
3
2
2
2
4
2
1,3
1
1,2,3
1
1,3
1,2,3
1,2,3
1,2,3
1
1
1,2,3
1
1,2,3
1
1
1
1
2,3
1
1,2
1,2
1
1,2,3
1
1,2,3
1,2
1,2
1
1
2
1
1,2,3
1,2,3,4
1,4
1,2
1
1,2
1
1
1,2,3,4
1,4
61
1
1
1
139.01 10.7262
139.02 2.6756
141.01 1.4408
142.01 3.7354
144.01 3.7045
148.01 2.6944
148.02 3.2778
148.03 5.6283
149.01 7.8599
150.01 3.5591
150.02 5.0711
151.01 2.6612
152.01 8.5892
152.02 6.7876
152.03 5.0646
153.01 2.7092
153.02 2.5456
155.01 4.5785
156.01 2.4887
156.02 2.4671
156.03 2.8987
157.01 4.6051
157.02 5.5677
157.03 4.3105
157.04 6.3817
157.05 9.7575
157.06 4.1041
159.01 4.1073
161.01 1.9363
162.01 4.6255
163.01 3.3145
165.01 2.7694
166.01 2.4622
167.01 4.2389
168.01 6.1290
168.02 5.7377
168.03 4.7708
171.01 3.6443
172.01 4.9815
173.01 4.4592
174.01 3.3658
3542
116
2421
1188
1396
453
960
519
961
783
796
1302
2845
753
636
990
797
733
554
330
1423
757
975
1352
524
1119
297
477
898
706
654
916
704
415
358
80
98
489
586
421
1060
102
13
167
105
166
54
107
37
114
75
53
58
118
39
40
57
67
84
35
26
96
83
80
86
36
54
36
46
137
62
58
50
45
70
42
13
13
62
46
44
27
75.0881
74.354
65.30523
66.0242
66.08938
57.0628
58.3427
79.0652
78.0897
67.0052
76.8337
65.8279
91.7438
66.6192
69.6257
72.7136
61.5475
70.4159
76.0363
78.3602
75.7045
71.1768
81.4549
87.1604
158.0328
220.288
71.5062
69.7359
66.21002
75.2079
72.7543
72.5644
71.4619
67.602
66.2761
70.389
71.317
70.1549
70.8361
71.9655
77.8417
0.0028
0.0066
0.00055
0.0013
0.00084
0.0021
0.0013
0.0037
0.0017
0.0016
0.003
0.0017
0.0019
0.0059
0.005
0.0017
0.0015
0.0017
0.0028
0.0039
0.001
0.002
0.002
0.0015
0.0034
0.004
0.0038
0.0033
0.00063
0.0024
0.002
0.002
0.002
0.002
0.0041
0.011
0.011
0.002
0.0034
0.0033
0.0054
224.7937
3.3418
2.624219
10.914785
4.176263
4.777978
9.67374
42.89554
14.55792
8.408848
28.57378
13.44739
52.09119
27.40415
13.484
8.925031
4.753978
5.660629
8.04144
5.18856
11.776179
13.02495
22.68696
31.99541
46.68872
118.3772
10.3039
8.99093
3.105501
14.00656
11.11978
13.22216
12.49334
4.919592
10.74356
5.0918
7.10664
5.968839
13.72288
10.06092
56.3509
0.0032
0.00012
0.000011
0.000076
0.00002
0.000053
0.000068
0.0007
0.00015
0.000076
0.0005
0.00013
0.00063
0.00089
0.00039
0.000085
0.000039
0.000057
0.00013
0.00012
0.000054
0.000093
0.00015
0.00018
0.00081
0.0031
0.00013
0.00017
0.000011
0.00019
0.00013
0.00016
0.00015
0.000055
0.00025
0.00025
0.00032
0.000069
0.00026
0.00019
0.0025
126
7
10.7
23
7.9
9
16
53
14.722
18.63
33
22.5
48.52
31.74
18
19
8
9.64
18
10
32.64
15
17.8
33.5
57.4
95.9
18.2
8.9
11
23.73
22
29
34
8
12
6.93
11.4
12.89
21.44
17.75
142.2
22
36
8.4
6.9
4.7
16
16
16
0.083
0.21
55
6.8
0.27
0.67
66
34
12
0.09
46
36
0.37
11
5
9.7
1.1
1.2
5.5
9.1
12
0.3
37
69
84
13
22
0.29
0.53
0.17
0.35
0.31
5.3
0.0576
0.012
0.0489
0.03073
0.0345
0.0218
0.0305
0.02093
0.02799
0.02552
0.0276
0.03831
0.04816
0.02485
0.024
0.03
0.0295
0.02428
0.023
0.02
0.03337
0.0278
0.0322
0.0387
0.02041
0.02976
0.01559
0.0235
0.0293
0.02379
0.0242
0.028
0.026
0.0195
0.018
0.00908
0.00978
0.02039
0.02184
0.01863
0.02897
0.0022
0.011
0.0077
0.0003
0.0047
0.0076
0.006
0.00041
0.00016
0.00024
0.0081
0.00062
0.00026
0.00051
0.015
0.012
0.0086
0.0002
0.013
0.014
0.00028
0.0038
0.0015
0.002
0.00036
0.00034
0.00033
0.0038
0.0068
0.00026
0.0082
0.014
0.013
0.0055
0.006
0.00035
0.00042
0.00022
0.00031
0.00028
0.00083
0.67
0.7
0.73
0.53
0.8
0.72
0.216
0.0005
0.006
0.7
0.74
0.0002
0.024
0.5
0.7
0.83
0.0011
0.7
0.8
0.027
0.76
0.84
0.84
0.014
0.03
0.128
0.86
0.69
0.0008
0.6
0.7
0.7
0.6
0.5
0.029
0.015
0.0172
0.0102
0
0.027
0.37
2
0.72
0.78
1
0.82
0.065
1.1
0.22
0.032
1.9
1.1
0.8
1.4
1.3
0.027
0.69
0.34
0.35
0.025
0.032
0.038
0.62
0.91
1.3
1.4
1.4
1.3
1.4
0.01
0.01
0.025
0.05
5.7
1.2
4.3
2.5
6.6
2.1
3.0
2.0
4.1
3.4
3.7
4.6
4.9
2.5
2.4
3.2
3.1
3.8
1.9
1.6
2.8
3.0
3.5
4.2
2.2
3.2
1.7
3.1
5.3
2.6
2.8
1.9
3.7
1.8
3.7
1.9
2.0
2.5
1.6
1.9
2.5
0.741
0.045
0.037
0.095
0.053
0.054
0.087
0.235
0.122
0.083
0.187
0.114
0.282
0.184
0.114
0.08
0.053
0.065
0.071
0.053
0.091
0.111
0.16
0.201
0.259
0.481
0.095
0.087
0.043
0.116
0.097
0.104
0.107
0.058
0.102
0.062
0.077
0.067
0.112
0.093
0.267
288
1169
1090
661
1198
908
716
435
890
939
625
823
497
616
782
708
870
1164
642
743
567
751
625
558
491
361
811
963
1306
733
756
541
796
1072
1112
1427
1280
1125
598
808
355
1.9E-05
4.4E-05
1.5E-05
2.9E-05
7.5E-05
1.5E-04
1.1E-04
1.3E-04
2.9E-05
6.7E-05
6.5E-05
5.9E-05
5.6E-05
9.1E-05
9.4E-05
1.8E-05
2.0E-05
2.9E-05
2.4E-05
2.8E-05
1.9E-05
1.5E-04
1.4E-04
1.1E-04
1.7E-04
1.3E-04
2.0E-05
1.1E-04
2.5E-05
7.2E-05
2.4E-05
3.8E-05
5.9E-05
3.0E-05
3.2E-05
7.6E-05
4.0E-05
2.8E-05
4.3E-05
2
2
2
2
2
2
2
2
2
2
2
3
2
2
2
2
2
2
2
2
2
1
1
1
1
1
1
2
2
2
2
2
2
2
2
4
4
2
2
2
2
1
1
1,2
1,3
1
1,2,3
1
1
1
1
1
2
1
1
1,2
1,2
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
1
62
176.01 6.5324
177.01 4.8343
179.01 10.2799
180.01 3.2069
183.01 2.6997
186.01 3.0609
187.01 5.3569
188.01 2.2281
189.01 6.0251
190.01 4.4351
191.01 4.1332
191.02 2.1206
191.03 1.4863
191.04 5.3874
192.01 4.2999
193.01 5.0147
194.01 2.0031
195.01 2.1873
196.01 2.2855
197.01 4.2447
199.01 3.4738
200.01 2.8848
201.01 2.8358
202.01 1.9597
203.01 2.2791
204.01 3.0172
205.01 3.0463
206.01 6.2693
208.01 3.2881
209.01 10.8828
209.02 7.1448
211.01 4.8294
212.01 3.5920
214.01 1.4852
216.01 3.6988
217.01 2.8377
219.01 5.3499
220.01 2.5693
220.02 2.8695
221.01 2.6291
222.01 2.8034
397
281
972
626
18301
17321
24933
14813
22443
11465
15314
680
210
265
10023
20885
16271
14694
10797
10776
10575
8465
6043
10265
20902
7176
10043
5001
9253
5841
2349
7800
5153
5803
5400
22161
3196
1912
109
3998
1305
36
26
94
20
1464
1071
739
1052
778
431
523
41
21
9.6
511
667
118
494
1009
593
847
542
777
1056
500
430
554
464
99
209
147
91
250
324
146
818
228
265
12
283
65
67.5141
76.6066
75.8002
62.0919
66.35411
66.66821
84.52867
66.5079
81.09127
72.30197
65.38412
65.5052
66.3662
77.73
70.02102
90.34941
72.46531
66.631
70.18042
66.83869
70.48111
67.34424
70.5598
66.02029
65.79282
66.37805
75.17334
64.98094
67.711
68.6335
78.8225
69.0141
72.23136
64.74221
74.2081
66.41389
65.46923
65.93893
66.6388
65.44215
65.6572
0.0049
0.0059
0.0027
0.0038
0.0001
0.00012
0.00025
0.00009
0.00024
0.00032
0.00025
0.0019
0.0029
0.015
0.0003
0.00029
0.00061
0.00019
0.00009
0.00027
0.00015
0.0002
0.0003
0.00008
0.00014
0.0003
0.00022
0.00042
0.0011
0.0011
0.0031
0.001
0.00055
0.00022
0.00097
0.00019
0.00078
0.00038
0.0072
0.00037
0.0017
30.2303
21.05996
20.74007
10.0456
2.684327
3.2432615
30.88252
3.7970199
30.360407
12.265011
15.358776
2.418402
0.7086217
19.3245
10.291006
37.590346
3.120831
3.2175236
1.8555565
17.276276
3.2686931
7.3407361
4.2253865
1.7208618
1.4857106
3.2467374
11.720115
5.334076
3.00385
50.78974
18.79567
372.1084
5.69584
3.3118618
20.17213
3.9050889
8.025085
2.4220912
4.12515
3.4130416
6.312382
0.0008
0.00071
0.00033
0.0002
0.0000015
0.0000021
0.000048
0.0000018
0.000057
0.000024
0.000016
0.00002
0.000009
0.0013
0.000018
0.00007
0.000011
0.0000035
0.000001
0.000027
0.0000029
0.0000086
0.0000072
0.0000008
0.0000012
0.0000053
0.000015
0.000013
0.000019
0.00031
0.00034
0.0015
0.000048
0.0000042
0.00013
0.0000051
0.000037
0.0000053
0.00012
0.0000073
0.000058
24
28
15.93
25.5
8.581648
9.1033
50.291303
14.451
42.5
15.27
28.4
8.45
3.035907
29.5
19.951591
74.98
8.9
11.28
5.87
36.447
7.899543
21.103
12.387
5.27
5.682
8.855
30.4
6.941
7.443
38.12
21.0514
639.12
12.88171
9.4
52.37
11.892
12.067
6.3
11.37
10.544
18.28
41
86
0.1
1.4
0.000005
0.0094
0.000079
0.017
1.1
0.32
1.3
0.5
0.000039
7.9
0.000035
0.12
1
0.91
0.27
0.065
0.000007
0.04
0.032
0.12
0.014
0.021
3
0.011
0.071
0.12
0.003
0.68
0.00011
2.8
0.4
0.017
0.042
3.3
0.64
0.04
0.28
0.0202
0.0162
0.02832
0.02066
0.122
0.11805
0.142
0.10841
0.13323
0.11222
0.115
0.028
0.01386
0.0148
0.09
0.12875
0.1338
0.1144
0.09728
0.09147
0.093
0.08279
0.07155
0.10151
0.13028
0.07562
0.0918
0.06342
0.08887
0.06873
0.044
0.081
0.064
0.1106
0.06487
0.13352
0.0505
0.041
0.01042
0.05615
0.03254
0.0056
0.0092
0.00019
0.00093
0.019
0.00009
0.013
0.00009
0.00083
0.0006
0.0011
0.0013
0.0037
0.021
0.00016
0.0037
0.0019
0.00088
0.00012
0.017
0.00012
0.00014
0.00047
0.00024
0.00014
0.002
0.00009
0.00066
0.00021
0.04
0.096
0.014
0.0035
0.00038
0.00014
0.00015
0.0042
0.00052
0.00016
0.00039
0.8
0.6
0.0005
0.028
0.0072
0.0007
0.0004
0.29
0.814
0.49
0.0176
0.615
0.006
0.0001
0.0017
0.79
0.57
0.51
0.0002
0.0001
0.0103
0.74
0.46
0.0016
0.0003
0.031
0
0.023
0.0002
0.93
0.0005
0.0004
0.0012
0.55
0.0198
0.0298
1
1.7
0.062
0.18
0.1
0.22
0.027
0.24
0.28
0.22
0.12
0.01
0.33
0.02
0.014
0.039
0.28
0.72
-
2.2
1.9
3.3
1.8
9.9
11.5
11.6
8.0
12.6
16.3
11.6
2.8
1.4
1.5
9.9
14.2
12.0
11.9
10.0
10.3
8.7
6.9
7.8
11.5
13.8
7.9
8.3
8.0
8.5
7.6
4.9
9.6
6.5
12.1
8.2
10.4
3.8
2.6
0.7
4.4
2.1
0.197
0.153
0.152
0.092
0.038
0.044
0.194
0.046
0.181
0.107
0.122
0.036
0.016
0.142
0.095
0.226
0.043
0.043
0.03
0.128
0.044
0.075
0.052
0.029
0.026
0.043
0.099
0.062
0.042
0.278
0.143
1.048
0.064
0.044
0.145
0.048
0.077
0.034
0.049
0.043
0.057
630
664
681
731
1113
1156
499
859
461
843
666
1226
1839
617
855
548
1133
1165
1377
615
1216
810
1064
1559
1518
1098
647
1102
1229
522
728
273
977
1119
635
935
710
987
822
935
613
5.4E-05
1.7E-04
1.6E-05
1.5E-05
1.6E-05
1.2E-05
2.1E-05
6.0E-06
1.0E-05
4.6E-05
1.3E-04
1.4E-05
1.1E-05
6.7E-06
1.2E-05
2.1E-05
2.6E-05
2.2E-05
2.8E-05
1.3E-05
1.6E-05
6.4E-05
3.4E-05
5.6E-05
1.2E-05
1.6E-05
5.3E-05
2.2E-05
8.3E-05
2.0E-05
1.0E-04
6.1E-05
2.7E-05
3.7E-05
2
2
2
2
2
2
2
2
2
2
2
3
2
2
2
2
2
2
2
2
2
2
3
2
2
2
2
2
3
2
2
3
2
2
2
2
2
2
4
2
2
1
1
1,2,3
1
NoObs
1
1
NoObs
NoObs
1
1
1
1
NoObs
NoObs
NoObs
1
NoObs
1
NoObs
1
1
NoObs
1
1
63
222.02 3.2313
223.01 1.5125
223.02 4.0259
225.01 1.2452
226.01 3.0258
227.01 4.6968
229.01 2.9170
232.01 4.9765
232.02 3.7903
234.01 4.5866
235.01 2.0142
237.01 3.4487
238.01 4.4245
239.01 2.8293
240.01 4.2286
241.01 3.5173
242.01 5.7720
244.01 2.8876
244.02 3.5837
245.01 4.7135
246.01 3.4381
247.01 2.0575
248.01 2.5695
248.02 2.0752
248.03 1.6378
249.01 1.8415
250.01 2.8200
250.02 2.1205
250.03 1.9814
251.01 1.8489
252.01 3.5652
253.01 1.7694
254.01 1.9011
255.01 4.1157
256.01 1.2273
257.01 2.3916
258.01 5.2610
260.01 4.5271
260.02 10.7302
261.01 3.8752
262.01 4.1589
891
1128
991
2571
773
1304
3054
2256
354
778
661
601
472
1378
1322
825
3941
1176
395
575
283
999
1803
1348
764
1775
2855
2011
343
2342
2052
2157
39093
2457
16968
514
998
94
324
693
111
32
67
25
200
39
55
228
158
32
53
46
50
32
76
84
46
193
211
157
96
127
22
54
28
31
74
74
39
15
82
45
49
795
65
55
33
39
20
37
45
27
63.7728
67.477
80.0334
74.537
71.1091
69.5662
67.93353
67.00465
67.0179
65.1832
66.8175
67.7859
68.0935
71.5556
71.6146
64.7933
71.34318
111.52718
104.7062
108.239
106.85727
114.1234
103.2885
102.8387
105.1278
108.75705
103.4024
82.8815
69.2598
104.08747
103.5012
103.6019
103.82108
122.8256
102.77735
105.6621
105.4942
105.786
178.0423
104.0206
105.6257
0.0044
0.0011
0.004
0.00032
0.0029
0.0024
0.0005
0.00095
0.0056
0.0026
0.0019
0.0024
0.0047
0.0013
0.0016
0.0027
0.00098
0.00043
0.0013
0.0013
0.0007
0.0023
0.0013
0.0022
0.0019
0.00086
0.0012
0.0023
0.0046
0.0008
0.002
0.0012
0.00009
0.0015
0.00093
0.0021
0.0018
0.0063
0.0039
0.0022
0.0035
12.79397
3.177431
41.0084
0.838598
8.3089
17.66076
3.5732
12.465891
5.76607
9.61391
5.632479
8.50827
17.23217
5.640649
4.286837
13.82145
7.258477
12.720359
6.23855
39.79454
5.398753
13.81524
7.203494
10.91401
2.576536
9.549259
12.282356
17.25204
3.543871
4.164371
17.60439
6.38324
2.4552389
27.52156
1.378681
6.883344
4.157642
10.49577
100.27937
16.23844
7.81279
0.0003
0.000019
0.00084
0.0000022
0.00014
0.00025
0.00001
0.000067
0.00018
0.00014
0.000061
0.00011
0.00045
0.000043
0.000041
0.00027
0.000041
0.000038
0.000058
0.00038
0.000027
0.00032
0.000065
0.00018
0.000033
0.000058
0.000097
0.00025
0.000071
0.000023
0.00024
0.000071
0.0000016
0.00031
0.000012
0.000098
0.000069
0.00046
0.00052
0.00017
0.00019
30.47
12
68
4.2
15
42.02
9.976
19.996
11.83
11
21.29
19.7
23
9.3
8.04
22
10.183
19.1
7.5
67.02
9.5
52.5
22.73
43.1
13
43
36.32
34
14.5
18.37
40
31.13
11.95
54.25
9
18
5.2
17.32
61
20
7
0.95
24
381
1.3
39
0.57
0.044
0.1
0.36
15
0.51
0.33
61
5.9
0.076
49
0.042
2.7
6.3
0.57
6.7
2.3
0.4
1.8
38
101
0.48
10
1
0.28
135
0.81
0.42
0.7
2.7
65
7.6
0.52
127
29
21
0.02647
0.034
0.03
0.04932
0.028
0.03955
0.04922
0.04269
0.0185
0.0278
0.02282
0.02262
0.0214
0.0382
0.03302
0.028
0.05567
0.03659
0.0214
0.02158
0.0167
0.0312
0.03948
0.0343
0.027
0.039
0.04892
0.0486
0.0173
0.04436
0.042
0.04291
0.1841
0.04484
0.1235
0.023
0.0281
0.0096
0.0178
0.027
0.0111
0.00065
0.013
0.034
0.00032
0.014
0.00039
0.00017
0.00018
0.00048
0.0067
0.00042
0.00031
0.0098
0.0041
0.00027
0.012
0.0002
0.00081
0.0027
0.00015
0.0022
0.0011
0.00055
0.0011
0.012
0.014
0.00048
0.0015
0.001
0.0005
0.022
0.00079
0.0012
0.00047
0.0023
0.014
0.0069
0.00026
0.006
0.0067
0.0046
0.0253
0.7
0.6
0.47
0.7
0.031
0.0003
0.028
0.0102
0.73
0.0027
0.021
0.7
0.81
0.0098
0.7
0.0013
0.87
0.84
0.0171
0.63
0.0309
0.025
0.0088
0.1
0.5
0.028
0.81
0.0412
0.02
0.1
0.0427
0.44
0.018
0.158
0.7
0
0.012
0.6
0.8
0.9
1.2
2.4
0.14
1.3
0.033
0.017
0.95
1.4
0.56
1.3
0.22
0.59
0.78
0.033
2
1.6
0.03
0.24
0.027
2.2
0.2
0.01
0.048
1.6
1.4
0.01
1.4
0.85
1
1.7
2.7
2.4
4.9
1.6
2.9
6.0
3.6
1.6
3.5
1.8
2.3
2.5
3.9
3.1
1.7
5.7
4.5
2.6
2.1
1.9
2.1
2.9
2.5
2.0
3.1
3.6
3.6
1.3
2.9
2.7
2.9
13.0
3.6
14.8
4.0
4.5
1.2
2.2
5.6
1.6
0.092
0.041
0.226
0.018
0.076
0.11
0.047
0.107
0.064
0.091
0.06
0.083
0.135
0.064
0.053
0.107
0.074
0.11
0.068
0.215
0.062
0.089
0.06
0.079
0.03
0.07
0.085
0.107
0.037
0.04
0.104
0.054
0.029
0.149
0.021
0.075
0.054
0.097
0.435
0.133
0.081
482
964
410
1903
595
440
1207
694
897
897
781
834
742
1003
1063
516
850
865
1101
482
1032
437
584
509
825
519
491
438
744
653
406
592
824
388
1160
1230
1449
919
434
929
1106
3.9E-05
3.6E-05
6.1E-05
1.9E-05
5.9E-05
3.4E-05
5.6E-05
3.4E-05
7.9E-05
8.0E-05
8.5E-05
1.6E-04
3.5E-05
1.4E-05
5.6E-05
5.3E-06
1.2E-05
1.3E-05
5.5E-05
5.5E-05
6.7E-05
1.5E-05
1.8E-05
1.8E-05
4.6E-05
2.8E-05
1.4E-05
2.5E-05
2.5E-05
1.7E-05
2
2
4
3
3
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
4
2
2
2
3
2
3
2
3
2
2
2
2
1
1
1
1
3
1
NoObs
NoObs
1
NoObs
1
1
1,2,3
1,2,3
1,2,3
3
3
3
1,2,3
3
3
1,2,3
3
3
NoObs
NoObs
1
1
1
1,2
64
263.01 4.1456
265.01 3.1809
268.01 12.0373
269.01 6.1397
270.01 5.9033
270.02 8.3939
271.01 6.9832
271.02 6.9360
273.01 1.8180
274.01 4.5111
275.01 7.0060
276.01 4.6992
277.01 7.6827
279.01 8.0747
279.02 6.4306
280.01 2.5779
281.01 8.0749
282.01 5.8542
282.02 3.2310
283.01 3.3342
284.01 2.7486
284.02 3.4231
284.03 3.2542
285.01 5.8394
288.01 6.2875
289.01 7.8380
291.01 7.3578
291.02 2.1775
292.01 2.2814
294.01 5.5281
295.01 2.8818
296.01 5.2805
297.01 2.9110
298.01 2.6557
299.01 1.9962
301.01 3.8551
302.01 8.6779
303.01 6.3927
304.01 2.6128
305.01 2.3541
306.01 2.9825
165
88
486
89
105
139
312
338
281
61
156
429
421
1369
213
341
284
648
73
460
173
107
106
406
202
453
339
140
219
422
277
437
123
259
312
184
540
762
604
416
550
13 117.7331
19 102.7477
68 108.9277
25 118.0993
32
108.033
31
95.044
43 105.5501
66 142.0721
49 108.0667
14 108.9264
32 109.8237
58 143.4006
93 104.6804
176 109.70148
31
69.9418
80 113.89515
57 122.0403
112 115.1037
18
72.0688
37 103.5999
20
112.423
23 102.6342
23 101.8617
30 112.2811
57 110.2711
52 124.9949
38 118.1545
16
67.1034
48 104.8415
32 126.0347
19 104.8769
25 111.4863
21 105.2745
17
111.308
51 103.5428
34
104.716
52 106.9965
64 106.3643
58 107.9095
36 104.8397
12 111.3658
0.0086
0.0036
0.0032
0.0059
0.0043
0.0059
0.0041
0.0022
0.0012
0.0072
0.0048
0.0023
0.0018
0.00091
0.0054
0.00098
0.0029
0.0014
0.0048
0.0028
0.0037
0.0039
0.0036
0.0054
0.0026
0.0026
0.0041
0.0048
0.0015
0.0037
0.0018
0.0038
0.0035
0.0039
0.0012
0.0029
0.0031
0.0021
0.0016
0.0022
0.0068
20.7183
3.567971
110.3742
18.01136
12.58084
33.67205
48.6292
29.39292
10.573667
15.09124
15.79142
41.74523
16.23675
28.45557
15.41304
11.87286
19.55687
27.50882
8.45735
16.09173
18.01109
6.41508
6.17824
13.74872
10.2754
26.62907
31.51605
8.12993
2.58665
34.4361
5.317406
28.8605
5.65189
19.96343
1.541677
6.00245
24.85467
60.92983
8.511982
4.603576
24.3077
0.0013
0.000083
0.003
0.00073
0.00036
0.00087
0.0014
0.00036
0.000089
0.00055
0.00077
0.00077
0.00021
0.00019
0.00034
0.000081
0.00048
0.00026
0.00017
0.00031
0.00046
0.00017
0.00015
0.00052
0.00019
0.00054
0.00086
0.00017
0.000037
0.001
0.000085
0.0017
0.00019
0.00059
0.000013
0.00011
0.00051
0.00085
0.000093
0.000072
0.0013
40.1
8.67
61
12
16.01
31.08
33
32.9
46.9
12
14
47
16.85
24.1
13
16.6
13
26
20
20
19.8
8
7
13
12.72
26.43
33.08
28
9
35
7
30
8
29
3.8
11.91
22.35
48
18
12
71.9
2.3
0.27
73
30
0.34
0.65
48
9.9
1
63
30
65
0.1
8.6
30
5
14
15
124
28
5.9
26
27
29
0.15
0.33
0.58
197
20
83
33
96
27
146
9.7
0.27
0.23
35
35
29
5.5
0.01143
0.0087
0.0205
0.0099
0.00925
0.01051
0.0181
0.01655
0.01548
0.0089
0.0118
0.0207
0.01945
0.0346
0.0147
0.02031
0.0163
0.0251
0.008
0.0237
0.01509
0.0117
0.0112
0.0201
0.01287
0.01911
0.01626
0.012
0.0139
0.0195
0.017
0.02
0.0126
0.017
0.0176
0.01253
0.02266
0.0277
0.0249
0.02
0.0232
0.00058
0.00024
0.0041
0.0037
0.00018
0.00022
0.0042
0.00021
0.00028
0.0067
0.0045
0.0048
0.00012
0.0022
0.0068
0.00023
0.0031
0.0027
0.01
0.0053
0.00058
0.0062
0.0063
0.008
0.00014
0.00023
0.00027
0.017
0.0057
0.008
0.012
0.011
0.0067
0.014
0.0076
0.00024
0.00024
0.0036
0.0079
0.011
0.0014
0.021
0.012
0.5
0.8
0.01
0.017
0.79
0.016
0.9
0.6
0.75
0.029
0.5
0.7
0.82
0.71
0.72
0.2
0.89
0.88
0.9
0.9
0.7
0.0046
0.007
0.016
0.4
0.2
0.7
0.9
0.7
0.8
0.9
0.8
0.029
0.02
0.77
0.8
0.7
0.011
0.054
0.036
1.1
1
0.01
0.01
0.87
0.033
1.2
1.4
0.93
0.022
0.62
1.3
0.25
0.87
0.64
2.9
0.65
0.26
1.1
1.1
1.2
0.017
0.014
2.9
1.7
1.4
1.2
1.4
1.2
1.3
1.1
0.044
0.02
0.64
0.98
1.4
0.022
1.5
1.1
1.8
1.7
0.9
1.0
2.0
1.8
1.1
1.1
1.2
2.6
2.1
4.9
2.1
3.1
3.7
2.8
0.9
4.7
2.5
2.0
1.9
2.1
1.5
2.0
1.5
1.0
2.0
2.2
2.0
2.4
1.8
1.7
3.6
1.6
3.8
2.9
5.0
2.5
3.6
0.151
0.047
0.406
0.143
0.101
0.195
0.269
0.192
0.093
0.124
0.121
0.244
0.124
0.191
0.127
0.108
0.152
0.178
0.081
0.132
0.141
0.071
0.069
0.11
0.093
0.171
0.196
0.079
0.038
0.213
0.06
0.189
0.065
0.136
0.028
0.067
0.179
0.306
0.087
0.053
0.168
682
1303
295
918
735
529
520
615
655
805
717
569
723
708
868
1018
930
620
919
930
859
1211
1228
757
878
604
495
780
1478
565
1088
619
1192
610
2002
1142
873
426
1199
963
657
8.0E-06
3.2E-05
1.6E-05
2.3E-05
4.8E-05
1.2E-05
1.2E-05
2.3E-05
1.7E-05
1.3E-05
1.5E-05
1.7E-05
1.4E-05
1.8E-05
2.7E-05
2.3E-05
2.2E-05
1.8E-05
2.2E-05
2.3E-05
2.7E-05
2.8E-05
1.2E-05
5.1E-05
1.5E-05
4.5E-05
1.3E-05
1.3E-05
1.5E-05
2.2E-05
3.1E-05
7.7E-05
5.8E-05
3.3E-05
1.7E-05
1.4E-04
8.5E-05
3
2
2
2
2
4
2
3
2
3
2
2
2
2
4
2
2
2
4
2
2
3
3
2
2
2
2
4
2
2
2
2
2
3
2
2
2
2
2
2
2
1,2,3
1,2,3
1
1
1,2
1,2
1,2,3
1,2
1,2,3
1,2,3
1,2,3
1
1
1
1
1
1
1,2
1
1,2
1,2,3
1,2
1,2
1,2
1
1
1
1
1,2
1
1
1
1
NoObs
1
1
1
1
1
1,2
65
307.01
308.01
312.01
313.01
313.02
314.01
314.02
315.01
316.01
317.01
318.01
319.01
321.01
323.01
326.01
327.01
330.01
331.01
332.01
333.01
335.01
337.01
338.01
339.01
339.02
340.01
341.01
341.02
343.01
343.02
344.01
345.01
346.01
348.01
349.01
350.01
351.01
351.02
351.03
352.01
353.01
3.6490
6.3242
2.7215
3.1424
3.2232
2.4517
2.0157
4.3681
5.0479
7.2681
10.3373
5.3951
2.5947
3.3770
2.9995
2.9306
5.2342
6.3739
3.8993
6.0214
7.4741
5.3936
2.9400
2.4238
3.1373
14.2340
2.9799
2.7109
3.3150
2.4768
5.8847
4.8165
2.7973
4.6221
2.3194
2.5804
14.4207
11.9806
8.0060
4.4932
7.0683
224
754
197
547
320
747
558
979
524
427
1286
1793
174
592
890
147
281
355
221
345
763
324
293
286
167
21220
796
300
474
234
1113
1246
989
1888
582
397
8331
4236
460
393
3685
24
55
24
36
33
42
21
68
56
44
44
137
39
11
26
30
27
32
40
24
53
25
27
44
17
172
31
14
68
47
70
79
20
108
38
24
210
60
21
21
93
109.2686
120.5441
108.586
110.6353
112.8879
110.852
103.9994
121.9796
117.9011
139.3631
107.8303
109.6254
103.4551
102.8509
104.0345
105.6621
107.5328
103.8303
105.0885
102.8642
129.3109
110.7155
107.5777
103.1393
71.3385
93.6222
109.6648
110.6123
103.3364
103.4963
104.3354
106.1889
103.7797
120.3634
103.4557
110.2199
73.4753
80.098
91.9518
124.8039
109.5299
0.004
0.0024
0.0036
0.0022
0.0026
0.0015
0.0028
0.0017
0.002
0.003
0.0025
0.001
0.002
0.0073
0.0031
0.0025
0.0048
0.0047
0.0028
0.0039
0.0024
0.004
0.0033
0.0017
0.0052
0.0073
0.0026
0.0054
0.0013
0.0018
0.0018
0.0015
0.0045
0.0012
0.0019
0.0027
0.0012
0.0015
0.0078
0.0049
0.0019
19.67445
35.59061
11.57898
18.73564
8.43628
13.78105
23.0904
35.5917
15.77135
22.20767
38.58439
46.15115
2.426307
5.83674
8.97297
3.254241
7.97398
18.68416
5.458491
13.28468
46.56623
19.78404
7.01048
1.980349
6.41681
23.67378
7.17068
4.69975
4.76166
2.024138
39.3095
29.88569
12.92463
28.51109
14.38666
12.99192
331.6457
210.4526
59.7389
27.08268
152.1011
0.00055
0.00058
0.00029
0.00031
0.00015
0.00016
0.00034
0.00045
0.00022
0.0006
0.00038
0.00034
0.000032
0.00029
0.0002
0.000056
0.00025
0.00059
0.0001
0.00025
0.00083
0.00042
0.00016
0.000031
0.00015
0.00058
0.00013
0.00012
0.000044
0.000025
0.00054
0.00055
0.00041
0.00027
0.00025
0.00033
0.0017
0.0021
0.0022
0.00098
0.0027
42.2
22
33.1
25
14
24.2
73
41
18
18
29.99
54
7.27
14.5
19
8.974
7
22.47
11.27
17.1828
45
28.67
19.24
3.9
16.6
14.366
19.09
14.3
11.21
6.593
42
37
36
51.65
51.7
22
190.34
142.4
53
28
95.2
1.4
8
1.1
37
39
7.3
680
30
26
33
0.45
16
0.16
1.2
80
0.082
17
0.48
0.22
0.0013
95
0.78
0.66
9.1
0.19
0.071
0.54
0.8
0.14
0.042
49
32
241
0.43
1.4
96
0.16
1.6
713
85
8.3
0.01374
0.0281
0.01322
0.0254
0.0178
0.02918
0.023
0.0325
0.0221
0.0199
0.03035
0.04055
0.01226
0.021
0.029
0.01156
0.0174
0.01684
0.01399
0.02
0.0257
0.01613
0.01587
0.0175
0.01286
0.12942
0.02618
0.01781
0.01969
0.0147
0.0318
0.0351
0.03
0.03813
0.02231
0.02
0.0827
0.05855
0.019
0.02
0.064
0.0004
0.0016
0.00037
0.0068
0.0095
0.00058
0.039
0.0049
0.0056
0.0058
0.00048
0.00022
0.00022
0.0014
0.023
0.00024
0.0071
0.00034
0.00022
0.13
0.0093
0.00043
0.00043
0.0064
0.00043
0.00052
0.0006
0.00077
0.0002
0.00021
0.0067
0.0063
0.045
0.00026
0.00044
0.014
0.0064
0.00061
0.044
0.01
0.0012
0.008
0.88
0.015
0.87
0.7
0.74
0.7
0.81
0.7
0.6
0.03
0.39
0.0016
0.03
0.6
0.0593
0.8
0.012
0.0377
0.011
0.4
0.011
0.011
0.8
0.0625
0.001
0.027
0.011
0.0089
0.041
0.6
0.72
0.1
0.018
0.028
0.9
0.011
0.001
0.4
0.8
0.88
0.01
0.34
0.037
0.72
1.3
0.22
2.5
0.59
1.1
1.2
0.036
0.12
0.085
1.9
1.1
0.01
0.01
1.6
0.01
0.035
1.1
0.01
0.042
0.046
1
0.76
3.1
0.017
0.04
1.3
0.035
0.069
4
1.2
0.17
1.7
4.7
1.6
3.1
2.2
1.9
1.6
4.8
2.8
3.7
4.4
4.3
0.9
2.9
0.9
1.3
2.5
1.1
1.1
1.9
4.3
1.6
2.3
1.5
1.1
30.4
3.3
2.3
2.2
1.6
4.0
5.8
3.4
5.3
2.8
2.5
8.5
6.0
1.9
2.4
8.2
0.148
0.223
0.102
0.139
0.081
0.091
0.128
0.211
0.126
0.166
0.235
0.248
0.035
0.065
0.05
0.044
0.081
0.134
0.06
0.114
0.269
0.146
0.072
0.031
0.069
0.173
0.074
0.056
0.057
0.032
0.232
0.192
0.106
0.18
0.119
0.111
0.966
0.713
0.308
0.181
0.589
736
699
867
651
852
446
376
526
750
918
671
508
1068
1051
332
1304
1021
494
841
843
674
636
940
1319
884
862
949
1091
1065
1421
564
592
684
549
772
810
266
309
471
621
417
5.2E-05
3.3E-05
6.6E-05
1.3E-05
1.7E-05
2.3E-05
2.3E-05
4.6E-05
1.4E-05
9.9E-05
1.2E-05
1.7E-05
1.3E-05
1.4E-05
2.5E-05
3.3E-05
4.0E-05
4.7E-05
2.6E-05
2.3E-05
6.3E-05
5.7E-05
1.8E-05
4.5E-05
5.7E-05
2.9E-05
3.4E-05
1.0E-05
9.9E-06
4.0E-05
1.0E-05
1.3E-05
1.4E-05
1.9E-05
5.9E-05
1.5E-05
3
2
2
2
2
2
2
2
3
3
3
2
2
2
3
2
3
2
2
2
2
3
3
3
4
3
2
2
2
2
2
2
2
2
2
2
3
4
4
2
2
1
1
1
1,2,3
1,2
1
1
1
1,2
1
1
1
1
NoObs
1
NoObs
1
1
1
NoObs
NoObs
NoObs
NoObs
1
1
1
NoObs
1
1
NoObs
NoObs
1
NoObs
1
NoObs
NoObs
66
354.01 4.5028
355.01 2.8403
356.01 2.1029
360.01 4.5515
361.01 2.5126
364.01 4.5649
365.01 6.6552
366.01 4.9911
367.01 2.8404
368.01 12.7602
369.01 1.8748
370.01 9.7635
371.01 10.1954
372.01 9.1846
373.01 8.7090
374.01 11.2542
375.01 7.0221
377.01 4.5242
377.02 5.0267
377.03 1.7745
379.01 2.5183
384.01 5.0735
385.01 3.4446
386.01 5.3012
386.02 5.9833
387.01 3.3365
388.01 5.3710
392.01 7.3677
393.01 6.7617
398.01 4.7975
398.02 2.4429
398.03 1.7407
401.01 5.3596
401.02 6.2359
403.01 1.5859
408.01 3.1757
408.02 3.7260
408.03 5.0363
409.01 4.3307
410.01 1.8788
412.01 3.0251
473
32 104.5198
304
38 105.8966
1195 143 103.52521
150
15 104.5813
191
24 104.2741
451
28 156.9082
638
83 144.6778
3808 271 140.7142
2267 176 110.20526
7307 1409 130.36472
143
19 107.4265
348
46 136.6501
1202
58 177.0753
8267
46
186.349
648
35 123.9263
646
44 169.9597
5087 121 172.22424
7507 129 115.66381
6754
83 108.4011
244
22 115.0924
273
24 103.9955
191
30 107.4333
292
19 107.8373
917
46
106.905
716
24 133.6702
1021
32 115.8646
290
34 102.5496
235
14
104.316
249
21 109.2556
9436 155
103.085
1704
74 106.7183
492
28
66.8188
2154 100 118.4415
1531
30 184.2868
1309
41 104.1305
1485
63 106.0728
869
31
99.7951
734
20
85.9989
632
49 112.5253
4057 211 109.28616
3615 226 103.32514
0.0034
0.0021
0.00051
0.0051
0.0031
0.0022
0.0019
0.00036
0.00049
0.0002
0.003
0.0035
0.0048
0.0044
0.005
0.0038
0.00095
0.00078
0.0014
0.0059
0.003
0.0036
0.0042
0.0029
0.0064
0.003
0.0035
0.01
0.0066
0.001
0.0015
0.0024
0.0013
0.0049
0.0016
0.0015
0.0039
0.0061
0.0025
0.00033
0.00037
15.95999
4.903454
1.8270789
5.94042
3.247565
173.9
81.7378
75.1119
31.57867
110.32148
5.88521
42.8821
278
125.6125
135.1937
172.6735
220
19.25832
38.9116
1.592928
6.71743
5.07977
13.14613
31.15847
76.735
13.89952
6.14974
33.4205
21.41586
51.84581
4.180054
1.729364
29.19859
160.0112
21.0569
7.381987
12.56093
30.82869
13.24874
7.216812
4.147024
0.00037
21
0.000074
10
0.0000064
6
0.00063
9.13
0.000069
10.37
1.6
132
0.0015
64
0.00021
77.4
0.00011
98
0.00015
51.53
0.00013
20
0.0012
21
1488
65
0.0064
111
0.0072
92
0.0051
96
- 150.80509
0.00017
32
0.0006
36.2
0.000068
7
0.00014
13
0.00012
4.7
0.0004
30
0.00063
47.12
0.0034
101.1
0.0003
28
0.00015
10
0.0024
35.4
0.00096
19
0.00033
80
0.000043
13.67
0.000018
6.9
0.00029
45.63
0.0069
114
0.00024
31.9
0.000074
18.92
0.00034
25.58
0.00088
49
0.00024
17
0.000017
14.5
0.00001 11.416
51
25
6.3
0.41
0.37
39
44
3.8
108
0.31
90
20
20
65
142
124
6.4
2.9
41
54
9.5
151
0.75
3.2
98
158
1.6
72
14
0.27
2.1
0.38
43
9.6
0.29
0.69
315
34
4.4
0.052
0.0217
0.0179
0.0328
0.01108
0.01302
0.02395
0.0251
0.06441
0.0438
0.08456
0.0116
0.0194
0.2
0.0813
0.025
0.0243
0.07725
0.0776
0.0839
0.014
0.018
0.015
0.016
0.02782
0.02374
0.031
0.006
0.01417
0.0152
0.092
0.03726
0.02047
0.041
0.0434
0.35598
0.03466
0.02735
0.024
0.0247
0.1016
0.05341
0.0094
0.0077
0.0071
0.00046
0.00038
0.00058
0.0032
0.00061
0.0085
0.00008
0.0089
0.003
3.8
0.0093
0.0067
0.0055
0.003
0.0017
0.016
0.012
0.0051
0.016
0.00038
0.00071
0.02
0.017
0.00061
0.0097
0.0036
0.00056
0.00065
0.00028
0.0034
0.00096
0.00041
0.00062
0.032
0.0098
0.005
0.00019
0.7
0.7
0.59
0.03
0.0439
0.84
0.75
0.83
0.6
0.715
0.5
0.8
1.3
0.17
0.7
0.6
0.8738
0.56
0.88
0.2
0.8
0.8
0.2
0.029
0.011
0.5
0
0.013
0.6
0.57
0.0002
0.218
0.0002
0.9
1.74
0.0189
0.011
0
0.7
0.97
0.0011
1.3
1.4
0.99
0.066
0.25
0.66
0.15
1
0.064
2.2
0.69
0.39
0.9
1.1
1.1
0.44
0.16
2.9
1 .3
1
2.6
0.036
0.04
1.9
4.8
0.042
1.8
0.41
0.065
0.32
0.52
0.01
3
1.2
0.29
-
4.9
2.0
5.8
1.3
1 .3
2.6
2.3
10.2
5.7
17.4
1.3
4.9
60.1
8.5
3.5
3.3
8.8
5.7
6.2
1.0
3.1
2.0
1.8
3.4
2.9
2.5
0.6
1.9
1.2
8.6
3.5
1.9
6.2
6.6
39.7
3.6
2.9
2.6
1.4
12.4
7.3
0.134
0.058
0.03
0.065
0.044
0.619
0.368
0.4
0.203
0.544
0.066
0.262
0.916
0.499
0.534
0.628
0.729
0.141
0.225
0.027
0.074
0.06
0.11
0.2
0.366
0.1
0.063
0.209
0.154
0.267
0.05
0.028
0.19
0.591
0.152
0.075
0.108
0.196
0.108
0.076
0.052
1034
1115
1655
1075
1132
313
363
586
646
742
1073
810
400
344
400
365
300
553
438
1264
1267
1143
743
623
461
534
925
614
578
403
932
1246
629
357
637
889
741
550
545
1009
1211
2.6E-05
3.2E-05
2.4E-05
2.8E-05
2.7E-05
1.7E-05
1.5E-05
1.3E-05
3.6E-06
6.1E-06
1.5E-05
2.4E-05
5.1E-06
2.0E-05
3.9E-05
2.1E-05
9.7E-06
1.8E-05
2.1E-05
3.6E-05
6.8E-05
1.2E-04
7.7E-05
9.3E-05
9.7E-05
2.8E-05
4.1E-05
4.6E-05
1.2E-04
1.4E-05
2.3E-05
2.5E-05
1.0E-05
4.4E-05
5.0E-05
4.6E-05
1.6E-05
2
2
2
3
2
3
2
2
2
2
2
2
3
2
2
2
2
1
1
1
3
2
2
2
2
2
2
3
2
2
2
4
2
4
3
2
2
4
2
2
2
1
1
NoObs
1
1
1,2
NoObs
1
1
1
NoObs
NoObs
1,2,3
1,2
1
1
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
3
3
NoObs
1
1
67
1
1
1
413.01 2.6270
415.01 7.0021
416.01 3.7319
416.02 4.0059
417.01 2.4571
418.01 4.8665
419.01 2.7205
420.01 2.2582
421.01 2.6993
422.01 9.0034
423.01 6.0128
425.01 1.5268
426.01 3.4978
427.01 2.9072
428.01 6.8663
429.01 4.0370
430.01 2.7448
431.01 3.1580
431.02 3.8717
432.01 2.1018
433.01 2.8751
433.02 11.7758
435.01 5.4169
438.01 2.3764
439.01 2.1891
440.01 4.0463
440.02 1.6038
442.01 4.4306
442.02 2.3333
443.01 4.7403
444.01 4.0665
446.01 2.7087
446.02 3.7173
448.01 2.8620
448.02 5.0051
452.01 5.0013
454.01 4.6580
456.01 4.2628
456.02 2.9208
457.01 1.8924
458.01 4.0333
1023
4827
1645
1143
6728
12155
7678
2700
17361
17493
9104
12252
907
1812
3825
2892
1720
1128
833
1041
2960
12968
1558
940
2240
984
748
426
188
745
469
857
609
1263
2340
458
831
1093
241
742
3343
34
118
83
32
185
610
292
195
687
274
241
122
36
44
361
150
52
44
24
72
104
195
57
42
201
41
36
26
23
44
29
23
14
27
33
50
23
51
18
40
60
109.5582
178.1412
118.8413
86.78
109.96607
105.79613
122.38996
107.08404
105.81931
183.63055
135.856
102.75274
105.1505
124.7364
105.51811
105.52804
112.4041
111.7122
87.3073
107.35008
104.09249
132.2029
111.9483
107.7956
103.44904
110.9313
103.8861
104.6832
67.5316
113.0459
110.3174
107.7539
118.4722
111.4491
127.4625
102.9417
103.5546
104.4739
67.0265
107.2985
141.0775
0.0025
0.0014
0.0013
0.0033
0.00044
0.00023
0.0003
0.0004
0.00025
0.00071
0.00051
0.00034
0.0027
0.002
0.00049
0.00079
0.0016
0.002
0.0045
0.0009
0.00084
0.0013
0.0019
0.0017
0.00038
0.0023
0.0015
0.0043
0.0036
0.0027
0.0039
0.0032
0.0066
0.0033
0.0037
0.0025
0.0047
0.0023
0.0054
0.0017
0.0018
15.22926
166.7879
18.20811
88.2547
19.193112
22.418338
20.13146
6.010401
4.4542074
200
21.087391
5.428352
16.30089
24.6157
6.873163
8.600087
12.37645
18.86998
46.90198
5.263436
4.03042
328.2403
20.54902
5.931204
1.9022064
15.90655
4.973444
13.53981
1.732341
16.21718
11.7228
16.70916
28.5532
10.13961
43.6205
3.705996
29.008
13.70035
4.30954
4.921331
53.71858
0.00027
0.0019
0.00017
0.0013
0.000062
0.000036
0.000044
0.000017
0.000009
0.024
0.000085
0.000013
0.00035
0.00034
0.000023
0.000048
0.00019
0.00031
0.00094
0.000033
0.000023
0.0019
0.00033
0.00007
0.000005
0.00027
0.00005
0.00041
0.000026
0.0003
0.00031
0.00036
0.0015
0.00023
0.0013
0.000064
0.001
0.00023
0.0001
0.000057
0.00079
47.8
229.111
38.65
115
36
24.82
42
21
16.852
136.12
29.034
15
37.91
38
8.103
17.1
33
36
51
14
11
176.2
29.53
16
5.8
22
23.7
23.22
6.29
26.46
22
32
59
28.6
45
5.758
40
25.57
13.06
13
49
1.4
0.016
0.11
200
11
0.36
13
17
0.036
0.016
0.097
4.2
0.94
11
0.017
0.1
80
84
68
24
19
8.4
0.4
39
4.1
47
0.77
0.68
0.2
0.44
114
129
364
1.2
38
0.08
156
0.38
0.56
40
15
0.02991
0.062
0.03601
0.035
0.0972
0.11484
0.09084
0.0474
0.11481
0.13831
0.08496
0.133
0.02709
0.0457
0.05591
0.04762
0.038
0.033
0.032
0.0321
0.049
0.1133
0.0352
0.03
0.0447
0.031
0.02488
0.01862
0.01435
0.02481
0.02
0.03
0.022
0.03002
0.0488
0.01956
0.027
0.03051
0.01621
0.028
0.0768
0.00062
0.063
0.00028
0.012
0.0017
0.00044
0.00037
0.0081
0.00018
0.00025
0.014
0.00055
0.001
0.0001
0.00023
0.018
0.015
0.008
0.0096
0.018
0.0013
0.00041
0.016
0.0063
0.014
0.00048
0.00048
0.00037
0.00037
0.019
0.025
0.031
0.00094
0.0088
0.00025
0.022
0.00039
0.00054
0.017
0.0062
0.042
0.006
0.0038
0.78
0.84
0.803
0.65
0.39
0.001
0.8077
0.0003
0.9
0.029
0.75
0
0.027
0.4
0.7
0.88
0.7
0.3
0.73
0.003
0.6
0.56
0.7
0.031
0.008
0.06
0.0056
0
0.8
0.2
0.013
0.79
0.0028
0.6
0.009
0.0615
0.8
0.93
0.01
0.01
0.97
0.25
0.085
0.19
1
0.26
0.01
0.22
0.01
0.017
1.7
1.3
0.66
1.1
1.5
0.18
0.01
1.4
0.83
1.2
0.048
0.01
2.7
1.5
2.9
0.04
0.67
1.9
0.022
1.3
0.28
2.8
7.7
2.9
2.8
9.0
12.7
7.5
4.3
14.5
16.5
9.6
13.2
3.5
4.6
5.6
4.8
2.7
3.6
3.5
3.6
5.8
13.4
3.0
2.2
2.7
2.8
2.2
1.9
1.4
2.2
2.0
2.3
1.7
2.3
3.8
2.3
2.4
3.1
1.7
2.2
10.5
0.119
0.611
0.131
0.376
0.142
0.155
0.146
0.061
0.053
0.692
0.154
0.061
0.13
0.165
0.073
0.081
0.087
0.139
0.254
0.061
0.05
0.935
0.148
0.056
0.029
0.12
0.055
0.113
0.029
0.127
0.103
0.115
0.164
0.079
0.21
0.048
0.181
0.114
0.053
0.054
0.286
619
352
536
317
608
580
573
763
1068
333
685
967
773
554
959
760
493
622
460
1049
1076
249
579
668
1014
576
850
722
1425
631
763
490
411
564
346
1242
487
714
1047
799
515
1.2E-04
2.8E-05
2.4E-05
3.9E-05
3.1E-05
1.1E-05
1.4E-05
3.9E-05
1.4E-05
2.7E-05
4.2E-05
1.1E-05
4.1E-05
4.3E-05
1.4E-05
1.2E-05
2.3E-05
4.7E-05
2.2E-05
2.3E-05
2.5E-05
7.2E-05
9.6E-05
8.2E-05
3.7E-05
8.4E-05
2.4E-05
2.6E-05
1.7E-04
1.5E-04
6.7E-05
2.8E-05
2.9E-05
3.2E-05
1.1E-05
2
2
2
4
2
2
2
2
2
2
2
2
2
2
2
3
2
2
4
2
3
4
2
2
2
2
2
2
4
2
2
2
2
2
2
2
2
2
4
2
3
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
68
459.01
459.02
460.01
463.01
464.01
464.02
465.01
466.01
467.01
468.01
469.01
470.01
471.01
472.01
473.01
474.01
474.02
475.01
475.02
476.01
477.01
478.01
479.01
480.01
481.01
481.02
481.03
483.01
484.01
486.01
487.01
488.01
490.01
490.03
492.01
494.01
496.01
497.01
497.02
499.01
500.01
3.5933
3.3100
4.2947
2.2233
6.3270
2.2822
7.8994
2.1253
4.8878
3.2229
1.5075
1.9936
3.6749
3.4034
2.3654
3.1718
3.3543
2.5576
2.8820
2.9423
3.7966
1.7873
5.3442
2.0071
2.7127
1.6900
4.8919
3.0292
3.6637
5.1182
3.0191
3.3557
2.3764
2.8056
6.3675
3.7520
1.5390
4.9474
3.6013
2.4759
2.5052
976
157
1445
2830
5551
725
1609
2724
3161
1547
2449
2462
505
1464
884
535
447
756
888
743
825
1908
1106
736
988
421
1044
827
1050
678
653
470
415
391
889
1039
408
560
161
405
1457
47
13
64
60
162
42
25
71
129
48
80
140
24
85
36
32
17
27
26
22
28
62
48
37
56
42
38
50
38
31
26
17
12
26
34
26
8
32
13
24
51
103.1027
67.1191
109.0751
118.2658
129.55353
128.7576
137.0202
103.53919
115.4428
107.5957
107.60632
104.15067
104.7317
106.5627
113.6359
109.72
67.7739
109.7
104.7906
111.4386
102.6428
104.1148
126.387
105.3089
104.969
102.8291
116.228
106.2564
108.059
102.4949
106.0424
109.447
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177
31.7
29.66
58.1
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9.95
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47
25.89
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40
28
21.4
41
14
19
7
28
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36.19
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21.02
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10
13
38.59
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5
15
6
18
22.62
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0.25
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0.36
74
53
9.5
0.19
1.2
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58
0.11
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154
188
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6.4
85
51
40
17
14
18
0.83
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2
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2
4
2
2
2
2
3
2
2
2
2
2
2
2
2
3
3
3
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2
2
3
2
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2
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1
1
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500.02
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501.01
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509.02
510.01
510.02
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512.01
513.01
517.01
518.01
518.02
519.01
520.01
520.02
520.03
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522.01
523.01
523.02
524.01
525.01
526.01
528.01
528.02
528.03
530.01
531.01
532.01
533.01
534.01
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434
532
289
490
1414
680
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727
1578
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856
912
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534
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514
868
753
1006
570
592
886
282
725
1302
1131
3388
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1002
1205
926
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961
718
567
2812
629
661
752
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67.025
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67.5914
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66.1708
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132.256
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107.809
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70.3827
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105.921
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71.3679
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11.53
11
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23
24.44
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39.7
12.11
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12
27
9
23
5
12
19.76
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39.22
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36.78
57
16
19
11
62
23
35.55
43.4
39.6089
15.85
52
6
17
130.6
61
40.2
26
11.06
32.7
17
83
0.6
51
19
123
0.6
1.8
1.4
0.26
150
23
84
24
94
16
46
0.4
90
0.74
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0.72
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41
62
396
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0.15
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2
10
44
3.9
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3.6
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4
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2
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2
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2
2
2
4
2
2
2
3
2
2
2
2
2
2
4
4
3
2
2
4
2
2
2
2
4
4
2
3
2
2
2
1
1
1
1
1
NoObs
1
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1100
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448
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753
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842
2224
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3528
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876
897
753
214
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3079
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66.5566
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102.64
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107.316
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109.9
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66.3315
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112.774
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0.000089
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0.00018
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0.00067
60.2
0.00013
26
0.00015
40
0.000038
9
0.00042
16.33
0.00011
14
0.000042
8.378
0.0004
41
0.0012
32
0.46
0.089
0.0072
18
38
89
1.8
0.52
0.68
0.66
0.56
111
0.64
75
1.1
2.6
1.3
31
3.3
92
128
3.5
234
33
65
0.5
0.58
682
23
73
682
66
3.3
106
1.2
17
0.39
52
0.08
162
165
0.02015
0.02989
0.03241
0.022
0.0255
0.025
0.02195
0.02529
0.02041
0.02575
0.04137
0.026
0.02143
0.025
0.02122
0.0967
0.0687
0.018
0.02676
0.028
0.025
0.0137
0.028
0.024
0.017
0.02326
0.04929
0.024
0.0286
0.023
0.022
0.016
0.02221
0.024
0.02827
0.026
0.01827
0.025
0.01674
0.031
0.024
0.00059
0.00023
0.011
0.0082
0.02
0.00066
0.00057
0.00067
0.0006
0.00043
0.016
0.00047
0.018
0.00074
0.0013
0.0034
0.015
0.00079
0.019
0.019
0.0011
0.039
0.013
0.012
0.00051
0.00037
0.058
0.0075
0.013
0.043
0.012
0.00096
0.015
0.00067
0.007
0.00045
0.018
0.00053
0.025
0.022
0.0291
0.0075
0.4793
0.7
0.8
0.8
0.023
0.0378
0.0847
0.003
0.0096
0.7
0.032
0.7
0.0662
0.79
0.9
0.8
0.041
0.5
0.1
0.29
0.6
0.7
0.7
0.019
0.013
0.2
0.82
0.8
0.1
0.6
0.017
0.1
0.0141
0.87
0.024
0.3
0.0437
0.4
0.7
1.4
1
1.5
0.028
0.01
1.7
0.01
1.6
0.24
0.25
1.5
0.039
1.8
2.3
0.087
2.4
1.4
1.7
0.01
0.04
4.3
0.83
1.3
3.8
1.9
0.01
2.4
0.8
0.01
2.1
2.1
1.9
1.4
3.3
3.0
1.4
2.9
1.9
2.7
1.9
1.5
2.8
3.5
2.6
1.8
2.1
1.8
11.2
6.1
1.5
2.3
3.1
2.3
1.4
1.8
2.1
1.8
2.4
5.0
2.3
2.9
2.3
2.2
1.0
2.1
1.7
2.0
1.8
2.4
3.2
2.1
2.4
2.6
0.037
0.065
0.588
0.039
0.155
0.11
0.241
0.05
0.041
0.152
0.164
0.155
0.109
0.101
0.063
0.043
0.047
0.046
0.376
0.121
0.085
0.052
0.154
0.058
0.124
0.152
0.505
0.175
0.096
0.147
0.187
0.043
0.144
0.059
0.088
0.039
0.097
0.066
0.033
0.14
0.169
936
1011
296
1003
683
603
526
844
932
673
489
654
660
688
871
1316
1068
947
331
636
730
981
445
829
734
619
340
586
758
612
543
856
540
563
461
692
882
1054
1491
507
640
6.8E-05
5.4E-05
1.7E-05
2.0E-05
3.6E-05
3.0E-05
3.5E-05
3.5E-05
2.8E-05
2.8E-05
2.4E-05
1.1E-04
1.3E-04
6.9E-05
3.4E-05
8.0E-05
2.8E-05
1.8E-04
3.4E-05
3.0E-05
1.9E-05
1.0E-04
6.7E-05
6.1E-05
5.6E-05
6.1E-05
5.6E-05
3.6E-05
1.9E-05
1.2E-04
1.2E-04
1.3E-04
2.0E-05
3.0E-05
3.8E-05
2
2
2
2
2
2
3
2
4
3
2
3
2
3
4
2
3
2
4
3
2
3
2
2
2
2
4
3
2
2
2
2
3
2
2
4
2
2
4
2
3
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
1
1
71
577.01
578.01
579.01
580.01
581.01
582.01
583.01
584.01
584.02
585.01
586.01
587.01
588.01
589.01
590.01
590.02
592.01
593.01
596.01
597.01
597.02
598.01
599.01
600.01
601.01
602.01
605.01
607.01
609.01
610.01
611.01
612.01
612.02
614.01
617.01
618.01
620.01
622.01
623.01
623.02
623.03
5.2888
5.1938
1.8672
2.7903
2.6717
2.5505
3.1312
3.7109
4.4730
1.9189
3.7971
3.4973
2.6497
4.2971
3.7243
5.8287
4.7864
3.2745
1.3419
4.8348
2.6017
2.9641
2.4207
2.5733
2.5206
5.2372
1.7663
1.5864
1.8343
2.5145
1.4497
3.3581
5.3336
1.8723
2.9128
2.6232
5.8762
8.9133
4.2819
5.5070
3.7922
500
1173
319
743
1206
844
246
720
553
818
571
816
595
189
412
615
478
524
689
510
184
767
581
388
825
445
980
6629
4272
886
4347
540
799
3854
7003
1028
6402
4669
106
103
74
9
90
31
32
49
34
28
47
27
37
23
38
19
8.6
22
20
19
16
42
17
14
34
29
26
19
19
54
74
56
26
319
26
28
122
158
38
53
58
23
21
21
111.55
102.8794
103.0698
108.7093
108.9144
103.4687
103.7392
108.6885
103.3728
104.558
108.9754
104.6019
108.6871
119.5356
107.5461
74.3251
108.4815
104.7889
103.4508
109.9401
66.0722
104.1666
106.2091
103.3635
105.1847
110.2739
102.7178
106.48563
105.028
113.8431
104.05987
106.2164
149.5591
103.02216
131.59768
111.3474
92.1077
146.4969
107.0644
112.4629
104.4771
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0.0015
0.0021
0.0025
0.0016
0.002
0.0033
0.0021
0.0044
0.0017
0.0041
0.0028
0.0041
0.0092
0.0045
0.0073
0.0061
0.0051
0.0012
0.0056
0.0064
0.0027
0.0027
0.0032
0.0038
0.0063
0.0011
0.00036
0.0011
0.0026
0.00018
0.0031
0.0046
0.00059
0.00057
0.0022
0.0026
0.0031
0.0043
0.0054
0.0049
39.6729
6.412547
2.020003
6.52125
6.996895
5.945053
2.436893
9.9265
21.22343
3.722176
15.77916
14.03513
10.35547
17.4808
11.38933
50.6962
39.7521
9.99757
1.682706
17.30819
2.092181
8.30811
6.45469
3.59594
5.40425
12.91408
2.628144
5.894028
4.396913
14.28246
3.2516578
20.74022
47.4276
12.874706
37.86537
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45.15416
155.0467
10.3496
15.67781
5.5992
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0.000063
0.000028
0.00011
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0.000083
0.000055
0.00015
0.00069
0.000042
0.00044
0.00026
0.0003
0.00085
0.00035
0.0017
0.0018
0.00034
0.000014
0.00069
0.000057
0.00016
0.00012
0.00011
0.00014
0.00054
0.00002
0.000052
0.000034
0.00026
0.0000041
0.00046
0.0019
0.00005
0.00017
0.00014
0.00078
0.0044
0.00032
0.00065
0.00018
59
9.811
9.093
18
20.47
17
4
21.68
37
15.33
22
25
23
21
17
68.1
35
18
10.097
27.63
6.2
21.48
17
10.27
17.1
19.55
11.29
39.45
9.4
45.2
10.3
32
72.4
39
52
19
63.25
81
9
22.78
6
477
0.082
0.05
95
0.39
74
12
0.46
1.1
0.43
72
63
100
180
72
2.4
85
124
0.022
0.97
1.9
0.56
93
0.33
1.6
0.77
0.26
0.91
2.8
1.8
3.1
102
2.1
12
16
54
0.93
12
31
0.74
19
0.02
0.03075
0.01747
0.025
0.03159
0.027
0.0164
0.02287
0.02177
0.02686
0.024
0.028
0.023
0.014
0.021
0.02208
0.0229
0.023
0.02575
0.02229
0.01204
0.02527
0.023
0.01839
0.0182
0.01904
0.02757
0.07544
0.089
0.02681
0.07259
0.024
0.02517
0.06268
0.177
0.031
0.07225
0.0732
0.0112
0.00954
0.0099
0.034
0.00023
0.00038
0.025
0.00048
0.024
0.0083
0.0004
0.00053
0.00053
0.014
0.014
0.023
0.02
0.015
0.00071
0.0088
0.028
0.00042
0.00072
0.00079
0.00052
0.022
0.00049
0.0015
0.00068
0.00044
0.00093
0.011
0.00084
0.00037
0.015
0.00061
0.0006
0.021
0.017
0.00091
0.0025
0.0055
0.00026
0.0048
0.1
0.004
0.0295
0
0.001
0.4
0.7
0.0173
0.025
0.0528
0.7
0.6
0.7
0.8
0.7
0.031
0.85
0.7
0.0338
0.014
0.0223
0.6
0.0478
0.11
0.002
0.023
0.031
0.92
0.022
0.79
0.8
0.004
0.58
1.11
0.7
0.016
0.85
0.9
0.032
0.9
3.4
2.7
2.3
1.4
0.01
1.4
1.5
1.9
2.2
1.7
0.063
0.98
2.4
0.01
2.2
0.01
0.01
0.033
0.032
0.28
0.044
0.24
1.3
0.01
0.17
0.33
1.4
0.022
0.24
1
0.078
1
2.6
3.8
1.5
1.5
2.1
2.2
1.6
1.6
1.5
2.0
2.1
3.0
2.2
1.2
2.1
2.2
2.7
2.1
1.7
2.6
1.4
1.7
2.3
2.1
1.7
2.3
1.6
6.8
12.0
2.0
7.3
3.5
3.6
4.0
17.8
3.2
7.2
9.3
2.0
1.7
1.8
0.227
0.069
0.03
0.067
0.07
0.062
0.036
0.088
0.146
0.046
0.124
0.113
0.085
0.134
0.102
0.276
0.234
0.092
0.022
0.135
0.033
0.077
0.069
0.047
0.062
0.111
0.031
0.064
0.054
0.096
0.044
0.15
0.26
0.107
0.224
0.086
0.253
0.568
0.099
0.13
0.066
502
1035
1154
716
714
783
1266
633
492
932
630
672
619
637
809
492
550
760
864
724
1464
644
935
1213
974
831
782
871
1200
481
1235
668
507
587
499
790
486
327
1121
978
1373
3.5E-05
4.1E-05
4.1E-05
3.9E-05
4.2E-05
3.7E-05
2.8E-05
2.2E-05
2.3E-05
3.8E-05
1.7E-05
5.7E-05
1.4E-05
3.2E-05
7.0E-05
4.4E-05
5.2E-05
1.6E-05
3.4E-05
2.6E-05
6.6E-05
2.2E-05
2.8E-05
3.2E-05
4.8E-05
2.1E-05
2.6E-05
6.6E-05
2.4E-05
2.2E-05
5.8E-05
2.6E-05
2.5E-05
2.9E-05
3.0E-05
3.1E-05
3
2
2
2
2
3
3
2
2
2
3
2
2
3
2
4
3
2
2
2
4
2
3
3
2
3
2
3
3
2
2
2
2
3
3
2
2
3
3
3
3
NoObs
1
1
NoObs
NoObs
NoObs
1
NoObs
NoObs
NoObs
1
1
1
72
624.01 4.4288
625.01 4.4579
626.01 3.9008
627.01 3.5631
628.01 3.0462
629.01 6.7051
632.01 3.1532
633.01 10.3584
635.01 3.4572
638.01 5.2480
638.02 7.1418
639.01 5.6758
640.01 3.1182
641.01 3.3757
644.01 7.3023
645.01 2.8982
645.02 7.6570
647.01 4.6876
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650.01 2.3266
652.01 2.9306
654.01 2.9044
655.01 5.6200
657.01 2.0229
657.02 2.8468
658.01 1.9455
658.02 2.0263
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660.01 6.7029
661.01 3.4869
662.01 5.5389
663.01 1.8327
663.02 2.8399
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665.01 4.0178
665.02 3.1579
665.03 3.7875
666.01 3.9017
667.01 2.7220
670.01 3.2407
671.01 3.2752
921
1257
343
400
413
383
267
713
602
1147
1245
422
679
1172
24143
184
209
187
245
865
3206
328
399
532
799
499
477
291
243
349
226
527
644
202
423
89
75
615
10130
252
152
23
58
29
38
22
18
21
31
20
64
47
33
39
37
903
17
21
33
29
58
87
20
44
35
34
46
35
20
37
20
30
64
39
22
59
21
14
44
124
20
21
115.4407
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105.2217
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0.00015
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0.00041
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0.0023
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0.00022
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0.0005
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0.00025
32
0.000048 54.776631
0.00029
13
0.0013
21
0.00012
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0.00088
22.24
0.00011
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0.0001
44
0.00022
13
0.00061
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0.000049
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0.00025
45
0.000033
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0.000079
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0.0008
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0.00016
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0.00042
27
0.00033
13
0.000017
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0.00029
57
0.00052
15
0.000072
11.55
0.000033
1.9
0.0001
6.2
0.00039
45
0.000024
13.95
0.00028
14
0.00012
6
1.1
7
68
30
89
142
0.71
31
163
6.3
1.2
0.56
225
70
0.000058
64
71
12
0.46
40
87
51
0.57
0.51
1.4
0.46
60
144
0.12
143
53
11
1.5
44
0.16
7.9
0 .4
183
0.13
57
22
0.02703
0.0623
0.0186
0.0197
0.022
0.019
0.01483
0.0283
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0.022
0.016
0.01413
0.018
0.0127
0.0245
0.02282
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0.00024
0.017
0.0094
0.0065
0.00043
0.0077
0.00022
0.0068
0.00043
0.017
0.00064
0.011
0.0085
0.031
1
0.7
0.7
0.9
0.7
0.028
0.86
0.7
0.84
0.017
0.026
0.6
0.5
0.0008
0.8
0.5
0.8
0.01
0.83
0.1
0.8
0.0157
0.014
0
0.04
0.7
0.7
0.0093
0.5
0
0.84
0.031
0.7
0.0003
0.9
0.008
0.1
0.024
0.8
0.8
0.066
0.3
1.5
1.3
1.3
1.8
0.055
0.42
2
0.36
0.022
0.035
1.8
1.6
1.5
1.9
1.1
0.02
0.83
1.7
1.3
0.036
0.01
1.7
1.9
2.3
2.4
0.81
0.049
1.4
1.1
0.01
2.4
0.022
1.5
1.3
2.1
15.1
2.2
2.9
3.1
3.0
1.2
5.4
2.7
4.8
4.1
2.1
2.9
3.2
35.3
2.6
2.5
1.8
2.0
3.8
3.0
2.9
2.1
1.6
1.9
1.5
2.2
2.5
2.2
2.1
1.5
1.9
1.7
2.1
2.3
1.2
0.8
2.0
6.5
2.1
1.4
0.133
0.241
0.121
0.08
0.12
0.244
0.072
0.614
0.132
0.166
0.333
0.139
0.193
0.104
0.271
0.086
0.171
0.061
0.167
0.101
0.112
0.085
0.177
0.046
0.115
0.043
0.061
0.168
0.067
0.119
0.095
0.033
0.124
0.113
0.066
0.028
0.043
0.156
0.044
0.09
0.051
565
828
817
1066
826
669
761
428
762
682
482
747
533
535
698
1124
797
1168
727
728
459
1013
674
798
504
1162
975
818
1077
776
875
846
436
863
1066
1636
1320
570
711
883
1126
2.0E-05
1.1E-04
7.1E-05
4.3E-05
7.8E-05
4.6E-05
9.5E-05
8.4E-05
8.0E-05
1.7E-04
1.2E-04
1.2E-04
2.1E-06
1.3E-04
1.3E-04
5.3E-05
4.8E-05
3.2E-05
3.2E-05
2.7E-05
5.0E-05
2.5E-05
2.3E-05
1.7E-04
1.7E-04
5.4E-05
2.9E-05
2.7E-05
5.8E-05
2.3E-05
2.1E-05
6.1E-05
4.0E-05
7.2E-05
7.1E-06
6.2E-05
7.2E-05
2
2
2
2
2
2
2
2
2
2
4
2
2
3
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
3
2
4
4
2
3
3
2
1
NoObs
1
NoObs
NoObs
NoObs
1
NoObs
1
1
NoObs
NoObs
1
NoObs
1
1
1
1
NoObs
1
NoObs
NoObs
NoObs
NoObs
NoObs
1
NoObs
1
1
1
NoObs
1
1
NoObs
NoObs
73
672.01
672.02
673.01
674.01
676.01
676.02
678.01
679.01
680.01
682.01
683.01
684.01
685.01
686.01
687.01
688.01
689.01
691.01
691.02
692.01
693.01
693.02
694.01
695.01
697.01
698.01
700.01
700.02
701.01
701.02
701.03
703.01
704.01
707.01
707.02
707.03
707.04
708.01
708.02
709.01
710.01
3.0784
5.8817
3.0279
9.4755
2.8769
1.7470
2.7421
8.1270
8.9336
9.9203
4.4673
1.8215
3.4760
3.0231
2.1209
2.9239
3.5876
8.3024
6.1582
1.8674
7.3509
7.0385
4.8698
4.9238
3.6358
2.4663
2.9694
3.2972
2.9877
2.3257
6.8714
1.6971
2.5400
7.8208
9.8121
8.5541
6.4886
6.7713
4.9436
3.7885
3.9341
554
966
247
1610
3080
1693
113
307
4384
4927
2328
794
286
14530
285
270
582
614
108
173
311
321
827
566
480
7776
564
211
919
411
697
135
498
677
396
373
246
525
269
615
140
32
50
20
97
53
41
21
33
586
163
55
50
41
620
13
31
21
47
9.7
20
27
36
56
45
45
386
28
19
48
34
25
24
14
48
23
22
21
42
26
31
21
105.8116
86.8426
103.7904
110.9192
104.5826
103.8934
105.59
123.2486
110.64238
118.99358
110.5186
105.2568
103.9261
104.67404
104.983
103.2535
115.398
122.3661
77.039
104.8412
126.3107
79.3547
117.2445
108.293
104.7324
105.99432
105.9348
104.9588
113.8108
103.9187
83.398
102.9528
118.13
122.631
105.5817
68.8687
76.6803
104.0034
109.5127
111.791
103.9326
0.0028
0.0037
0.0041
0.0022
0.0014
0.0014
0.013
0.0051
0.00045
0.00099
0.0021
0.0012
0.0024
0.00014
0.0059
0.0027
0.0047
0.0038
0.015
0.0028
0.0058
0.0051
0.0023
0.0027
0.0021
0.00028
0.0031
0.0044
0.0017
0.0023
0.0045
0.0025
0.0051
0.0036
0.0091
0.0091
0.0079
0.0035
0.0047
0.0029
0.0044
16.08822
41.749
4.41748
16.33886
7.972513
2.453224
6.04097
31.8049
8.600116
163.7133
278.1232
4.034923
3.173885
52.513492
4.17853
3.275814
15.87403
29.66717
16.2245
2.462367
28.7784
15.66002
17.42154
29.90653
3.032186
12.718733
30.86436
9.36127
18.16428
5.714973
122.3894
1.3686
18.39714
21.77654
41.0315
31.7845
13.17535
17.40696
7.69315
21.38418
5.37503
0.00033
0.0012
0.00013
0.00021
0.000076
0.000023
0.00054
0.0012
0.000027
0.0083
0.003
0.000033
0.000053
0.000039
0.00017
0.00006
0.00046
0.00092
0.001
0.000047
0.0013
0.00032
0.00028
0.00063
0.00004
0.000023
0.00069
0.00028
0.00025
0.000087
0.0017
0.000024
0.00067
0.00055
0.0025
0.0012
0.00045
0.00044
0.00025
0.00044
0.00016
25
58.85
11.98
11.3
12
9.5
10.2
30.4
7.817
156.9
385
6
4.7
147.001
11.6
5
34.3
27.7
20.8
10.33
24
18.23
27.97
32
5
23
45
13
35
14
138.6
3
60.8
21.9
32.14
29.17
11
20.02
10
43
10.67
67
0.87
0.55
5.8
3.6
2.8
3.1
9.1
0.011
1.4
340
1.8
9.9
0.00011
3.5
16
1.3
0.36
1.3
0.41
74
0.23
0.39
51
10
6.9
113
45
74
41
4
15
5.1
0.29
0.77
0.77
38
0.3
33
202
0.16
0.025
0.02823
0.01412
0.0378
0.0593
0.03888
0.011
0.01568
0.05966
0.04688
0.0489
0.0407
0.0175
0.1077
0.0164
0.0175
0.02165
0.02253
0.01006
0.01309
0.0169
0.01624
0.02593
0.0241
0.0215
0.1209
0.025
0.0159
0.03
0.021
0.02341
0.013
0.0167
0.02384
0.01873
0.01761
0.0156
0.02136
0.0167
0.023
0.0113
0.011
0.00037
0.00056
0.0042
0.0034
0.00086
0.0026
0.00039
0.00008
0.0004
0.0078
0.0042
0.006
0.0032
0.0013
0.0083
0.00074
0.0003
0.00059
0.00042
0.0088
0.00029
0.00028
0.0065
0.008
0.0025
0.01
0.0091
0.013
0.013
0.00059
0.0093
0.0014
0.0003
0.00047
0.00047
0.009
0.0003
0.0098
0.021
0.00031
0.8
0.016
0.0305
0.59
0.84
0.308
0.66
0.0002
0.002
0.8
0.96
0.8
0.0028
0.44
0.8
0.021
0.018
0.056
0.0614
0.6
0.022
0.031
0.76
0.7
0.92
0.86
0.8
0.7
0.7
0.015
0.9
0.015
0.0044
0.041
0.029
0.7
0.027
0.6
0.3
0.0171
1.1
0.022
0.69
0.35
0.092
0.2
0.032
0.67
0.29
1.1
0.13
1.2
0.01
0.01
0.014
1.7
0.01
0.055
0.98
1.3
0.28
0.97
1.2
1.2
1.5
0.046
1.3
0.01
0.01
0.04
1.6
0.028
1.7
2.5
-
4.0
4.5
1.8
11.3
4.5
2.9
1.7
1.8
7.6
4.9
4.2
8.3
2.8
11.3
1.7
2.5
2.0
2.9
1.3
0.8
1.8
1.7
1.7
3.1
4.0
12.0
3.1
1.9
2.2
1.5
1.7
1.7
1.7
3.4
2.6
2.5
2.2
2.2
1.7
2.2
1.7
0.13
0.245
0.055
0.137
0.067
0.03
0.066
0.197
0.085
0.591
0.839
0.052
0.045
0.275
0.052
0.045
0.123
0.195
0.13
0.035
0.19
0.126
0.13
0.195
0.043
0.103
0.197
0.089
0.127
0.059
0.454
0.025
0.136
0.159
0.242
0.204
0.113
0.135
0.078
0.152
0.067
821
598
1303
959
598
894
1028
598
989
307
239
1414
1570
442
1060
1465
622
653
799
1004
611
750
530
643
1601
748
588
875
496
728
262
1866
619
745
604
658
884
703
924
588
1320
5.1E-05
4.7E-05
5.6E-05
2.4E-05
3.4E-05
3.9E-05
3.3E-05
2.8E-05
5.1E-05
3.8E-05
1.3E-05
8.9E-05
2.7E-06
4.1E-05
6.5E-05
2.0E-05
4.2E-05
2.3E-05
1.9E-05
1.7E-05
3.3E-05
1.2E-05
3.5E-05
4.6E-05
1.7E-05
2.0E-05
5.1E-05
1.6E-05
2.1E-05
2.5E-05
4.4E-05
5.2E-05
2.1E-05
5.1E-05
2
2
2
3
2
2
3
2
2
2
2
2
2
3
3
2
2
2
4
2
2
4
2
2
2
2
2
2
2
2
4
2
2
2
2
4
4
2
2
2
2
1
1
1
NoObs
NoObs
1
1
NoObs
NoObs
1
NoObs
NoObs
1
NoObs
NoObs
NoObs
1
1
1
1
NoObs
NoObs
1
1
1
1
NoObs
1
74
711.01 6.1018
711.02 3.1710
711.03 9.8334
712.01 1.9895
714.01 2.2176
716.01 2.2744
717.01 3.1618
718.01 3.2541
718.02 5.7207
718.03 5.5414
719.01 1.6354
720.01 2.4833
721.01 6.8323
722.01 6.9235
723.01 1.8098
723.02 4.3932
723.03 1.4752
725.01 3.3669
728.01 2.0043
730.01 5.7701
730.02 5.4941
730.03 4.3590
730.04 5.2290
732.01 1.7619
733.01 2.6528
733.02 2.9996
733.03 2.1611
734.01 7.1431
735.01 4.7686
736.01 3.0657
736.02 3.1139
737.01 3.1240
738.01 3.1466
738.02 3.3240
739.01 1.4949
740.01 3.1145
741.01 3.9182
743.01 10.5338
745.01 9.3456
746.01 3.3082
747.01 1.5804
786
184
685
132
862
2182
285
367
499
332
538
1235
206
468
1328
1302
1541
8800
7786
746
393
343
259
1149
1540
1152
460
1075
2970
1422
607
3249
1219
933
779
864
37406
9931
10890
1296
1906
34
22
25
17
89
103
22
42
33
16
41
27
25
35
24
13
15
31
211
20
13
9.7
9.1
72
41
23
16
34
28
19
14
73
34
23
42
18
874
189
98
46
37
107.8257
68.4376
187.1803
104.23
105.78778
112.95307
108.7924
102.8579
80.2934
74.9787
104.013
107.0488
113.6486
125.9894
102.6479
127.916
106.0831
102.6447
103.11774
109.796
71.36
68.131
70.475
103.4084
102.7156
67.3199
68.6747
120.9151
104.5711
110.7903
68.2816
115.6786
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119.3644
102.83287
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113.8723
106.2476
104.6042
0.0048
0.0044
0.0076
0.0031
0.00081
0.0008
0.0038
0.0021
0.0041
0.0082
0.0015
0.0026
0.0064
0.0038
0.0026
0.0049
0.0034
0.0023
0.00035
0.0062
0.011
0.011
0.014
0.00081
0.002
0.0042
0.0047
0.0043
0.0051
0.0042
0.0074
0.0014
0.0028
0.0041
0.0013
0.0045
0.00017
0.0014
0.0031
0.0021
0.0016
44.6987
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2.178191
4.182017
26.89291
14.70752
4.585494
22.71449
47.9042
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13.72423
46.408
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7.38469
1.2602586
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11.34917
3.132968
24.54369
22.34101
18.79523
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14.49847
10.33677
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17.67221
23.355367
19.40335
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0.000048
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0.0019
0.000093
0.0001
0.0006
0.0013
0.000069
0.00043
0.00025
0.00011
0.000018
0.00099
0.00047
0.00051
0.00047
0.000007
0.000081
0.0002
0.000064
0.0008
0.00073
0.0006
0.00021
0.00015
0.0002
0.0004
0.000012
0.00061
0.000028
0.00021
0.00034
0.00013
0.000065
56.3
4
87
9.893
14.8
40
37.7
9
31.07
55
32
17
15.7
51.86
17.4
50.5
66.1
18
17.5
17
13.71
12
11.25
5.834
17.95
30
9
26.84
37.4
43
20.4
18
22
32
7.23
25
33.6
15.3162
14.67
16
24
1.2
23
382
0.073
0.18
12
1.5
21
0.65
327
111
102
0.39
0.95
0.84
2.5
7.2
5.4
5.2
77
0.67
103
0.44
0.018
0.43
1.2
51
0.52
1.1
244
1.1
2.5
83
248
0.2
94
3
0.0011
0.12
29
82
0.02508
0.012
0.024
0.01118
0.02607
0.0606
0.01569
0.0186
0.02078
0.017
0.024
0.032
0.01352
0.01951
0.034
0.0349
0.0384
0.0833
0.09887
0.026
0.01915
0.021
0.01532
0.0318
0.03568
0.0307
0.024
0.02948
0.0483
0.036
0.0264
0.0638
0.033
0.029
0.02741
0.03
0.2416
0.087
0.0917
0.036
0.043
0.00047
0.011
0.021
0.00044
0.00024
0.0027
0.0005
0.0082
0.00038
0.018
0.014
0.04
0.00032
0.00036
0.0011
0.0015
0.0031
0.0024
0.00097
0.021
0.00083
0.033
0.00098
0.00031
0.00066
0.001
0.027
0.00055
0.0011
0.038
0.0011
0.002
0.024
0.042
0.00051
0.023
0.0062
0.021
0.00065
0.014
0.032
0.004
0.9
0.5
0.0809
0.0001
0.93
0.044
0.6
0.031
0.6
0.8
0.4
0.029
0.001
0.0378
0.025
0.015
0.8
0.5
0.04
0.7
0.049
0.0447
0.0002
0.025
0.6
0.012
0.032
0.5
0.064
0.89
0.6
0.3
0.0416
0.8
0.89
0.006
0.0082
0.7
0.7
0.025
1.3
2.2
0.28
0.01
1.5
0.054
2.2
1.4
2.7
0.044
0.025
0.049
0.24
2.1
0.01
2.4
0.01
0.01
2.2
0.01
0.1
2.5
0.01
0.2
1.9
3.1
1.4
0.15
0.01
1.1
1.6
2.7
1.3
2.6
0.8
2.2
6.3
0.9
1.6
1.8
1.5
1.9
3.0
2.3
1.8
2.8
2.9
3.2
6.8
9.9
3.1
2.3
2.5
1.8
2.9
2.2
1.9
1.5
2.4
5.0
2.6
2.0
5.6
3.3
2.9
2.0
2.3
18.7
10.9
9.7
3.1
2.8
0.249
0.047
0.494
0.033
0.051
0.18
0.114
0.055
0.159
0.261
0.075
0.061
0.118
0.259
0.048
0.177
0.09
0.071
0.075
0.12
0.092
0.092
0.076
0.023
0.061
0.094
0.04
0.166
0.153
0.117
0.059
0.114
0.095
0.112
0.019
0.123
0.159
0.139
0.124
0.08
0.056
486
1118
345
1101
929
595
510
964
567
443
605
849
942
485
918
478
670
720
922
746
852
852
937
1424
683
551
844
535
557
442
623
597
781
719
1058
497
518
617
613
648
633
4.6E-05
1.8E-05
3.0E-05
1.5E-05
2.4E-05
2.0E-05
4.3E-05
6.5E-05
6.0E-05
2.3E-05
2.3E-05
2.1E-05
7.0E-05
2.6E-05
3.0E-05
3.1E-05
5.4E-05
3.1E-05
3.9E-05
6.0E-05
6.5E-05
1.9E-05
3.0E-05
1.6E-05
4.2E-05
2.5E-05
1.5E-05
2
4
4
3
2
2
3
2
4
4
2
2
3
2
2
2
2
2
3
2
4
4
4
2
2
4
4
2
2
2
4
2
2
2
2
3
3
2
2
2
2
NoObs
1
NoObs
1
1
1
NoObs
NoObs
1
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
1
75
749.01 3.0377
749.02 2.3564
750.01 3.3702
751.01 2.0883
752.01 3.0592
752.02 4.1260
753.01 1.8813
755.01 1.6211
756.01 4.6503
756.02 3.0514
756.03 2.4819
757.01 3.5566
757.02 4.6490
757.03 2.4488
758.01 3.4108
759.01 4.8992
760.01 2.0728
762.01 3.7651
763.01 4.9957
764.01 10.3560
765.01 2.2835
766.01 3.1048
767.01 2.6063
769.01 2.8675
771.01 48.1018
772.01 5.5841
773.01 5.5792
774.01 2.8950
775.01 2.8272
775.02 2.4216
776.01 2.6154
777.01 2.9867
778.01 1.1499
779.01 6.4631
780.01 1.9891
781.01 2.5888
782.01 4.3279
783.01 7.3311
784.01 2.9416
785.01 3.3041
786.01 2.3232
848
375
985
995
593
885
7451
660
1502
691
231
5214
2395
840
1282
1713
9959
483
12565
2681
990
1447
17466
688
19287
4359
692
26414
955
1320
5364
6883
811
14710
940
3141
2926
3022
1246
937
472
33
15
21
20
19
14
48
25
39
25
9.4
99
35
22
22
40
425
18
307
71
24
63
915
31
236
30
20
359
13
22
212
29
27
377
41
44
107
176
20
19
19
104.8065
69.0904
104.5295
104.74
103.5366
95.5164
108.8504
104.5925
104.2018
105.9703
112.5496
106.622
98.035
104.3013
109.354
127.1363
105.25698
104.3455
112.40123
141.9341
104.6302
102.7521
103.96676
104.8993
142.0388
106.8349
105.817
102.9705
105.724
109.3746
104.79264
106.5648
103.6798
110.19884
104.7599
113.3936
106.63389
102.9929
119.7842
111.7494
103.36
0.0028
0.0052
0.0049
0.0045
0.0044
0.0081
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0.0029
0.004
0.0047
0.0086
0.001
0.0038
0.0044
0.0041
0.0031
0.00017
0.0055
0.00055
0.0031
0.003
0.0016
0.00009
0.0027
0.0035
0.0042
0.005
0.00031
0.0047
0.0023
0.00039
0.0031
0.0017
0.0006
0.0016
0.0018
0.00093
0.001
0.0044
0.0046
0.0035
5.349518
3.940973
21.67821
4.99682
9.48851
54.4154
19.89939
2.525605
11.09431
4.13463
2.5667
16.0686
41.19249
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16.016
32.6272
4.9593304
4.4987
19.65119
41.43958
8.35404
4.125488
2.8165077
4.280889
10389
61.2592
38.37813
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16.38523
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3.7287253
40.41887
2.24334
10.405935
2.337466
11.59823
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19.2693
12.39325
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0.000099
0.000088
0.00074
0.00014
0.0003
0.0022
0.00019
0.000046
0.00028
0.00013
0.00011
0.00017
0.00069
0.00025
0.00074
0.001
0.0000059
0.00016
0.00012
0.00098
0.00023
0.000042
0.0000018
0.000079
133
0.0032
0.00087
0.000016
0.0007
0.00018
0.0000099
0.00089
0.000036
0.000066
0.000026
0.00015
0.000045
0.000053
0.00059
0.00037
0.000087
14.486
12.83
30
13
22
84
49
12.53
18.85
10.55
8.67
37.1
72
14
39.8
55
12.01
9.19
24.49
31.83
20
10.66653
7.05
11.636
1855
53
51.4
27.75
44.3
26.4
11.606493
52
17.99
13.752186
9.901
39
12.201573
7.987
47
29.4
13.82
0.099
0.7
57
61
130
693
15
0.55
0.37
0.36
0.63
0.37
2.1
58
2
1.1
0.35
0.46
0.94
0.27
106
0.00011
0.18
0.1
24
17
1.9
0.11
3.2
1.2
0.000031
16
0.98
0.000088
0.046
113
0.000083
0.034
256
1.4
0.62
0.02772
0.01895
0.034
0.034
0.023
0.029
0.1015
0.02434
0.03516
0.02509
0.017
0.06336
0.0431
0.03
0.03
0.03774
0.10675
0.01832
0.10979
0.04707
0.03
0.035
0.12849
0.02389
0.12445
0.0695
0.02311
0.14349
0.0285
0.0332
0.065
0.3477
0.0279
0.109
0.02856
0.05
0.048
0.04895
0.032
0.027
0.02241
0.00052
0.00081
0.013
0.031
0.026
0.048
0.0072
0.00072
0.00059
0.0007
0.0011
0.0005
0.0011
0.026
0.0011
0.00064
0.00076
0.0008
0.0009
0.0004
0.03
0.073
0.00076
0.0005
0.0044
0.00078
0.00043
0.0016
0.0012
0.023
0.0036
0.001
0.021
0.00048
0.029
0.093
0.00019
0.033
0.0011
0.00076
0.0612
0.0316
0.85
0.7
0.4
0.7
0.84
0.0327
0.027
0.0209
0.2236
0.0188
0.013
0.7
0.003
0.0003
0.85
0.027
0.71
0.003
0.7
0.0065
0.68
0.019
0.84
0.015
0.0002
0.043
0.027
0.0007
1.56
0.01
0.0496
0.2
0.0001
0.029
0.5
0.042
0.0624
0.86
1.7
2.6
2.6
0.25
0.033
0.022
1.7
0.01
0.11
0.01
0.16
0.02
1.9
0.14
0.36
0.01
0.01
0.052
0.47
0.042
2
0.017
2.5
0.01
-
2.0
1.4
2.6
3.2
2.7
3.4
6.9
2.8
3.7
2.6
1.8
4.8
3.3
2.3
3.8
3.6
9.7
1.7
13.2
5.6
2.4
3.8
14.2
2.0
15.0
8.2
2.1
15.8
2.1
2.5
4.3
36.0
1.9
12.8
2.2
4.3
5.6
3.5
2.3
2.1
1.8
0.059
0.048
0.139
0.056
0.089
0.286
0.143
0.037
0.099
0.052
0.037
0.119
0.223
0.063
0.123
0.2
0.058
0.054
0.147
0.236
0.079
0.052
0.039
0.051
9.514
0.313
0.225
0.077
0.105
0.065
0.046
0.23
0.027
0.095
0.032
0.083
0.07
0.072
0.117
0.103
0.047
789
875
458
896
853
476
519
1350
791
1092
1294
530
387
729
663
495
982
1013
700
500
713
1144
1221
946
84
482
477
939
458
582
852
471
857
821
995
521
989
707
429
620
980
3.3E-05
3.2E-05
7.0E-05
3.4E-05
2.9E-05
6.5E-05
7.9E-05
1.4E-05
1.7E-05
2.2E-05
5.9E-05
1.5E-05
1.6E-05
7.8E-05
1.7E-05
3.1E-05
1.9E-05
3.0E-05
1.6E-05
4.3E-05
1.2E-05
3.2E-05
1.8E-05
1.6E-05
2.0E-05
1.2E-05
1.8E-05
1.6E-05
3.8E-05
3.0E-05
2.3E-05
2.7E-05
3.3E-05
4.0E-05
3.5E-05
2
4
2
2
2
4
3
2
2
2
4
2
2
2
2
2
2
3
2
2
2
2
2
2
2
2
3
3
2
2
2
3
2
2
2
2
2
2
2
2
3
NoObs
NoObs
NoObs
NoObs
1
NoObs
NoObs
NoObs
NoObs
76
787.01
787.02
788.01
790.01
791.01
794.01
795.01
797.01
799.01
800.01
800.02
801.01
802.01
804.01
805.01
806.01
806.02
806.03
809.01
810.01
811.01
812.01
812.02
812.03
813.01
814.01
815.01
816.01
817.01
818.01
821.01
822.01
823.01
824.01
825.01
826.01
827.01
829.01
829.02
829.03
830.01
3.1631
2.1124
3.3280
2.6555
4.9811
2.4001
1.8917
2.9281
1.6033
3.0081
3.9728
2.4077
2.2149
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7.8222
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4.7450
2.2740
5.1665
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3.4728
3.1504
2.4193
4.3866
3.0811
1.4379
3.7671
3.2182
2.9092
2.5968
4.2648
4.1408
4.5589
2.6064
1031
39
435
12
1708
29
991
23
6273 181
401
22
1430
31
6082 111
1525
70
961
38
924
26
8385 533
22158 264
987
29
18439 430
10175
57
19862 195
1115
14
16511 602
1024
41
2267
48
1757
43
1491
21
1471
14
8958 258
941
19
4926
62
2412
70
1242
12
1618
33
1235
21
16197 257
5445
58
19284
80
846
21
765
40
860
30
893
27
403
17
976
22
23232 1241
104.0208
66.8549
109.0511
107.1626
113.89115
102.6744
103.5759
110.1418
102.81727
103.0385
105.8128
103.82617
114.88094
110.2
107.58168
87.2386
176.89513
83.6924
103.64747
103.51
114.4316
104.9773
80.4576
98.2376
103.52731
108.4529
105.6313
107.9981
119.2141
109.3409
107.0084
105.18019
103.22827
106.6086
109.9535
104.134
107.7764
107.7772
71.7806
96.8416
103.04717
0.0025
0.0064
0.0032
0.0039
0.00077
0.0036
0.0022
0.0011
0.00087
0.0023
0.0044
0.00016
0.00028
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0.00069
0.0035
0.00088
0.0086
0.00018
0.0018
0.0021
0.0015
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0.01
0.0003
0.005
0.0017
0.0018
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0.0023
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0.00031
0.00086
0.0014
0.004
0.0022
0.0028
0.0041
0.0073
0.0056
0.00007
4.431061
5.68952
26.3953
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12.611939
2.539147
6.77034
10.18151
1.6266615
2.711437
7.21227
1.6255204
19.620402
9.02971
10.327948
143.1814
60.32875
29.1654
1.5947453
4.782942
20.50617
3.34024
20.06086
46.1851
3.8959257
22.367
34.8442
7.748017
23.9716
8.11429
21.8131
7.919371
1.0284369
15.3755
8.10341
6.365997
5.97569
18.64902
9.75222
38.5596
3.5256346
0.000075
11.1
0.00015
21.8
0.00057
47
0.00023
25.1
0.000069 20.757
0.000061
8.98
0.0001
29.7
0.000069
21.8
0.0000097
5.6
0.000043
7.37
0.00022
14
0.0000017 5.639292
0.00004
83
0.00022
16
0.000074 11.377346
0.0027
133
0.00037
78.27
0.0012
47.3
0.0000027 7.145002
0.000062
14
0.00032
39.8
0.000035
13
0.00047
50.3
0.0019
75.7
0.0000082
14.23
0.00045
33
0.00043
47
0.000094
17.74
0.0011
64.4
0.00013
21
0.0015
34
0.000017
15.49
0.0000061
4.2
0.00048
39.69
0.00023
16
0.000094
17.35
0.00012
12
0.00053 34.8801
0.00032
14
0.001
67.1
0.0000018 11.745
0.27
1.5
158
1.1
0.099
0.35
1.2
6.5
1.7
0.17
99
0.000006
15
56
0.000082
47
0.44
7
0.000012
45
0.74
50
2.2
4.2
0.067
173
14
0.23
4.6
59
171
0.73
1.3
0.58
66
0.39
40
0.0027
76
2.6
0.012
0.02873
0.0219
0.04
0.02876
0.07053
0.02019
0.03458
0.07652
0.03934
0.02941
0.027
0.081
0.1345
0.031
0.1195
0.0933
0.12509
0.032
0.114
0.03
0.04186
0.039
0.0352
0.0341
0.08461
0.028
0.101
0.04406
0.033
0.04
0.034
0.1279
0.0753
0.1221
0.028
0.02535
0.03
0.03
0.02
0.02809
0.13434
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0.0012
0.028
0.00094
0.00028
0.00063
0.00099
0.00073
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0.013
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0.021
0.0095
0.0073
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0.08
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0.028
0.0011
0.0017
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0.00045
0.002
0.021
0.033
0.0015
0.0015
0.0013
0.026
0.00045
0.017
0.34
0.022
0.00086
0.0001
0
0.0618
0.7
0.02
0.0007
0.0296
0.02
0.49
0.57
0.0402
0.2
0.001
0.26
0.7
0.0002
0.29
0.03
0.391
0.0001
0.5
0.031
0.5
0.031
0.003
0.0009
0.4
0.94
0.02
0.03
0.7
0.6
0.73
0.6
0.028
0.6
0.017
0.8
0.015
0.7
0.008
0.0003
0.03
1.6
0.01
0.042
0.15
0.17
3.1
0.49
1.6
0.68
0.017
0.03
1.8
0.041
2.1
0.064
0.017
2.5
0.28
0.022
0.028
1.4
2.2
0.18
0.18
0.028
1.9
1.4
0.01
2.1
0.033
-
2.9
2.2
3.2
1.4
7.1
2.1
2.4
7.7
4.5
2.7
2.5
9.6
7.3
3.0
14.4
9.0
12.1
3.1
12.2
2.7
4.3
2.5
2.2
2.1
6.5
1.8
10.4
4.6
2.1
3.6
3.9
11.5
8.7
12.5
2.4
1.7
3.1
2.6
1.9
2.7
7.7
0.054
0.063
0.166
0.076
0.107
0.037
0.069
0.094
0.027
0.039
0.075
0.027
0.139
0.083
0.094
0.53
0.298
0.183
0.027
0.054
0.141
0.036
0.118
0.206
0.048
0.15
0.209
0.078
0.129
0.066
0.154
0.078
0.021
0.117
0.074
0.066
0.066
0.14
0.091
0.228
0.042
1020
944
463
551
718
1296
733
791
1511
1224
882
1525
464
735
820
296
395
504
1512
859
544
720
398
301
902
456
502
882
370
591
623
783
1874
604
671
749
960
651
807
510
767
3.8E-05
2.4E-05
3.8E-05
1.8E-05
1.0E-04
8.6E-05
5.9E-05
1.1E-04
9.4E-05
9.5E-05
6.4E-05
4.6E-05
9.3E-05
2.2E-05
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4.4E-05
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4.3E-05
4.3E-05
8.1E-05
1.4E-04
2.6E-05
1.1E-04
2.7E-05
5.0E-05
1.2E-04
1.7E-05
3.2E-05
5.3E-05
1.3E-04
5.4E-05
2.1E-05
2
4
2
2
2
2
2
3
3
2
2
2
2
2
3
2
2
2
2
2
2
2
4
4
2
2
2
2
3
2
2
3
3
2
2
2
2
2
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4
2
NoObs
NoObs
NoObs
NoObs
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843.01 2.8728
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846.01 4.1032
847.01 11.0533
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850.01 2.7054
851.01 2.7220
852.01 2.9127
853.01 2.7276
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854.01 4.1155
855.01 5.2392
856.01 5.7434
857.01 2.5010
858.01 2.4580
861.01 1.8610
863.01 2.1284
864.01 2.7477
864.02 4.2836
864.03 1.4038
865.01 8.1358
867.01 3.7401
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870.01 2.7731
2413
3516
448
276
141
997
884
367
4715
10350
3128
4395
1227
1631
3081
2096
1010
26361
3594
727
10320
3982
548
1044
489
1432
24330
14173
859
5738
341
816
1118
765
696
7359
1584
23042
987
1570
900
80
156
23
18
14
32
21
13
92
454
35
41
32
31
149
68
35
550
91
28
317
58
20
29
11
14
571
335
34
97
22
32
45
18
14
142
45
160
19
18
23
106.2753
104.3739
73.3322
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113.9362
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68.9218
106.0116
102.9486
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108.3511
131.5836
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110.2954
119.71309
136.8967
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102.6947
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0.00024
0.0019
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23.3
14
10.44
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24
26.7
15.96
12.5
12
34.98
54.1
28
69.7
9.1
9.73
16
44.82
59.0063
18
32.5
13.63
10.2
21
30
105.3
72.69
30
17
24.2
9.37
9
12.46
36.1
56
120.686
34.88
171
18
37
11.9
4
0.1
66
0.18
0.2
77
1.3
0.96
3.7
1.7
0.96
1.1
87
1.9
4.6
0.14
26
0.76
0.0017
62
6.8
0.25
0.44
79
377
5.3
0.13
1.5
81
7.3
0.41
29
0.27
1.6
5.3
0.085
0.71
13
100
45
3.6
0.04987
0.05283
0.02
0.01505
0.01504
0.031
0.02694
0.0213
0.07226
0.0957
0.0485
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0.03655
0.0531
0.04117
0.0323
0.16567
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0.027
0.0924
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0.021
0.0357
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0.0912
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0.03025
0.0249
0.0253
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0.02
0.00052
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0.00091
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0.018
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0.00073
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0.0027
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0.02
0.5
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0.0149
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0.7
0.62
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0.5
0.0255
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0.769
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0.7
0.45
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0.5
0.002
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0.89
0.3
0.86
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0.84
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0.83
0.53
0.18
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1.6
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0.35
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1.5
0.49
0.035
2
3.6
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0.01
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0.26
1.6
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0.02
0.032
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0.14
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0.74
0.16
4.3
4.9
1.9
1.4
1.4
1.6
1.8
1.4
7.8
10.7
4.0
4.9
2.8
3.1
6.3
2.8
3.6
15.3
5.1
2.8
8.7
5.5
2.4
2.9
2.1
1.9
12.5
13.1
2.2
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1.5
2.7
2.2
1.8
1.8
6.0
3.4
12.5
3.2
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3.6
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564
683
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1273
485
625
774
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1098
583
458
565
399
1169
878
701
534
372
750
704
989
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733
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444
498
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713
1090
1109
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809
478
859
1.0E-04
3.7E-05
1.3E-04
5.8E-05
6.8E-05
5.5E-05
4.9E-05
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6.5E-05
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3.6E-05
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5.6E-05
2.8E-05
6.7E-05
5.6E-05
5.8E-05
2
2
4
4
4
2
2
4
3
2
2
2
2
4
2
2
2
3
2
2
2
2
2
2
4
3
2
3
2
3
3
2
2
4
4
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2
2
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2
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NoObs
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870.02
871.01
872.01
873.01
874.01
875.01
876.01
877.01
877.02
878.01
880.01
880.02
880.03
880.04
881.01
881.02
882.01
883.01
884.01
884.02
884.03
886.01
887.01
889.01
890.01
891.01
892.01
893.01
895.01
896.01
896.02
897.01
898.01
898.02
898.03
899.01
899.02
899.03
900.01
901.01
902.01
4.3907
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1071
40083
6657
363
718
2374
17802
1323
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1362
1774
3757
692
248
1837
3196
24911
36019
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2038
442
1325
622
17546
7353
911
1221
627
14694
2608
1319
14879
1950
1210
1362
858
518
788
1391
6817
8447
29
206
128
19
28
99
89
32
21
33
40
93
32
16
35
29
121
333
86
42
19
25
30
311
219
38
31
25
73
64
47
663
30
23
17
29
25
21
24
123
90
108.6825
112.4222
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0.00011
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0.00026
0.00056
0.000046
0.0017
21.71
38.6
50.2
15.47
16.56
11.42
21.8
19
35.1
19.5
25.1
64.08
12
5
41.2
139
7.8
11.296
24
53.6
11.74
28
22.71
36.26
15.649
14
24
7.85
9.459
32.61
16.7
8.527
31
18
44
24
13.34
35
39.4
53.09
107.2
0.84
2.5
7.4
0.73
0.63
0.11
3.6
78
1.6
6.9
6.9
0.53
41
25
1
42
2.3
0.052
37
1.2
0.55
256
0.76
0.18
0.064
40
95
0.23
0.054
0.45
0.36
0.019
144
96
278
128
0.53
221
1.7
0.54
1.1
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0.01882
0.02429
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0.16675
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0.04552
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0.034
0.028
0.02123
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0.0334
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0.89
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0.8
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0.4
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0.6
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0.01
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0.28
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0.31
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0.017
1.6
1.5
0.35
0.11
0.014
1.3
0.03
3.4
0.017
0.01
1.7
2
0.022
0.01
2.4
2.5
2.7
2.4
2
0.01
0.02
0.01
3.5
10.9
7.4
1.3
2.2
2.2
9.2
2.5
2.3
5.2
4.9
5.8
2.8
2.0
2.5
3.9
13.6
10.0
3.0
2.7
1.2
2.0
2.3
11.7
7.6
2.7
2.8
2.6
12.8
3.9
2.8
12.0
3.0
2.4
2.5
1.7
1.3
1.7
4.3
4.4
5.7
0.081
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751
531
456
866
882
607
693
652
516
568
569
456
936
1275
459
208
1176
829
564
436
797
488
867
754
878
785
654
1091
1093
578
789
1417
540
664
424
510
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397
798
463
270
5.8E-05
1.8E-05
2.0E-05
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1.9E-05
5.4E-05
5.7E-05
8.1E-05
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4.5E-05
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5.8E-05
5.4E-05
1.9E-05
2.3E-05
8.7E-05
1.9E-05
1.6E-05
2.1E-05
2
2
2
2
2
2
2
2
2
2
2
2
4
4
2
2
3
2
2
2
4
2
2
2
2
2
2
3
2
2
2
2
2
2
4
2
4
4
2
2
2
NoObs
1
1
NoObs
NoObs
1
1
NoObs
NoObs
NoObs
NoObs
NoObs
79
903.01
904.01
904.02
905.01
906.01
907.01
907.02
907.03
908.01
910.01
911.01
912.01
913.01
914.01
916.01
917.01
918.01
920.01
921.01
921.02
921.03
922.01
923.01
924.01
926.01
928.01
929.01
931.01
934.01
934.02
934.03
935.01
935.02
935.03
936.01
936.02
937.01
938.01
938.02
939.01
940.01
4.2191
1.8541
3.2550
2.4135
2.5473
4.1177
5.0796
2.9275
3.3536
3.0648
2.2475
2.8941
3.2508
3.2170
1.7644
2.1878
6.5105
2.8954
3.5805
4.0886
1.6334
2.7126
3.4256
2.6522
3.3262
1.8191
4.1458
3.2164
2.9175
3.3818
3.9208
5.1637
6.4005
8.5789
2.5574
1.1718
4.1031
3.2072
1.7854
2.6119
4.7016
7315 262 106.43312
611
20 103.1507
1667
20 111.8263
1773
51 105.6967
871
24 107.1339
961
26
109.117
875
21
123.386
178
8.2
69.3138
8282 398 104.44572
1158
47
104.724
650
22
104.007
1632
24
104.804
18588 1072 102.63655
500
23 102.7363
1387
67 104.31311
828
23 106.3562
15499 228 139.58885
1096
23 123.4895
1137
29 108.3417
1625
32 115.6245
344
10
66.2771
652
19 104.6377
1232
40 107.8993
1115
17 106.3084
1561
75
103.964
474
27 103.8588
7699 252 107.63388
16852 806 103.67816
1662
48 106.0083
581
12
75.543
821
15
80.1226
1942
62 113.0119
1764
43
74.1845
1035
20
67.9393
2215
62 111.4147
729
45
67.5395
982
22 109.5797
1014
29 104.7015
234
16
66.9239
299
17 103.5282
2114 187
102.573
0.00049
0.0031
0.0045
0.0016
0.0033
0.0039
0.0058
0.0097
0.00028
0.002
0.0033
0.0036
0.0001
0.0042
0.00091
0.0032
0.00095
0.0038
0.0034
0.0036
0.0064
0.0049
0.0022
0.0049
0.0017
0.0022
0.00064
0.00014
0.0018
0.0087
0.0085
0.002
0.0038
0.0084
0.0012
0.0011
0.0041
0.0033
0.0043
0.004
0.00073
5.007341
2.211073
27.93886
5.795111
7.15684
16.51385
30.1324
4.79085
4.7083263
5.392096
4.093609
10.84847
4.0822762
3.88667
3.314908
6.71972
39.64552
21.80587
10.28175
18.11903
3.78406
5.15456
5.743325
39.4766
3.166392
2.494093
6.49162
3.8556046
5.826727
12.41208
18.74711
20.85987
42.6329
87.6464
9.467895
0.8930442
20.83479
9.94611
1.0456
3.388069
6.104843
0.000017
9.815
0.000047
7
0.00095
58
0.000065
18.83
0.00016
18
0.0007
32.2
0.002
48.4
0.00021
8
0.0000091 12.227
0.000073
14.21
0.000094
14.8
0.00027
28
0.0000027 10.784082
0.00011
9.85
0.000021
12
0.00015
19
0.00038
51.72
0.0006
53.5
0.00025
23.15
0.00046
36.3
0.0001
19
0.00017
12
0.000091
13.24
0.0014
127
0.000035
7.537
0.000027
12
0.000042 12.851
0.0000038 10.241915
0.000073
15
0.00047
25
0.00068
29
0.00029
25
0.00069
52.68
0.0036
74
0.000083
31.19
0.0000044
6
0.00058
39.5
0.00022
18
0.00002
4.65
0.000089
9.74
0.00003 10.38695
0.034
33
299
0.39
83
1
1.7
60
0.034
0.28
0.73
121
0.000007
0.35
23
69
0.2
2.1
0.2
1
1.7
57
0.3
1723
0.037
35
0.047
0.000011
52
247
220
19
0.37
499
0.49
12
1.4
61
0.29
0.14
0.000051
0.07665
0.027
0.038
0.03715
0.031
0.02811
0.02725
0.017
0.08075
0.03107
0.02338
0.037
0.1216
0.02162
0.037
0.03
0.11111
0.02909
0.03071
0.03581
0.0198
0.026
0.03148
0.03
0.03513
0.023
0.07807
0.1162
0.037
0.023
0.028
0.0426
0.03741
0.029
0.04437
0.026
0.02849
0.032
0.01405
0.01682
0.041
0.00021
0.028
0.042
0.00053
0.029
0.00071
0.00087
0.021
0.00017
0.00049
0.00085
0.031
0.0049
0.00061
0.013
0.02
0.00035
0.0008
0.00069
0.00081
0.0015
0.024
0.00057
0.073
0.00032
0.014
0.00023
0.0075
0.024
0.047
0.042
0.0054
0.00055
0.04
0.00046
0.011
0.00085
0.021
0.00074
0.00056
0.024
0.7
0.6
0.029
0.7
0.03
0.025
0.8
0.0001
0.0403
0.0196
0.4
0.0002
0.0097
0.7
0.7
0.0034
0.031
0.023
0.026
0.0153
0.6
0.015
0.3
0.0107
0.1
0.0007
0.0059
0.3
0.5
0.6
0.64
0.016
0.4
0.031
0.2
0.018
0.7
0.0461
0.018
0.0004
0.01
1.8
2.1
0.037
1.7
0.052
0.01
2
2 .3
1.2
1.6
0.084
0.01
0.037
2
0.03
4.1
2.1
2.1
3.2
2.6
0.8
0.02
2.9
0.039
1.7
0.037
1.6
0.01
-
5.6
2.1
3.0
2.0
2.8
3.5
3.4
2.1
11.4
1.9
1.7
2.6
9.1
1.2
3.9
3.2
10.6
1.9
2.3
2.7
1.5
2.7
2.9
3.1
3.4
2.3
9.0
8.6
3.2
2.0
2.4
3.6
3.2
2.5
3.5
2.0
2.3
2.9
1.3
1.6
3.5
0.057
0.029
0.159
0.062
0.071
0.13
0.194
0.057
0.056
0.057
0.05
0.081
0.049
0.047
0.044
0.071
0.226
0.148
0.089
0.13
0.046
0.058
0.064
0.233
0.043
0.036
0.07
0.048
0.064
0.106
0.14
0.152
0.246
0.397
0.07
0.014
0.146
0.09
0.02
0.045
0.064
853
960
410
698
759
738
604
1115
1140
696
945
521
902
805
1112
932
463
469
618
512
860
951
911
526
1154
1208
998
948
889
691
601
632
496
391
519
1161
530
719
1525
1099
816
6.3E-05
2.9E-05
2.2E-05
7.8E-05
4.1E-05
8.5E-05
8.9E-05
6.7E-05
2.5E-05
4.5E-05
7.7E-05
4.8E-05
4.1E-05
1.3E-04
1.2E-05
3.9E-05
4.1E-05
3.6E-05
5.3E-05
4.0E-05
3.3E-05
2.3E-05
2.6E-05
1.5E-05
4.0E-05
2.6E-05
4.1E-05
1.7E-05
5.1E-05
5.2E-05
6.2E-05
5.2E-05
2
2
2
3
2
2
2
4
2
2
2
2
3
2
2
3
2
2
2
2
4
2
2
3
2
3
2
2
2
4
4
2
4
4
2
4
2
2
4
2
2
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
3
NoObs
NoObs
80
941.01 3.2620
941.02 1.8622
941.03 3.3174
942.01 2.1136
943.01 2.2705
944.01 2.2498
945.01 5.8083
945.02 7.1766
947.01 3.6722
949.01 4.0447
951.01 3.7463
952.01 2.1831
952.02 2.2980
952.03 3.1143
952.04 1.6236
953.01 2.7191
954.01 2.9184
954.02 4.7151
955.01 3.9934
956.01 2.8217
959.01 2.5462
960.01 6.1820
961.01 0.5391
961.02 0.5518
961.03 0.7135
972.01 4.5448
974.01 10.3158
975.01 3.4387
976.01 5.7336
977.01 3.5914
978.01 13.5255
981.01 3.0023
984.01 2.8947
986.01 3.1093
987.01 1.0682
988.01 3.1800
991.01 2.3459
992.01 3.9772
993.01 3.3032
994.01 2.1635
998.01 5.2630
2355
61 107.7862
636
21 103.6646
2621
38 122.0188
1332
33 107.8585
840
33 104.9918
1941
89 103.24424
530
16 121.8574
754
19
79.35
1682
31 122.9264
1144
35 103.7626
2332
67
104.545
1642
40 104.4075
1379
29 103.6308
1897
30
88.2077
385
12
66.6118
2760
98 103.4274
798
29 107.5203
924
19 107.2189
554
28 108.7269
2199
72 108.6457
36851 957 108.07184
39678 1062 110.15256
1609
50 103.48288
1282
71 66.86865
982
31
66.7918
356 134 194.53889
164
37 105.9806
70
37 193.8369
23783 137
117.971
1143
42 194.4372
471 100 195.4346
104
12
194.726
717
12 195.0462
553
19 193.8655
176
13 194.8413
807
9.7 201.0204
298
24
71.2251
416
12
69.4505
406
14
77.3278
212
11
65.8649
88851 564 147.03869
0.0016
0.0034
0.0028
0.0022
0.0023
0.00084
0.0074
0.0085
0.0025
0.003
0.0016
0.0019
0.0026
0.0029
0.0051
0.0011
0.0029
0.0057
0.0035
0.0012
0.00012
0.0002
0.00053
0.00041
0.0011
0.0006
0.006
0.0017
0.0011
0.0019
0.0016
0.0052
0.0047
0.0034
0.0023
0.0038
0.0035
0.0098
0.0074
0.0069
0.00025
6.581521
2.382649
24.66469
11.51507
3.601425
3.108254
25.8529
40.7193
28.59891
12.53274
13.19712
5.901255
8.75246
22.78033
2.896029
3.584109
8.11522
36.9254
7.03918
8.36077
12.713795
15.801109
1.2137724
0.4532882
1.8651126
13.118925
53.5067
2.785755
52.56862
1.353659
18.95486
3.99942
4.28899
8.18758
3.179301
10.38143
12.06208
9.93167
21.85242
4.29889
161.78801
0.000076
0.000056
0.00051
0.00018
0.000058
0.000018
0.0014
0.0016
0.00057
0.00026
0.00014
0.000076
0.00015
0.00031
0.000063
0.000025
0.00016
0.0014
0.00018
0.000072
0.000017
0.000035
0.0000044
0.0000009
0.0000091
0.000085
0.002
0.000034
0.00047
0.000027
0.00049
0.00022
0.00022
0.0003
0.000077
0.00044
0.00018
0.00042
0.0007
0.00013
0.00019
16.67
8
45
37
9
11.23
37.25
35
49
24.61
23
21.08
20
57.6
14.6
10.46
20
52
13
21
47
20.85
9.3
2.6
6.7
16
39.95
3.4
62
2.95
10
2.9
7.9
19
23
11.8
29
18.8
44
11.4
297.87
0.27
45
50
174
31
0.15
0.73
96
15
0.57
29
0.53
40
1.7
1.4
0.11
110
300
84
35
1.2
0.22
2.8
0.78
2
14
0.57
8.7
19
0.89
11
0.87
2.4
157
165
3.5
179
1.2
418
3.4
0.69
0.04256
0.027
0.052
0.034
0.03
0.03893
0.02154
0.028
0.03953
0.03051
0.046
0.03745
0.038
0.04023
0.0188
0.04688
0.027
0.028
0.021
0.044
0.17862
0.18276
0.053
0.19431
0.14
0.0192
0.01176
0.0089
0.1553
0.02656
0.0199
0.0132
0.027
0.022
0.014
0.0328
0.018
0.01897
0.019
0.0142
0.26748
0.00051
0.034
0.012
0.035
0.02
0.00038
0.00081
0.015
0.00093
0.0006
0.012
0.00067
0.011
0.00093
0.0015
0.00038
0.028
0.03
0.024
0.017
0.00065
0.0005
0.0033
0.00081
0.23
0.0025
0.00019
0.0037
0.0015
0.00079
0.0034
0.0012
0.0021
0.039
0.021
0.0021
0.021
0.00098
0.036
0.0011
0.00042
0.03
0.7
0.8
0.6
0.7
0.023
0.04
0.7
0.4
0.0129
0.6
0.028
0.8
0.015
0.0155
0.0058
0.4
0.5
0.3
0.6
0.29
0.46
0.82
1.29
1.2
0.76
0.012
0.8
0.55
0.051
0
0.96
0.58
0.4
0.6
0.84
0.8
0.024
0.5
0.46
0.001
0.035
2.1
0.75
2.1
1.5
0.027
0.01
1.4
0.12
1
0.04
1
0.033
2.6
2.4
2.9
1.3
0.18
0.11
0.25
0.39
0.36
0.74
0.028
1
0.17
0.015
1.2
0.29
0.17
3.1
2.5
0.25
1.8
0.014
3.1
0.14
0.014
5.4
3.4
6.6
2.5
2.2
3.9
2.0
2.6
2.7
2.5
6.0
2.3
2.3
2.4
1.1
4.4
2.3
2.5
2.3
5.1
5.3
13.9
3.9
14.4
10.7
5.3
1.5
1.1
27.5
0.8
3.0
5.9
4.4
1.3
1.3
6.3
3.2
1.6
1.4
1.5
25.0
0.069
0.035
0.165
0.095
0.045
0.041
0.175
0.238
0.146
0.106
0.108
0.05
0.065
0.124
0.031
0.046
0.08
0.219
0.074
0.077
0.063
0.12
0.019
0.01
0.025
0.126
0.289
0.039
0.337
0.014
0.147
0.055
0.054
0.077
0.042
0.097
0.108
0.091
0.152
0.052
0.592
904
1269
585
582
887
1080
595
510
353
670
702
575
504
365
730
1045
792
479
975
746
296
555
1106
1524
964
1540
542
1404
757
628
857
1928
1358
626
1041
947
981
735
519
1032
308
5.4E-05
6.9E-05
4.8E-05
2.2E-05
2.7E-05
4.2E-05
7.0E-05
2.6E-05
2.7E-05
3.7E-05
6.4E-05
6.6E-05
2.5E-05
2.8E-05
2.6E-05
2.9E-05
1.3E-05
3.2E-06
1.7E-05
3.7E-06
1.8E-05
1.3E-05
6.9E-05
6.7E-05
5.6E-05
8.8E-05
1.1E-04
-
2
2
2
2
2
2
3
4
2
2
2
2
2
4
4
2
2
2
3
2
2
2
3
4
4
2
2
2
3
3
4
3
3
2
2
2
2
3
3
3
3
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
NoObs
1
1
1
1
1
1
1
1
1
1
1
81
999.01
1001.01
1002.01
1003.01
1005.01
1008.01
1010.01
1013.01
1014.01
1015.01
1015.02
1017.01
1019.01
1020.01
1022.01
1024.01
1026.01
1029.01
1030.01
1031.01
1032.01
1050.01
1051.01
1052.01
1053.01
1054.01
1059.01
1060.01
1060.02
1061.01
1063.01
1064.01
1065.01
1072.01
1075.01
1078.01
1081.01
1082.01
1083.01
1085.01
1086.01
4.0767
1222
23
79.1504
12.8302
136
19
68.321
1.8181
155
14
65.9865
7.3074 24649 158 105.2651
8.5483
4926 105 130.0317
5.4787 31943 189 181.92435
18.1142
228
12
78.953
0.7714
862
62
66.661
3.1358
1437
19
75.3548
4.4039
552
26
73.1092
3.3973
151
9.6
68.752
4.1116
741
26
74.676
2.5586
39
8.2
68.32
6.3051 10344 300 97.06991
4.6376
1003
14 129.1832
1.8696
783
26
66.2982
18.9471
724
19
118.039
5.5950
668
15
66.871
2.8480
418
10
71.431
6.1479
304
8.6
68.978
24.0138
4165
87 109.1034
1.5002
349
37
66.3422
2.9340
429
18
71.1168
4.3752
546
15
76.3472
1.6860
230
14
66.2102
3.7930
219
13
67.384
1.4113
153
15
66.4557
5.5786
249
17
73.2117
4.8600
127
13
70.697
5.8923
406
14
75.732
5.0997 266763 7754 109.30531
3.2021 19234 310 66.46468
3.8421 21849 257 66.63778
3.6243
465
19
72.112
1.7654
4752 168 66.27522
1.4965
1305
30
67.8711
3.2893
619
24
67.3026
2.5360
521
12
68.2737
3.5414
338
14
71.5846
1.9381
428
10
72.1556
5.9559
438
17
77.8771
0.0052
0.014
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0.0014
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0.0052
0.011
0.0046
0.01
0.00072
0.008
0.0027
0.018
0.011
0.009
0.019
0.0044
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0.008
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0.0091
0.0039
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0.01
0.01
0.00006
0.00033
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0.006
0.0004
0.002
0.0042
0.0071
0.0079
0.0069
0.0092
16.56815
20.4024
3.481678
8.360619
35.61842
300
110.645
0.5187505
17.31731
9.42869
4.08909
17.44529
2.49677
54.35611
18.82778
5.747732
94.1023
32.3113
9.22978
14.5563
615.3
1.2690943
6.79673
17.0282
1.224848
3.32361
1.022666
12.10963
4.75793
41.818
89.69815
1.1873532
4.0206268
10.12804
1.343764
3.353682
9.95693
6.50318
7.33679
7.71794
27.6625
0.00039
30
0.0013 12.28752
0.000066
18.11
0.000057
9.94
0.00039 33.93486
361
0.021
26
0.0000015
6.51
0.0004
45
0.00018
16
0.00017
6
0.00036
23
0.00011
7.94
0.0002
42
0.00079
32
0.000065
25.2
0.0097
38.8
0.0014
47.1
0.00036
24.8
0.0012
17
4.3
106
0.0000089
4
0.00016
19.8
0.00058
18
0.000025
3
0.00013
7.05
0.000017
8.259
0.00045
17.02
0.00021
5
0.0021
34
0.000024
198
0.0000017
3.25
0.0000084
5.07
0.00026
19.22
0.0000023
5.4
0.000029
18.96
0.00018
21.7
0.0002
20.98
0.00025
16.4
0.00023
30.9
0.0012
24
215
0.00076
0.9
0.06
0.00038
108
48
0.21
384
108
42
84
0.47
12
1.7
1.1
1.1
2.3
1.5
146
32
16
0.93
65
15
0.28
0.023
0.69
25
162
59
0.97
0.41
0.34
1.6
0.81
1.2
0.25
0.96
4
93
0.032
0.01033
0.01455
0.1409
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1.46567
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0.0223
0.018
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0.01749
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0.4741
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0.061
0.029
0.02
0.02
0.00041
0.0024
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0.0008
0.001
0.0011
0.032
0.0015
0.015
0.00075
0.017
0.018
0.00055
0.0004
0.00053
0.012
0.019
0.00024
0.00039
0.0053
0.00099
0.00038
0.001
0.00081
0.0011
0.00082
0.0019
0.016
0.4
0.0848
0.0047
0.0023
5.3
0.85
0.014
0.2
0.3
0.8
0.7
0.018
0.88
0.025
0.073
0.019
0.007
0.089
0.4
0.86
0.8
0.0435
0.8
0.8
0.027
0.134
0.008
0.8
0.8
0.87
0.467
0.297
0.0461
0.052
0.0542
0.032
0.015
0.8
3
1.6
0.86
0.03
3.4
3
1.9
1.6
0.26
0.05
0.076
0.014
0.01
3.2
0.26
1.3
1.3
1.4
0.048
0.01
1.6
1.6
0.16
0.01
0.089
0.01
0.01
0.01
1.5
2.9
2.6
1.0
14.1
6.5
204.8
2.7
1.6
2.7
2.4
1.6
3.0
1.2
21.9
2.8
1.7
1.8
2.5
1.8
2.0
26.2
2.3
1.7
2.6
1.9
2.0
1.4
1.5
1.2
2.3
93.4
15.7
18.9
2.1
7.4
1.9
1.4
1.9
1.6
1.2
2.5
0.125
0.159
0.043
0.08
0.208
0.895
0.48
0.012
0.12
0.091
0.052
0.133
0.037
0.294
0.139
0.052
0.325
0.203
0.088
0.119
1.558
0.022
0.071
0.133
0.022
0.043
0.019
0.107
0.058
0.241
0.418
0.023
0.051
0.094
0.024
0.034
0.092
0.066
0.075
0.063
0.184
583
1006
842
766
469
283
506
1641
502
921
1218
659
1364
580
612
635
242
558
799
728
300
1462
841
719
1466
1116
1400
856
1163
520
547
1939
1160
881
1736
660
732
763
834
573
623
8.7E-05
8.1E-05
9.5E-05
-
2
3
3
3
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
3
4
4
4
4
4
4
4
4
4
4
1
1
1
1
1
1
82
1089.01 10.1641
1089.02 2.8501
1094.01 4.7951
1095.01 2.7384
1099.01 3.7160
1101.01 2.2767
1102.01 3.8679
1102.02 3.8409
1106.01 3.6049
1108.01 3.6924
1109.01 6.4230
1110.01 3.5692
1111.01 3.7924
1112.01 7.9162
1113.01 4.6584
1113.02 7.0361
1114.01 2.3308
1115.01 6.0624
1116.01 1.9015
1117.01 6.1980
1118.01 1.7024
1121.01 4.0277
1123.01 1.1651
1128.01 1.7084
1129.01 1.4556
1134.02 7.7281
1140.01 0.6290
1141.01 2.7088
1142.01 2.0797
1144.01 3.4602
1145.01 5.3510
1146.01 2.0887
1148.01 4.7868
1149.01 1.7338
1150.01 1.9085
1151.01 3.3203
1151.02 3.4924
1152.01 3.4095
1153.01 1.6005
1154.01 7.8146
1156.01 1.3680
8682
1893
847
5841
4771
362
543
408
366
369
231
339
358
436
412
491
304
232
187
148
198
58683
1856
192
336
12103
1146
765
465
225
486
403
202
269
82
113
116
84601
36772
14832
2964
199 108.5986
61
73.321
24
68.5851
50 136.9783
34
131.003
11
67.8593
18
70.6093
17
73.563
15
72.9022
18
73.0373
11
67.738
11
68.093
10
69.5
14
91.323
18
82.7491
15
91.699
11
72.7953
17
69.3262
21
68.1021
21
74.7572
12
70.6009
441 73.69733
116 66.58381
44
66.0736
9.1
66.3832
109 389.8516
120 66.44743
15
68.1853
16
66.4288
14
67.5826
23
95.8746
12
69.3494
15
68.4025
7.3
69.2328
20
66.9456
14
67.8179
12
68.7486
309 111.24288
273 67.01944
713 69.04584
112 67.36536
0.0011
0.0015
0.0056
0.0019
0.0027
0.0075
0.0063
0.0067
0.0069
0.0063
0.015
0.01
0.011
0.013
0.0072
0.01
0.0073
0.0097
0.0033
0.0081
0.0056
0.00035
0.00044
0.0015
0.0063
0.0025
0.00023
0.0063
0.0046
0.0077
0.0052
0.0063
0.009
0.0088
0.0036
0.007
0.008
0.00037
0.00053
0.00031
0.00048
86.67747
12.21822
6.10027
51.59825
161.5252
2.847635
12.3318
8.14561
7.42603
9.46255
6.72233
8.73492
10.26494
37.8122
25.93496
83.4411
7.0472
12.99172
3.749224
11.08977
7.37325
14.154037
0.8484851
0.9748817
4.89768
200.623
0.5532587
5.72796
3.755719
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30.5908
7.09695
11.47566
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0.677375
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4.7222503
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1.8724219
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0.000083
0.00015
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0.0021
0.000091
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0.00024
0.00022
0.00026
0.00043
0.00039
0.00051
0.0023
0.00086
0.0042
0.00022
0.00055
0.000053
0.00039
0.00018
0.000021
0.0000016
0.0000064
0.00013
0.016
0.0000006
0.00015
0.000073
0.000078
0.00075
0.0002
0.00044
0.00027
0.000011
0.00015
0.00025
0.0000086
0.0000029
0.000009
0.0000038
70.54
19
9.95
70
352.6
10.01
14
11.4
14.1
20.15
8
20.4
21.3553
36.4
23
52
14.1
16.66
14
11
36.4
27.2
4.1
4.493
24
169
6.888
16.43
13.9
5.44
45.6
22
10
18.3
2.78
11.62
18.1
12.99
2.39
7.3972
6.7
0.26
12
0.32
21
9.6
0.88
36
1.2
1.6
0.89
83
1.4
0.0018
1.6
84
141
4.2
0.45
68
41
3.1
8.2
1.2
0.078
145
51
0.071
0.91
4.2
0.21
1.4
201
44
5.5
0.22
0.54
1
0.5
0.061
0.009
2
0.0827
0.0488
0.02633
0.2841
0.0613
0.0177
0.025
0.0074
0.0093
0.01828
0.013
0.0182
0.02
0.01946
0.022
0.023
0.0181
0.01371
0.013
0.0119
0.01365
0.2488
0.04351
0.01342
0.022
0.1085
0.03185
0.0273
0.01927
0.01666
0.02011
0.024
0.015
0.0173
0.00648
0.0107
0.0109
0.2689
0.2025
0.10842
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0.00028
0.006
0.00072
0.0019
0.0012
0.0012
0.013
0.0031
0.0013
0.00064
0.03
0.0011
0.83
0.00084
0.014
0.012
0.0014
0.00052
0.013
0.009
0.00097
0.0012
0.00044
0.0003
0.027
0.0021
0.00021
0.0012
0.00098
0.00054
0.00055
0.044
0.012
0.0021
0.00053
0.00041
0.00051
0.003
0.0018
0.00011
0.00059
0.002
0.86
0.0201
1.41
0.031
0.0617
0.8
0.744
0.015
0.012
0.4
0.031
0.041
0.053
0.8
0.8
0.66
0.012
0.4
0.6
0.023
0.54
0.56
0.0103
0.7
0.5
0.028
0.0488
0.031
0.0224
0.023
0.7
0.8
0.7
0.0522
0.0566
0.057
0.41
0.79
0.71
0.022
0.48
0.42
0.056
1.1
0.022
0.014
0.01
3.6
0.01
0.01
0.014
1.2
1.1
0.2
0.014
2.3
1.8
0.01
0.16
0.17
2.1
0.15
0.017
0.009
0.014
2.4
1.3
0.21
0.01
0.21
0.11
0.21
9.6
5.7
2.4
25.8
3.7
1.1
3.2
0.9
0.9
1.4
1.4
1.9
1.6
2.2
2.6
2.8
2.2
2.0
1.4
1.2
1.8
24.7
4.4
1.0
2.7
9.7
11.2
2.0
1.5
1.6
2.0
1.3
2.2
1.6
0.7
1.2
1.2
19.2
20.8
22.2
6.0
0.395
0.107
0.066
0.272
0.573
0.036
0.108
0.082
0.076
0.086
0.068
0.085
0.092
0.226
0.178
0.388
0.073
0.111
0.048
0.101
0.077
0.115
0.018
0.019
0.056
0.646
0.015
0.052
0.046
0.036
0.195
0.056
0.104
0.072
0.015
0.059
0.075
0.046
0.015
0.077
0.029
429
824
893
422
244
865
841
966
905
672
822
837
689
547
676
458
960
837
1144
842
1049
676
1784
1378
959
245
3538
634
892
1250
549
512
952
783
1940
989
877
676
2137
1522
1289
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
83
1157.01
1159.01
1160.01
1161.01
1162.01
1163.01
1163.02
1164.01
1165.01
1166.01
1168.01
1169.01
1170.01
1171.01
1175.01
1176.01
1177.01
1178.01
1180.01
1185.01
1187.01
1190.01
1192.01
1193.01
1198.01
1198.02
1199.01
1200.01
1201.01
1202.01
1203.01
1203.02
1204.01
1205.01
1207.01
1208.01
1210.01
1212.01
1214.01
1215.01
1215.02
5.0609
5.0986
3.1995
3.7439
11.7092
1.8096
3.4700
3.5820
1.8463
1.5231
23.2431
1.5932
1.2491
1.7492
12.4129
1.8347
2.5220
7.6265
10.2896
1.4882
0.7778
1.3773
17.0021
3.2991
5.4692
5.2647
5.5648
1.4296
0.9997
1.3660
5.2656
3.3983
6.4828
5.2040
2.1368
8.5880
5.8162
3.8647
2.8863
7.4620
7.2268
1474
2444
1083
371
934
347
348
224
513
557
845
196
510
182
115
30840
21340
13791
18755
1707
1835
727
1399
2692
660
303
1056
424
616
414
813
516
326
378
718
3312
286
274
177
228
255
377
34
19
21
65
20
17
15
35
15
28
48
19
21
13
735
46
132
488
108
187
34
31
33
17
9.9
23
41
12
15
15
12
13
19
16
74
17
9.4
9.8
25
20
66.38704
99.1389
73.5808
68.9164
106.9379
68.7149
67.8239
66.3891
69.3531
66.2153
161.4507
66.2862
70.3023
66.5297
75.956
111.6887
113.6797
67.3695
96.01592
66.86259
66.79903
111.5863
105.5114
82.2193
72.4887
75.726
80.864
66.3066
66.0546
66.8036
93.2296
75.9003
69.33
72.9508
75.3282
182.4388
67.0989
67.918
66.4458
75.118
78.3889
0.00048
0.0072
0.0053
0.0054
0.0033
0.0034
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0.002
0.004
0.008
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0.0037
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0.9337473
64.6198
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458
0.6892091
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2.757529
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31.8811
14.12823
8.39776
8.63851
13.73459
300
14.55495
11.30143
4.24176
17.32298
33.0058
0.0000019
1.2
0.002
54
0.00029
32.4
0.00014
9
0.0026
90
0.000043
12.94
0.00022
18.36
0.000088
5.95
0.00006
34.8
0.00013
30
2054
154
0.000004
3.4
0.00009
29
0.000005
2.112
0.0028
19.76
0.000001
9.635
0.00003
11.3
0.000032
5.3
0.000099
22.65
0.0000034
5.2
0.0000004
3.809
0.0000022
2.32
0.0077
57.3
0.0011
59
0.00063
20
0.00063
16.75
0.0015
76.9
0.000002
1.4
0.000046
13
0.000015
6.04
0.0014
46.8
0.00054
21
0.00048
9.82
0.00029
8
0.00028
29
- 182.55974
0.00057
19.4
0.00059
24.8
0.00017 9.81878
0.00055
13
0.0015
35
0.36
18
1.6
46
86
0.56
0.88
0.26
1.3
221
693
1
185
0.058
0.73
0.024
3.4
1.6
0.45
1.6
0.035
0.69
0.19
18
152
0.97
2.5
1.1
3.9
0.28
2.4
146
0.3
34
158
0.8
2.1
0.0004
38
289
0.04357
0.0538
0.0296
0.02
0.0285
0.01869
0.01746
0.01489
0.02087
0.028
0.02577
0.01247
0.024
0.01437
0.00972
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0.83
0.87
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0.54
0.0677
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0.8
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0.74
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0.038
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0.67
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0.047
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0.9
0.8091
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0.25
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2
1.9
0.02
0.01
0.13
0.22
0.069
0.31
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0.01
0.028
0.75
0.2
0.07
2
0.01
1.6
1.4
0.01
0.01
1.5
3.4
17.8
5.3
1.8
2.3
3.9
1.9
1.8
1.2
2.9
2.8
3.9
1.2
1.4
1.1
0.9
11.1
9.8
13.7
13.8
5.8
2.5
2.0
4.1
12.9
2.0
1.5
2.7
2.4
1.4
1.5
2.5
2.4
1.7
2.1
2.9
7.0
1.2
1.8
1.5
2.2
2.1
0.021
0.304
0.104
0.065
0.594
0.04
0.079
0.032
0.074
0.078
1.221
0.015
0.073
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0.043
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0.01
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0.128
0.095
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0.015
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0.117
0.083
0.085
0.111
0.913
0.119
0.101
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3067
372
529
925
375
1153
821
829
1009
880
291
1895
670
2046
493
974
945
1293
478
1699
1789
2118
362
463
679
788
379
2399
686
1104
544
713
906
888
650
301
673
798
1146
869
701
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
84
1216.01
1218.01
1219.01
1220.01
1221.01
1221.02
1222.01
1225.01
1226.01
1227.01
1228.01
1229.01
1230.01
1232.01
1236.01
1236.02
1238.01
1240.01
1241.01
1241.02
1242.01
1244.01
1245.01
1246.01
1247.01
1251.01
1257.01
1258.01
1261.01
1263.01
1264.01
1266.01
1268.01
1270.01
1272.01
1273.01
1275.01
1276.01
1278.01
1278.02
1279.01
4.0428
4.7972
3.0841
2.3617
7.8099
12.5482
3.2088
1.7802
7.8230
1.7476
2.4024
1.5996
31.8501
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5.6648
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10.5451
12.6584
4.6572
3.0620
5.3201
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3.9417
1.2398
4.4410
6.3287
11.5198
9.5353
3.5197
3.9623
10.3358
1.2127
2.3435
5.3917
6.3429
5.1517
5.8956
6.2243
4.9091
181
16
67.3671
291
21
66.6822
97
7.8
67.686
129
14
69.8892
149
16
71.535
131
15
85.316
59
8.7
67.499
28197 668 66.31535
83463 1238 106.16362
18166 105 66.57494
17248 376 68.26916
10490 210 66.29515
6463 313
147.034
18640 289 165.64948
748
39
84.0494
194
20
70.6889
532
24
72.1086
256
26
66.6516
342
30
80.0705
153
22
68.746
2822
85 216.2398
327
18
67.0974
260
18
73.7271
354
13
81.5517
22189 455 67.54977
9222 383 67.10443
8084 110 106.7926
3080
58
93.3913
5135
90 149.0435
1074
27
66.8815
1122
25
75.2628
886
30
70.6651
6430
76 293.0702
885
29
71.5555
201
60
66.8481
1155
35 102.9068
1053
50 100.6306
561
26
71.6997
285
14
78.079
740
20
94.3182
317
25
71.2073
0.0074
0.006
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11.13127
29.61863
3.50394
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51.0917
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137.75992
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3.6613278
0.7697382
165.7537
238.8147
35.74468
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27.07239
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10.49447
99.642
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191
5.729434
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50.28661
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14
0.000043
0.0000033
0.00075
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0.00052
0.00061
0.0016
0.00035
12
28
8.93
15.6
27
18
10.81
6.6
169
10.6
8.82
4.1
43.5
131
35.69
8.25
29.55
7.74
9
4.2
95
23
20.1
23
5.988
3.9
164.8
37
94.43
25.99
31.8
23.21
135.9
20
1.924
58.8
56
26
16.24
56.8
22.86
51
91
0.24
4.7
149
46
0.53
2
51
3.2
0.27
1.2
2.4
39
0.62
0.21
0.86
0.27
10
8.5
29
178
0.8
97
0.012
1.2
1.4
22
0.75
0.61
1.1
0.66
9.9
65
0.025
1.3
150
94
0.72
2
0.67
0.015
0.018
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0.011
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0.8
0.034
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0.6
0.8
0.018
0.58
0.81
0.62
1.4
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0.8
0.78
0.5
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0.4742
0.9
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0.4
0.7
0.061
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1.2
0.01
0.14
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1
0.01
0.17
0.12
0.22
0.42
0.033
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0.67
1.1
0.23
2.8
0.01
1.2
0.01
0.02
0.72
0.017
0.039
0.01
0.047
1.1
0.039
1.8
1.7
0.01
0.01
0.033
2.0
2.2
1.2
1.1
5.0
5.3
0.8
14.3
26.6
8.3
14.8
7.8
50.2
48.6
2.8
1.7
2.1
1.5
10.4
7.0
6.3
1.5
1.5
2.4
19.7
6.8
10.4
4.2
6.3
2.0
2.7
2.0
8.6
2.0
1.9
2.8
3.3
1.5
1.6
2.4
1.1
0.101
0.192
0.044
0.065
0.212
0.301
0.048
0.023
0.514
0.032
0.046
0.016
0.67
0.75
0.222
0.069
0.177
0.033
0.17
0.106
0.436
0.097
0.116
0.144
0.04
0.013
0.385
0.214
0.521
0.182
0.114
0.087
0.671
0.06
0.013
0.23
0.269
0.154
0.107
0.25
0.115
883
593
1031
797
944
792
841
1002
301
1066
1058
1669
650
277
627
1125
543
1272
1142
1446
412
746
774
723
1617
1808
398
446
335
393
637
543
336
698
2667
460
466
474
744
487
584
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
85
1281.01 2.8618
1282.01 8.5310
1283.01 5.8824
1284.01 2.3467
1285.01 1.6718
1288.01 6.6527
1290.01 3.2832
1293.01 1.8991
1295.01 1.6040
1296.01 4.0478
1298.01 2.0927
1299.01 15.1959
1300.01 1.1440
1301.01 2.6177
1301.02 3.5078
1302.01 6.8896
1303.01 18.2696
1304.01 3.1186
1305.01 2.2079
1306.01 1.7321
1306.02 2.2614
1306.03 3.7452
1307.01 3.8988
1307.02 2.3012
1308.01 5.5317
1309.01 4.6916
1310.01 3.6617
1311.01 7.2596
1312.01 2.6895
1314.01 7.8679
1315.01 3.4409
1316.01 6.4621
1318.01 2.5645
1321.01 1.5476
1324.01 1.4501
1325.01 3.4427
1326.01 3.5523
1328.01 3.1414
1329.01 5.1611
1335.01 11.2408
1336.01 3.6241
568
15
230
30
58
20
8533 426
4957
94
9044 135
3485
78
3999
88
684
51
34583 1371
1509
28
856
68
452
57
763
13
1134
13
873
28
416
24
322
11
284
15
259
14
287
13
234
11
799
23
556
18
415
24
289
25
438
16
625
32
283
15
139
18
148
21
54
16
19619 195
6016 245
1448 113
2926
93
13485 847
4981
25
1074
24
1862
40
458
15
74.8243
95.883
71.0524
66.12539
67.72319
152.7044
77.7765
66.72149
66.3081
68.32449
76.2253
104.5278
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117.9894
122.2828
120.558
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69.4812
67.5591
66.327
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66.458
105.4744
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66.96805
67.22337
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86.6605
226.4189
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49.4787
30.86317
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11.973777
11.703074
1.577794
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11.00823
52.4989
0.6313314
12.69902
37.5214
55.6394
34.2936
4.59723
2.633895
1.796375
3.468005
5.91495
44.84967
20.342
23.58427
10.11672
19.12903
83.5755
6.14681
8.57549
6.84639
7.64981
1.6346139
0.711965
0.5220586
10.035392
53.100927
80.966
33.19959
127.8295
10.21869
0.0012
134
0.00087
28.97
0.00026
10.16
0.0000016
5.5
0.0000028
2.12
0.001
170.9
0.000072
23.8
0.000043
25.5
0.0000082
7.86
0.0000005
4.344
0.00013
22
0.0013
28
0.0000025
4.779
0.00037
33
0.0014
60
0.0014
63.6
0.0021
14.62
0.00018
9
0.000057
9.19
0.000036 10.201
0.000088
6
0.00027
9
0.00096
96
0.00039
58
0.00063
28
0.00022
11
0.00057
36
0.0021
93.4
0.00015
19.34
0.00038
6
0.00015
7
0.00033
9.1
0.0000031
5.5
0.0000008
3.14
0.0000012
2.94
0.000051 23.55971
0.000065
70
0.0014
266
0.00088
50.6
0.0072
84
0.00031
22
1323
0.62
0.31
1.7
0.28
1.2
7 .2
7.7
0.18
0.027
20
0.24
0.012
379
432
1.6
0.32
60
0.11
0.054
28
63
1068
404
134
32
330
2
0.19
22
23
2.7
1.7
0.94
0.035
0.00012
21
15
1.7
221
1.1
0.022
0.0138
0.00717
0.08219
0.0814
0.08401
0.05627
0.0757
0.0243
0.17956
0.0445
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0.034
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0.0174
0.02101
0.022
0.018
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0.024
0.019
0.0175
0.02
0.0223
0.01764
0.012
0.0142
0.00653
0.12474
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0.03508
0.049
0.44508
0.061
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0.04
0.02046
0.045
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0.00021
0.00025
0.0029
0.00047
0.00059
0.0019
0.00044
0.0003
0.0079
0.00024
0.00025
0.064
0.048
0.0006
0.00046
0.029
0.00058
0.00057
0.018
0.025
0.058
0.033
0.019
0.01
0.037
0.00045
0.00062
0.0086
0.0077
0.00032
0.00065
0.00034
0.00029
0.037
0.00036
0.0025
0.0008
0.021
0.00081
0.4
0.027
0.028
0.9
0.008
0.38
0.86
0.0138
0.635
0.9
0.021
0.07
0.6
0.7
0.004
0.026
0.7
0.0493
0.0975
0.9
0.7
0.1
0.7
0.6
0.8
0.5
0.026
0.084
0.7
0.89
0.41
0.013
0.0227
1.71
0.024
0.027
0.5
0.026
3.4
0.01
0.01
0.19
0.014
0.12
0.26
0.071
0.5
0.017
3.4
2.2
0.01
0.03
2.3
1.3
2.3
4
2.2
2.2
1.3
3.1
0.032
1.6
0.96
0.12
0.022
0.51
0.055
0.042
1.7
0.049
2.0
2.0
0.7
10.8
8.0
9.8
5.8
7.1
2.4
23.6
3.7
10.2
1.7
1.9
2.3
2.4
2.6
1.8
1.3
2.1
2.2
1.8
3.0
2.8
2.0
2.5
2.0
3.4
1.6
3.5
1.9
0.7
13.7
8.8
3.6
3.3
40.5
4.8
2.5
7.6
2.5
0.265
0.201
0.077
0.028
0.019
0.488
0.105
0.103
0.027
0.036
0.084
0.305
0.013
0.104
0.215
0.289
0.21
0.055
0.036
0.029
0.046
0.065
0.252
0.149
0.164
0.098
0.143
0.391
0.067
0.089
0.074
0.075
0.028
0.016
0.013
0.09
0.272
0.362
0.198
0.528
0.095
431
688
883
1800
1606
400
786
732
1488
1409
554
748
1485
588
409
427
579
964
1020
1431
1136
956
505
657
607
1117
657
494
950
1213
1106
936
1552
1915
1951
652
399
338
457
480
884
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
86
1337.01 1.8187
1338.01 3.0650
1339.01 2.8821
1341.01 2.9285
1342.01 3.1222
1344.01 2.6231
1345.01 2.0859
1346.01 2.7042
1348.01 2.9866
1349.01 3.8745
1353.01 10.8183
1355.01 5.1862
1360.01 4.5398
1360.02 2.3547
1361.01 4.8039
1363.01 2.3642
1364.01 4.0375
1364.02 2.8321
1366.01 4.5442
1367.01 0.9983
1369.01 2.7220
1370.01 2.3585
1372.01 10.4241
1375.01 4.7760
1376.01 2.6400
1377.01 5.0697
1378.01 4.8532
1379.01 2.4909
1381.01 3.8584
1382.01 3.7694
1383.01 3.0149
1384.01 1.6620
1385.01 4.0744
1386.01 2.0583
1387.01 4.8792
1389.01 2.2375
1390.01 1.5474
1391.01 1.9404
1395.01 1.5514
1396.01 3.1586
1396.02 2.5938
237
13
67.5043
229
16 111.0667
267
15
67.9005
232
14
67.0276
174
17
67.0578
127
15
66.3603
48165 262
66.6039
52057 318 70.07146
16949
93
70.5634
22623 107
75.187
13387
72 169.6578
3085
35
84.9328
1494
25
97.298
907
17
74.93
1478
32
84.1831
494
16
67.8975
924
13 119.0465
785
16 114.9246
962
28
97.7735
342
33
67.06
276
19
66.8903
436
12
68.2586
530
12
109.049
2569
61 139.9267
297
21 117.2434
193
12
67.557
237
23
66.3534
162
20
69.8878
64104 411 67.58585
49487 148 112.53263
45922 317 69.14077
38858 415 66.04537
49147 772 72.08453
16933 537 66.80499
59843 1404 85.56423
21642 162 67.79932
9692 124 67.50781
4574
90
66.8021
1579
20 114.2969
844
21 116.9867
368
11 113.2709
0.0052
0.0059
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7
8.24
8
11.49
9.94
15.27
1.6
13.5
22
26.2
115.5
80.9
62
39
100.4
11.87
41.3
20.6
33.04
5
9.07
22.7
43
207
21.28
17.91
30
18.43
9.54
10.271
6.74
3.25
42
4.7
36
10.3
8.1
17.9
35.1
16.7
11.85
39
0.36
66
0.18
0.4
0.15
0.48
4
6.6
7.9
1.4
1.9
441
361
2.5
0.74
2.6
1.2
0.94
31
0.11
1.7
265
62
0.8
0.96
181
0.85
0.24
0.082
0.49
0.97
13
1.4
11
2.5
4
5.4
2.7
0.72
0.85
0.016
0.01526
0.016
0.0133
0.01364
0.01191
0.19676
0.2291
0.1158
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0.01
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0.5
0.0451
0.7
0.2746
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0.49
0.72
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0.6
0.017
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0
0.6
1.14
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0.3
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0.69
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0.82
0.191
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0.88
0.59
0.84
0.0253
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0.15
0.22
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2.9
0.032
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0.01
0.039
2.9
0.01
2.4
0.34
0.014
2.8
0.13
0.18
0.057
0.018
0.22
0.26
0.68
0.25
0.01
-
1.4
1.7
2.0
1.6
1.6
1.1
18.2
22.2
7.7
19.6
18.1
2.8
2.7
2.3
2.2
1.8
2.9
2.7
2.4
1.2
1.8
1.7
2.2
17.9
2.8
1.6
1.3
0.8
25.0
24.1
28.4
18.6
15.1
12.9
31.1
16.3
6.9
8.3
2.5
2.5
1.9
0.03
0.044
0.052
0.055
0.049
0.054
0.009
0.056
0.075
0.133
0.52
0.266
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0.013
0.042
0.071
0.338
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0.13
0.062
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0.014
0.138
0.022
0.165
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0.024
0.08
0.064
0.07
0.048
1177
1195
1150
1165
1242
1021
2237
989
676
783
469
342
408
555
279
1052
596
854
582
1639
1239
795
416
300
1337
868
590
790
1004
1191
1313
1818
581
1685
615
1021
976
921
718
884
1067
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
87
1400.01 3.3141
1401.01 2.6369
1402.01 3.8080
1403.01 3.0231
1404.01 3.0415
1405.01 4.0389
1406.01 3.9013
1407.01 2.6597
1408.01 3.2050
1409.01 2.4035
1410.01 4.5646
1412.01 8.7616
1413.01 7.9911
1415.01 1.7411
1416.01 4.3558
1419.01 1.3238
1422.01 2.0371
1422.02 2.9373
1422.03 1.5785
1423.01 4.0874
1424.01 1.5471
1425.01 2.1991
1426.01 6.7799
1426.02 5.2850
1426.03 4.8985
1427.01 1.7776
1428.01 1.4407
1429.01 10.1791
1430.01 2.3132
1432.01 3.4501
1433.01 3.6136
1434.01 2.1140
1435.01 8.4693
1436.01 2.4834
1437.01 3.2369
1438.01 5.6224
1439.01 23.0602
1440.01 3.0898
1441.01 3.1188
1442.01 1.5890
1444.01 6.4860
783
261
461
824
467
536
522
217
565
731
597
379
185
34162
26075
2118
1361
1574
461
4570
486
514
924
4370
4322
564
476
2462
1055
455
705
282
519
230
287
199
1176
266
283
127
413
70
75.3301
64
66.8031
14
70.1876
15
74.7225
11
68.2404
11
119.3
27
69.9238
14
67.2441
16
78.4231
19
66.4929
21
83.2427
22
67.6756
16
71.634
250 66.80918
154
68.335
95 111.25851
26
68.9225
20
66.6483
10
67.7522
30
83.5949
35
66.4598
29
66.7336
29 104.2748
88
58.0562
76 157.6733
18
66.1119
60 66.90506
33 185.7365
22
85.6439
19
71.4089
13
72.3786
14
66.2056
26
79.5568
16
68.0097
8.8
66.896
25
69.6485
72 110.8684
11
69.0574
12
67.646
36
67.1309
19
73.2196
0.0015
0.0014
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14.72
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40
0.00026
13
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23.5
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16
0.000039
4
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36.3
0.00031
25.3
0.00043
26.6
0.0016
33.8
0.00064
9
0.0000004
1.75
0.0000094 5.026097
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4.1
0.000071
17
0.00038
57.3
0.000093
18.6
0.0019
277.7
0.0000092
7.26
0.000024
5
0.00096
46.5
0.00065
86
0.0015
103
0.000041
11.48
0.000004
5.068
0.0078
161.6
0.00017
35
0.00016
14
0.0007
37
0.000051
8.4
0.0014
36
0.000055
8.09
0.00034
11
0.00018
9.59
26
393.3
0.00027
19.1
0.00031
12
0.0000049
2.54
0.0018
34
0.32
0.018
0.7
408
98
1.5
59
52
2
7.6
2
1
39
0.53
0.000027
1.3
94
2.8
1.6
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0.22
59
1
17
31
0.78
0.098
3.4
300
91
391
0.14
174
0.4
90
0.27
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1.3
86
0.76
117
0.02523
0.01408
0.02196
0.028
0.024
0.023
0.023
0.01
0.02179
0.0307
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0.01294
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0.00018
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0.012
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0.043
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0.041
0.0013
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0.0015
0.00049
0.028
0.00056
0.0028
0.001
0.00098
0.00034
0.00087
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0.00076
0.02
0.00063
0.031
0.00032
0.00098
0.025
0.00026
0.014
0.029
0
0.0547
0.6
0.7
0.085
0.7
0.5
0.021
0.83
0.057
0.007
0.7
0.0081
0.9
0.7
0.02
0.0002
0.031
0.0673
0.8
0.017
0.79
1.53
0.0377
0.017
0.008
0.3
0.5
0.5
0.1399
0.3
0.0331
0.8
0.021
0.0686
0.032
0.8
0.46
0.8
0.032
0.025
3.1
2.4
0.01
1.6
3.7
0.01
0.25
0.017
0.01
1.8
0.3
2
0.044
0.062
2.5
0.01
0.32
0.46
0.074
3.3
2.6
3.3
2.5
2.2
0.033
0.01
1.7
0.14
1.4
2.9
2.0
1.7
2.0
1.5
2.1
2.5
0.7
1.8
3.7
1.6
2 .1
1.5
18.8
16.9
5.8
3.1
2.9
2.0
4.3
1.6
0.8
3.3
7.7
36.1
1.5
1.9
4.2
2.3
1.9
1.7
1.4
1.7
1.5
2.2
1.5
4.1
1.4
2.3
1.6
3.0
0.091
0.014
0.073
0.117
0.06
0.102
0.102
0.024
0.098
0.13
0.126
0.228
0.107
0.009
0.037
0.024
0.051
0.116
0.037
0.475
0.02
0.031
0.231
0.357
0.568
0.031
0.018
0.69
0.084
0.072
0.142
0.033
0.234
0.037
0.073
0.072
2.235
0.074
0.083
0.015
0.259
932
2820
792
444
603
767
828
1245
492
719
709
580
730
2812
1366
1674
627
416
736
274
1151
1106
551
443
352
830
1439
276
577
833
516
1084
454
1240
951
939
195
851
871
2242
611
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
88
1445.01 4.6119
100
18
1446.01 2.2971 44429 235
1447.01 7.1143 148151 303
1447.02 5.7569 15260 205
1448.01 2.9237 44947
86
1449.01 3.8021 49724 929
1450.01 4.0904 18255 225
1451.01 5.5358 78850 1241
1452.01 2.3632 13235
76
1454.01 9.6294 11369
35
1459.01 1.0700
4809 116
1461.01 2.1651
5706
68
1463.01 11.9788 22843 1036
1465.01 1.6975
4866
61
1468.01 6.2072
1392
65
1472.01 6.5891
4430
93
1474.01 5.8511
4548 125
1475.01 1.5907
816
18
1475.02 3.0303
1197
15
1476.01 5.7031
2770
24
1477.01 8.3090 15017
84
1478.01 8.0856
3028 150
1480.01 3.9475
1498
26
1486.01 7.0829
8289
75
1486.02 5.4993
849
18
1488.01 1.6191
827
24
1489.01 3.8636
982
20
1494.01 2.9005
767
13
1495.01 5.0903
803
26
1498.01 3.9280
502
19
1499.01 4.2960
737
41
1501.01 2.1661
442
16
1502.01 1.5056
448
19
1503.01 10.8923
2445
36
1505.01 3.1205
450
14
1506.01 6.3551
850
19
1507.01 6.0774
639
17
1508.01 4.5912
735
15
1509.01 14.3572
650
64
1510.01 1.1235
509
19
1511.01 2.2855
360
23
68.682
66.78619
94.30528
66.63923
67.1094
70.1369
66.98404
92.74682
66.2764
70.3035
66.11011
73.7078
77.08517
68.5853
68.8407
94.0088
129.0525
111.9412
118.4738
155.2876
161.9327
132.4853
75.3196
96.8928
79.6407
67.6076
73.4823
69.6943
70.5618
71.7503
73.59
67.0247
66.1275
71.289
70.3243
72.5005
68.0439
69.4735
86.043
111.3478
66.2205
0.0065
7.16875
0.00037 1.2277586
0.00069
40.24666
0.0008
2.279999
0.0012
2.486588
0.00015 10.9802481
0.00057 2.1446308
0.00017 27.322068
0.0012 1.1522207
0.00031 121.59089
0.00041
0.692023
0.0011
7.946693
0.00018
253.0083
0.001
9.771425
0.0025
8.480842
0.0018
85.35029
0.0014
69.74538
0.0033
1.609323
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56.3647
0.0016
400
0.001
76.13333
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20.38139
0.0021
254.5598
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30.1839
0.0026
3.949663
0.0057
16.00474
0.0092
8.19571
0.0057
15.5947
0.0061
5.83375
0.0033
14.16394
0.0048
2.61709
0.0032
1.876417
0.0057
150.2421
0.007
5.03266
0.0081
40.4291
0.0094
21.36041
0.0085
22.04698
0.0043
49.6443
0.0025
0.839992
0.0036
2.578886
0.0002
12.62
0.0000019
4.6
0.00013
52
0.0000078
3.4
0.000013
8.24
0.0000072
22.25
0.0000052
4.5
0.000024 47.197
0.0000057
3.01
0.00017
60.88
0.0000013
3.4
0.000038
23.9
0.0055
188.3
0.000044
30.9
0.000093
10.89
0.00072 104.42
0.00075
149.2
0.000024
7.5
0.00025
24.8
0.0024
80.6
- 315.54302
0.00047
75.54
0.0004
41.2
0.003 206.4403
0.0012
43.3
0.000044 20.809
0.00042
32.5
0.00026
17
0.00037
24.32
0.00016
11.59
0.00019
21
0.000053
8.9
0.000025
10.2
0.005
110
0.00015
13.09
0.0015
50.8
0.00093
27.6
0.00079 38.888
0.001
26.97
0.00001
7
0.000039
9.04
0.49
1.4
16
1
0.13
0.31
1.4
0.066
0.9
0.21
1
7.2
2.5
9.3
0.12
0.89
1.4
2.3
1.5
2.7
0.34
1.4
0.0024
1.8
0.089
1.4
162
0.74
0.46
66
2.7
0.48
2.2
0.63
1.9
1.2
0.0057
0.24
21
0.36
0.00943
0.19414
0.55
0.10971
0.1899
0.228
0.1201
0.25125
0.1211
0.10541
0.0754
0.073
0.13679
0.0728
0.03339
0.05905
0.06164
0.0259
0.0317
0.0467
0.12163
0.04886
0.03472
0.09359
0.0263
0.0273
0.02796
0.028
0.02528
0.02101
0.026
0.01899
0.02283
0.04384
0.02214
0.02622
0.02269
0.03
0.0226
0.028
0.01828
0.00033
0.00096
0.27
0.00048
0.0021
0.0011
0.00052
0.00024
0.0021
0.00026
0.001
0.001
0.00042
0.0014
0.00034
0.00044
0.00046
0.0013
0.0015
0.0013
0.00022
0.00094
0.00098
0.00075
0.00095
0.054
0.00066
0.00071
0.016
0.00098
0.0008
0.00077
0.00087
0.00088
0.00087
0.53
0.00022
0.018
0.00056
0.027
0.168
0.97
0.025
0.739
0.0072
0.67
0.824
0.72
0.43
0.22
0.66
0.019
0.03
0.001
0.106
0.006
0.001
0.7224
0.002
0
0.7941
0.038
0.0355
0.028
0.7
0.024
0.0229
0.6
0.103
0.0573
0.001
0.074
0.019
0.023
0.022
0.02
0.2
0.0019
0.01
0.05
0.29
0.028
0.092
0.2
0.039
0.22
0.13
0.13
0.2
0.02
0.022
0.028
0.032
0.01
0.01
0.017
0.014
0.025
0.048
2.7
0.037
1.7
0.031
0.059
0.014
0.01
0.014
0.017
2
-
1.2
22.7
69.3
13.8
23.5
24.9
17.7
17.5
22.0
9.2
6.9
5.1
16.3
4.9
3.7
3.6
11.3
1.8
2.2
4.6
9.4
3.7
2.5
8.5
2.4
2.6
2.4
2.4
2.6
1.8
3.0
1.7
1.9
2.7
2.2
2.3
2.3
1.6
3.2
1.8
1.6
0.076
0.023
0.239
0.035
0.037
0.099
0.034
0.174
0.023
0.487
0.013
0.071
0.795
0.089
0.083
0.37
0.356
0.022
0.073
0.286
1.044
0.348
0.138
0.796
0.192
0.048
0.12
0.073
0.124
0.064
0.115
0.035
0.029
0.535
0.058
0.232
0.154
0.152
0.276
0.016
0.037
1099
1790
594
1553
1383
801
1663
459
2562
327
1435
625
311
653
873
295
622
969
532
413
195
341
475
256
521
941
564
659
693
917
708
1003
1131
242
999
462
634
483
580
1275
1150
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
89
1512.01 2.0692
1515.01 1.5355
1516.01 5.1817
1517.01 6.0046
1518.01 5.2245
1519.01 2.2369
1520.01 3.2262
1521.01 4.0344
1522.01 5.0713
1523.01 5.3847
1525.01 4.4884
1526.01 3.0765
1527.01 5.6836
1528.01 1.5604
1529.01 3.5244
1530.01 3.5406
1531.01 2.3874
1532.01 4.9255
1533.01 3.0841
1534.01 5.9455
1535.01 6.6899
1536.01 2.9231
1537.01 6.1963
1539.01 4.1246
1540.01 2.9953
1541.01 3.2386
1543.01 4.7888
1546.01 1.7236
1548.01 2.1552
1549.01 3.7446
1553.01 6.6202
1557.01 1.9833
1560.01 2.7667
1561.01 2.0755
1564.01 5.3239
1569.01 2.7366
1573.01 3.4077
1574.01 11.5744
1576.01 2.7055
1577.01 1.7039
1581.01 10.6245
701
331
676
1010
554
349
542
594
569
260
219
200
1117
211
301
260
171
208
155
170
379
65
64
72512
48706
49845
27498
12880
5437
12205
5978
1794
4350
2226
3166
1192
1891
4848
840
558
629
19
70.867
25
67.7191
22
72.5445
37
84.8066
17
84.8435
11
66.8256
21
71.162
17
89.1984
20
81.9293
15
68.8682
22
66.5555
10
66.4632
18
95.8719
17
67.0984
15
80.7485
20
72.7821
20
69.5839
18
80.4987
16
67.8854
16
79.9832
18 121.5617
13
66.5632
14
69.678
205
66.8696
207 111.21359
549
66.6509
349 69.02882
105
66.9341
114 68.06092
254 67.22398
78
89.3039
54
66.9645
95
91.2984
34
115.081
70
82.2007
21
76.0275
63
89.521
134
98.1547
37
76.0467
13
66.7309
15
70.537
0.0039
0.0025
0.006
0.0041
0.008
0.0067
0.0048
0.0074
0.0074
0.01
0.0058
0.0094
0.008
0.0035
0.0074
0.0048
0.0042
0.0085
0.006
0.0099
0.0078
0.0071
0.012
0.00064
0.00049
0.00021
0.00042
0.00064
0.00069
0.00053
0.0022
0.0014
0.0011
0.002
0.0022
0.0042
0.0015
0.0021
0.0022
0.005
0.017
9.04184
1.937029
20.55453
40.06897
27.50658
5.1445
18.45865
25.94116
33.3857
8.47997
7.71467
4.44448
192.674
3.989558
17.97619
12.98486
5.69927
18.11417
6.24151
20.42238
70.699
3.74438
10.19201
2.8194478
1.2078522
2.37928
3.9643332
0.9175586
2.1393302
29.481036
52.75935
3.295711
31.56915
9.085928
53.44931
13.75242
24.80762
114.7316
10.41565
2.806213
29.5511
0.00015
25
0.000021
9.96
0.00052
31
0.00076
53.1
0.00096
29
0.00015
17
0.00037
40
0.00083
49
0.0011
52.6
0.00038
7
0.00019
12.78
0.00017
12.62
0.011
222
0.000057
21.7
0.00056
36
0.00028
16
0.0001
18
0.00067
17
0.00016
15
0.00086
16
0.0029
66
0.00011
10.32
0.00049
12.83
0.0000078
5.63
0.0000029
3.8
0.0000021 6.760957
0.000007
7.3
0.0000026
4.14
0.0000063
8.1
0.000071
36
0.00051
65.33
0.000019
13
0.00016
39
0.000088
19.1
0.00052
80.68
0.00026
41.4
0.00017
61.33
0.001
80.46
0.00011
29
0.00006
11.2
0.0022
16
167
0.4
237
1.1
158
127
328
559
2.1
28
0.4
0.87
705
1.3
320
70
103
70
99
65
314
0.47
0.34
0.25
1.1
0.000011
0.021
0.042
2.4
11
0.67
58
12
5.7
0.97
2
0.92
0.4
163
3.4
60
0.028
0.01774
0.024
0.02823
0.023
0.019
0.022
0.022
0.02135
0.019
0.01394
0.01487
0.034
0.01431
0.017
0.017
0.012
0.015
0.012
0.014
0.019
0.00854
0.00785
0.2574
0.1971
0.2
0.14827
0.10122
0.06561
0.26867
0.06878
0.039
0.24781
0.0521
0.05007
0.0314
0.03919
0.06184
0.026
0.022
0.025
0.037
0.00056
0.037
0.00051
0.025
0.03
0.036
0.052
0.00072
0.013
0.00037
0.00086
0.021
0.00079
0.03
0.014
0.014
0.011
0.016
0.01
0.018
0.00036
0.0003
0.0036
0.0011
0.013
0.00032
0.00077
0.0006
0.00068
0.0006
0.035
0.00089
0.0016
0.0005
0.0012
0.00046
0.0003
0.03
0.0015
0.018
0.7
0.014
0.1
0.029
0.7
0.4
0.4
0.3
0.023
0.8
0.006
0.0388
0.8
0.0163
0.5
0.8
0.2
0.8
0.3
0.8
0.6
0.0514
0.029
0.53
0.0001
0.0016
0.026
1.24
0
0.4
1.35
0.78
0.0032
0.025
0.021
0
0.3
0.252
0.7
2.1
0.044
3.3
0.036
2
3
3.1
3.8
0.042
1.4
0.032
1.3
3.1
1.4
2.8
1.5
2.9
1.4
2
0.01
0.21
0.022
0.37
0.022
2.3
0.41
0.23
0.053
0.025
0.022
2.7
0.076
1 .7
2.1
1.3
2.3
3.3
2.2
1.5
2.1
2.4
2.5
2.2
2.1
1.3
4.9
0.8
1.7
2.0
1.4
2.0
1.4
1 .6
2.4
1.0
1.0
32.7
19.3
20.6
14.9
5.8
4.9
32.8
7.1
5.2
29.6
5.6
3.1
2.5
3.8
5.8
3.2
1.5
2.3
0.082
0.025
0.151
0.235
0.18
0.056
0.136
0.168
0.207
0.082
0.081
0.054
0.67
0.046
0.138
0.112
0.064
0.141
0.069
0.152
0.347
0.049
0.094
0.04
0.022
0.036
0.05
0.018
0.029
0.189
0.282
0.043
0.2
0.087
0.275
0.103
0.17
0.465
0.095
0.032
0.186
652
927
656
544
541
785
597
532
562
835
1214
1003
337
746
699
819
1049
816
1062
730
485
1209
922
1313
1516
1394
1102
1309
986
579
481
1123
580
836
360
543
589
331
828
810
499
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
90
1582.01
1583.01
1584.01
1585.01
1586.01
1587.01
1588.01
1589.01
1589.02
1590.01
1590.02
1591.01
1593.01
1595.01
1596.01
1596.02
1597.01
1598.01
1599.01
1601.01
1602.01
1603.01
1605.01
1606.01
1608.01
1609.01
4.7382
4.5321
2.3611
4.9613
2.0622
3.1788
1.5328
4.2548
4.0724
3.6462
1.5004
2.4255
2.6164
5.1212
2.7169
4.3349
4.6377
5.6905
4.8627
6.2071
5.8532
2.7672
1.4484
1.9798
4.4061
5.4671
3809
482
553
833
607
4196
499
440
456
779
331
829
600
786
390
1185
342
1120
484
286
263
194
361
241
206
376
47
18
14
21
25
35
20
22
19
13
11
17
12
21
17
16
31
37
17
20
12
20
17
18
17
20
79.9795
70.2059
70.2416
72.7384
68.4635
92.0623
68.5461
71.7748
68.2065
134.2278
110.8828
73.2918
115.4672
75.0828
67.6846
71.6868
67.42
76.8112
72.9972
66.7171
70.223
66.485
68.0478
66.2173
71.7175
102.5701
0.0025
0.0072
0.0061
0.0065
0.003
0.003
0.003
0.0064
0.0061
0.0062
0.0051
0.0051
0.0075
0.007
0.0053
0.0073
0.0042
0.0039
0.0075
0.0079
0.013
0.0046
0.0035
0.004
0.0074
0.0077
186.3827
8.04725
5.87084
19.1797
6.991262
52.97102
3.517485
8.72548
12.88195
25.78004
2.355804
19.65703
9.69448
40.1088
5.9236
105.3551
7.79663
56.4754
20.42116
10.35066
9.97788
3.02153
4.939157
5.082573
9.1759
41.6984
0.0019
210
0.00025
13.64
0.00015
23.3
0.0006
30.7
0.000091
20
0.00077
68
0.000045 19.21441
0.00024
16.32
0.00033
24.9
0.00084
34
0.000058
13.15
0.00044
67.4
0.00035
18
0.0012
41
0.00013
12
0.0039
205
0.00014
13.1
0.0011
78.7
0.00068
19
0.00036
11
0.00058
8
0.000059
5
0.000074
16
0.000087
18.52
0.00028
15.85
0.0015
31
63
0.58
1.5
0.47
125
20
0.00025
0.57
1
106
0.92
4
152
158
65
2218
0.31
1.6
56
54
42
21
1
0.14
0.66
74
0.0636
0.01984
0.0248
0.02583
0.024
0.0795
0
0.01933
0.01983
0.029
0.0198
0.027
0.026
0.028
0.021
0.032
0.01668
0.02968
0.023
0.016
0.018
0.016
0.01413
0.0131
0.01344
0.0206
0.0012
0.00072
0.0011
0.0008
0.03
0.0067
1.8
0.00058
0.00068
0.017
0.001
0.0013
0.041
0.021
0.022
0.071
0.00035
0.00055
0.013
0.016
0.017
0.013
0.00073
0.00066
0.00049
0.009
0.64
0.03
0.0676
0.062
0.7
0.88
0.0582
0.017
0.011
0.8
0.0393
0.029
0.8
0.7
0.7
0.5
0.019
0.002
0.8
0.5
0.8
0.8
0.017
0.2899
0.047
0.86
0.19
0.01
0.014
2.2
0.26
0.01
0.01
1.3
0.01
2.2
1.5
1.9
3.5
0.032
0.025
1.2
2.2
1.7
1.4
0.053
0.01
0.95
4.5
1.8
1.9
2.2
1.7
7.4
1.5
2.2
2.3
2.8
1.9
1.5
2.5
2.9
2.3
3.5
2.1
3.0
2.5
1.5
1.7
1.4
1.8
1.2
1.6
2.3
0.626
0.079
0.054
0.14
0.066
0.269
0.037
0.085
0.11
0.163
0.033
0.134
0.09
0.233
0.061
0.416
0.08
0.292
0.149
0.093
0.092
0.042
0.058
0.058
0.089
0.243
240
797
667
573
647
393
751
895
787
494
1098
434
794
502
825
316
1043
437
636
726
757
1146
1126
908
943
551
-
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
4
91
92
Table 3.
Notes to table of Planet Candidate Characteristics
Key:
APO
Active pixel offset. The pixel that actually dims during a transit is offset from the position of the target
star implying a background variable star.
Double star There is within 4 an object evident in images that has not been ruled out as the source of the transit.
V-shaped
The transit light curve is V shaped, a possible indication of an eclipsing binary
Odd-even Transit depths are alternately deeper and shallower, an indication of an eclipsing binary
Occultation Evidence of secondary eclipse, implying possible EB or self luminous planet
SB1
Spectroscopic binary. RV varies by over 1 km/s in low SNR reconnaissance spectra. Double lines not seen.
SB2
Spectroscopic binary. Double lines seen in spectrum.
KOI
Note
1.01
2.01
3.01
4.01
5.01
7.01
10.01
12.01
13.01
17.01
18.01
44.01
51.01
63.01
64.01
69.01
72.01
97.01
99.01
100.01
102.01
112.01
117.02
117.03
119.01
131.01
135.01
144.01
151.01
155.01
157.01
157.02
157.03
TrES-2; O'Donovan et al. 2006 ApJ 650 L61
HAT-P-7b; Kashyap et al. 2008 ApJ 687 1339
HAT-P-11b; Dittman et al. 2009 ApJ 699 L48
Rapid rotator Vrot = 40 km/s
Double star; 0.16 NE; delta_m=3.1 at 692 nm
Kepler-4b; Borucki et al. 2010 ApJ 713 L126
Kepler-8b; Jenkins et al. 2010 ApJ 724 1108
Marginally saturated
Double star; 0.8 E; delta_m=0.4 mag at 692 nm
Kepler-6b; Dunham et al. 2010 ApJ 713 L136
Kepler-5b; Koch et al. 2010 ApJ 713 L131
Variable transit depths
Light curve has spot/rotation modulation
Radial velocity variations have a dispersion 23 m/s
May be an F-M binary
Saturated. Double star; 0.05 NW; delta_mag=1.4 mag
Kepler-10b; Batalha et al. 2011 ApJ accepted
Kepler-7b; Latham et al. 2010 ApJ 713 L140
Double star; 4 SE
Rapid rotator; Vrot=35 km/s
Double star; 2.5 SW
Double star; 0.09; delta_m = 2.7 at 692 nm
Possible APO
Possible APO
Possible SB1
Possible APO
Centroid analysis clean
KIC radius likely overestimated
V-shaped; may be triple system
Double star; 2 W
Kepler-11b; Lissauer et al. 2011 Nature accepted
Kepler-11c; Lissauer et al. 2011 Nature accepted
Kepler-11d; Lissauer et al. 2011 Nature accepted
93
157.04
157.05
157.06
179.01
180.01
184.01
191.01
191.02
208.01
225.01
226.01
254.01
256.01
258.01
263.01
268.01
271.02
274.01
284.01
340.01
377.01
377.02
377.03
531.01
607.01
687.01
741.01
774.01
961.01
962.01
968.01
972.01
973.01
976.01
977.01
978.01
981.01
984.01
992.01
993.01
994.01
998.01
1063.01
Kepler-11e; Lissauer et al. 2011 Nature accepted
Kepler-11f; Lissauer et al. 2011 Nature accepted
Kepler-11g; Lissauer et al. 2011 Nature accepted
Double Star; 4 E
Variable star
Odd-even
Double star; 1 E
Possible APO; Double star 1 E
Variable star with possible spots
Possible ellipsoidal variations
Possible APO
5% primary transit
KIC stellar radius may be too large
V-shaped; Multiple stars 1 and 2 E
Double star; 4 E
Multiple Stars: 2 S and 3 SE
Possible Odd-even
Possible APO
Double star; 0.9 E
Radius large; but log g may be too low in the KIC
Kepler-9b; Holman et al. 2010 Science 330 51
Kepler-9c; Holman et al. 2010 Science 330 51
Kepler-9d; Torres et al. 2010 arXiv:1008.4393
Strange light curve; worth follow-up.
Odd light curve; worth follow-up.
Varying depths; possible encroaching companion.
Slight V shape and deep; no APO.
Possible occultation
Short duration, under sampled transit
Weak transit signal; possible low radius planet
Not convincing transit
Pulsating star
Possible APO; poor light curve
V-shaped; poor fit
Phase-correlated variations; saturated
Possibly spurious
V-shaped; saturated
V-shaped
Poor fit to light curve
Possible APO
Possible APO
Eccentric eclipsing binary
V-shaped; large planet radius (2.1 RJ)
94
Table 4
Very Probable False Positives
Key:
t0
Period
APO
Time of a transit center based a linear fit to all observed transits and its uncertainty
Average interval between transits based on a linear fit to all observed transits and uncertainty
Active pixel offset. The pixel that actually dims during a transit is offset from the position of the target
star implying a background variable star.
Double star There is within 4 an object evident in images that has not been ruled out as the source of the transit.
V-shaped
The transit light curve is V shaped, a possible indication of an eclipsing binary
Odd-even Transit depths are alternately deeper and shallower, an indication of an eclipsing binary
Occultation Evidence of secondary eclipse, implying possible EB or self luminous planet
SB1
Single-line eclipsing binary star. RV varies by over 1 km/s in low SNR reconnaissance spectra. Double
lines not seen.
SB2
Double-line eclipsing binary Double lines seen in spectrum.
KOI
Kepler ID
t0
(BJD2454900)
Period
(days)
Depth
(ppm)
SNR
Comment
6.01
8.01
9.01
11.01
14.01
3248033
5903312
11553706
11913073
7684873
66.69954
54.70223
68.06724
104.65803
104.53055
1.334103
1.160154
3.719813
3.748075
2.947317
397
399
3423
547
302
97
41
380
65
59
15.01
16.01
19.01
21.01
23.01
3964562
9110357
7255336
10125352
9071386
68.25804
66.40566
66.93003
54.97329
69.86191
3.012481
0.895298
1.203197
4.288459
4.693309
1599
1527
2472
3127
14756
301
283
92
246
1443
24.01
25.01
26.01
27.01
28.01
31.01
33.01
43.01
45.01
48.01
52.01
53.01
61.01
66.01
68.01
4743513
10593759
5021737
3832716
4247791
6956014
5725087
9025922
3742855
7837302
3558981
2445975
8248939
10620329
8669092
103.98992
69.00948
77.1360
103.33754
101.14347
102.7
66.55824
110.08114
107.36379
106.7648
101.0114
105.26025
114.8623
103.68382
1.63959
2.086268
3.132604
15.03952
1.141879
4.100902
0.925516
0.366201
11.320908
6.397234
23.836924
2.987841
3.388834
1.633372
1.308783
1.000977
10806
7879
~10000
291300
111224
742
356
2518
18199
27844
46738
8807
623
691
2518
421
122
168
189
97
26
52
39
287
1008
127
55
16
206
53
74.01
76.01
6889235
9955262
58.87577
87.75975
5.188712
77.451216
790
914
50
27
APO Binary
APO Binary
APO Binary
APO Binary
Rapid rotator; Vrot = 90 km/s;
Secondary eclipse
APO Binary
APO Binary
Binary, Odd-even
Binary
SB1; 18 km/s radial velocity amplitude;
secondary eclipse in light curve
APO Binary
Binary
Binary
Multiple stellar eclipses
Multiple stellar eclipses
Binary
Probable binary star (Per=0.2 d)
APO Binary
APO Binary
Binary
Binary
APO Binary
APO Binary
Binary
Double star: 0.83arcsec SE; delta_m=2.7
mag at 692 nm; Light curve shows
modulation in phase with the transit.
Binary
Saturated star; Variable star
95
80.01
81.01
88.01
90.01
106.01
109.01
114.01
120.01
121.01
125.01
126.01
129.01
130.01
132.01
133.01
134.01
136.01
140.01
143.01
145.01
146.01
147.01
154.01
158.01
160.01
164.01
169.01
170.01
175.01
9552608
8823868
7700871
9210823
10489525
4752451
6721123
11869052
3247396
11449844
5897826
11974540
5297298
8892910
11673674
9032900
7601633
5130369
4649305
9904059
9048161
1996679
9970525
10555375
6631721
5652237
6185711
11044770
8323753
68.41332
76.07155
66.88714
68.72067
64.86603
65.86384
65.26635
70.89987
69.45725
84.85057
135.33287
65.88433
88.29605
65.95236
66.38896
86.18499
80.39962
70.17318
73.33962
91.0779
70.34138
79.05365
72.72903
70.57828
67.43403
65.31493
84.13743
77.29725
67.31485
9.250714
23.875999
2.589751
0.828212
1.612021
6.4149
7.360901
20.546581
8.810982
38.479316
33.77925
24.666561
34.193562
10.810049
4.618688
67.179946
15.66349
19.979085
22.650871
45.002812
8.667811
20
30
5.801762
13.738118
4.464747
11.700984
15.608935
6.714228
988
1640
236
240
240
414
297
1860
389
23913
17432
4378
14449
5811
6661
5056
5055
1132
2388
1612
4611
2697
1078
527
625
202
537
233
457
193
37
70
50
45
61
11
141
52
284
1050
171
1123
366
542
167
128
59
141
20
407
22
57
55
39
20
31
22
49
178.01
181.01
182.01
11455491
12504988
5376836
68.159
72.71686
69.79714
6.143084
5.093946
3.479294
179
26156
19156
28
1050
205
184.01
185.01
198.01
210.01
213.01
215.01
218.01
224.01
230.01
231.01
233.01
236.01
243.01
259.01
7972785
4178389
10666242
10602291
9164836
12508335
9838975
5547480
3862246
4043443
5023956
8453211
9592579
5790807
66.56668
67.38638
86.36912
72.32516
103.83962
88.20608
76.83238
65.07193
69.3061
95
80.48307
76.0925
67.21109
140.12541
7.300705
23.210439
87.233068
20.927351
48.118647
42.943545
18.692915
3.979789
4.70253
119.7
1.824639
5.776826
2.637587
79.996026
13378
29037
20687
8264
78601
9709
56736
1016
4069
6424
8311
3961
5743
24236
864
792
403
276
1240
158
648
51
90
60
685
323
359
667
SB1: V-shaped; Secondary eclipse
Binary
APO Binary
APO Binary
APO Binary 12arcsec S
APO Binary
APO Binary
Binary
APO Binary 1.2arcsec SW
SB1
Hierarchical triple
Binary
SB1
Binary
APO Binary
SB1
SB1; V-shaped
APO Binary 6arcsec N
SB1
Binary
APO Binary
APO Binary
APO Binary
APO Binary
APO Binary 4arcsec N; Odd-even
APO Binary
APO Binary
APO Binary
APO Binary 8arcsec NE; 3% transit on
nearby KIC 8323764
APO Binary MAST FP
Binary
SB1: secondary eclipse; 30 km/s
variation RV variation
Binary Brown Dwarf Odd-even
Binary
SB1: V-shaped; 9 km/s RV variation
SB1: V-shaped; 10 km/s RV variation
SB1
V-shaped Double star: 2arcsec N
Binary
APO Binary 4arcsec S
Binary
Binary
APO Binary
APO Binary
APO Binary
Binary
96
264.01
266.01
267.01
272.01
286.01
287.01
290.01
293.01
300.01
309.01
3097346
7375348
8167959
5716763
8258171
8703887
10488450
11200415
3438975
7024222
103.6909
104.51168
140.33404
102.6666
106.63073
108.60714
104.42464
105.21434
104.66069
103.19735
4.029783
25.308485
170.564783
1.281318
23.631011
14.170948
2.683386
4.639598
2.976105
1.633091
177
133
118
490
126
9409
327
144
111
64
61
26
9.2
101
28
268
53
31
28
12
311.01
320.01
322.01
324.01
325.01
328.01
7024511
8700558
8948424
9641041
9724984
9895004
108.64811
106.51072
106.58265
104.2285
104.00304
103.32188
66.155811
4.791957
5.888834
1.089083
7.863267
2.250817
3579
137
15417
139
449
545
30
32
110
62
45
49
329.01
334.01
336.01
347.01
358.01
359.01
362.01
363.01
376.01
376.02
378.01
380.01
381.01
10031885
10383687
10518725
11189127
12017140
12106929
1571511
2438070
12643589
12643589
2449074
2452450
3230578
107.94672
109.93541
108.25221
102.85301
105.8018
104.5856
110.5945
104.0968
144.53871
111.26218
106.75081
103.8115
103.18917
8.590949
8.487801
19.506989
2.671944
22.845232
5.936699
14.022451
2.442946
220.7246
1.411632
4.943872
8.09694
6.337653
113
363
173
15250
46728
348
20957
989
3856
513
928
1108
1734
14
27
12
142
2495
24
2270
130
50
36
57
109
99
382.01
389.01
390.01
391.01
394.01
395.01
396.01
397.01
399.01
400.01
402.01
404.01
405.01
406.01
407.01
411.01
3231137
3847708
3849155
3858804
4159347
4165960
4252322
4376644
7289157
2695110
3342592
4949751
5003117
5035972
5218441
5478055
105.36798
104.70781
103.60189
107.83701
107.35772
104.01164
113.84957
106.79527
106.82975
142.98685
103.54579
119.38611
123.6832
124.18974
104.42236
107.23072
3.900201
3.741174
1.168317
25.958842
12.28406
6.774472
14.591555
27.67775
5.266478
44.190443
17.17733
31.805916
37.617744
49.266722
3.613743
15.851644
883
862
308
405
511
548
1296
8384
72027
4005
24757
3360
29139
8503
5160
721
85
86
40
31
27
38
50
386
523
63
972
107
1119
215
362
21
APO Binary SB1; 10arcsec E
APO Binary 2arcsec NW
Spurious Detection Light curve artifact
APO Binary
Binary; V-shaped, secondary eclipse
APO: 8arcsec NE
APO Binary
APO: 8arcsec W
APO: 2arcsec S
APO: 8arcsec NE, V-shaped, Secondary
eclipse possibly on nearby KIC 7024229
APO Binary
Binary
Binary
Binary
Binary
APO: 3arcsec S, Double star: 2" S,
delta_mag > 5 mag at I filter
APO: 8arcsec E
APO Binary
APO Binary
Binary
Binary
APO: 10arcsec S
Binary
Binary
Binary
Binary; deep transit
APO Binary
APO Binary
SB1: 90 km/s RV variation, secondary
eclipse
APO Binary
APO
APO: 3arcsec S
APO: 7arcsec E
APO: 2arcsec S
APO: 4arcsec S
Binary
SB2
SB2, V-shaped, Secondary eclipse
APO
Binary
APO Binary
Binary
Binary
Binary
APO Binary
97
414.01
5872150
108.3429
20.355117
27585
1154
414.02
5872150
106.82314
5.922128
366
19
424.01
434.01
9597411
11656302
103.39252
106.10122
1.575632
22.265052
24382
19044
482
783
436.01
437.01
441.01
445.01
447.01
449.01
450.01
451.01
453.01
455.01
461.01
462.01
482.01
485.01
489.01
491.01
493.01
495.01
498.01
502.01
514.01
515.01
516.01
527.01
529.01
539.01
540.01
11805075
11824222
3340312
4384675
5021176
5779852
6042214
6200715
6758917
7101828
8621348
8773869
11255761
12316431
2576197
3541800
3834360
4049108
4833135
5282051
7602070
7812179
7840044
9636569
10068030
11246364
11521048
158.3578
110.1409
106.91384
191.3437
105.68099
173.23463
104.95475
105.18015
102.64822
126.20207
105.84204
103.88046
102.55198
108.55026
104.69565
102.66617
103.12284
102.63841
110.53567
104.15518
109.0658
102.60907
104.09574
104.68827
103.51226
104.24141
127.8248
200
15.84134
30.547936
200
4.045084
252.079331
27.046295
3.723577
2.23609
47.880541
11.344441
1.576334
4.992736
17.908864
2.217017
4.661868
2.908459
4.804379
8.660657
5.910368
11.756019
17.792292
13.542045
10.636614
2.023127
200
25.702616
32503
22106
632
4254
869
4341
1062
585
29399
923
916
839
771
1061
683
354
678
677
111
232
788
1310
607
330
1277
362
5252
327
139
18
33
51
73
37
39
58
24
44
132
38
46
42
22
39
39
7
19
36
54
32
24
48
8.3
54
544.01
545.01
549.01
549.02
553.01
556.01
565.01
570.01
576.01
591.01
595.01
603.01
604.01
606.01
11913012
11972666
3437776
3437776
5303551
5738496
7025846
8106610
8474898
9886221
10294465
2441151
3970233
5014753
104.66417
103.37698
126.50951
66.41894
104.45359
108.65576
103.19693
105.78106
173.84915
103.79579
183.93512
104.6703
107.4336
105.04683
3.747895
1.091763
42.899607
0.635578
2.399009
9.503451
2.340506
12.398394
199.444158
2.992808
200
2.19201
8.254955
3.170623
389
195
758
407
326
437
181
583
5745
140
4037
1490
20142
14181
27
16
13
63
20
17
22
24
82
10
40
105
662
140
SB1: 20 km/s RV variation, Possible
Odd-even, Possible secondary eclipse
SB1: 20 km/s RV variation, Possible
Odd-even, Possible secondary eclipse
Binary
Transit depth too deep, Double star: 3"
SE at J
Binary; deep transit depth
Binary
APO: 2arcsec S
Partial Single Transit
Binary
Binary
APO: 4arcsec NE
APO: 8arcsec W
Binary
APO Binary
Binary
APO Binary
APO:4arcsec ESE
APO
APO
APO: 8 arcsec S
APO: 4 arcsec SE
APO: 12 arcsec E
Spurious Detection
APO: 10 arcsec S
APO: 8 arcsec SE, transit depth changes
APO Binary
APO
APO Binary
Binary
Spurious Detection
APO: 4 arcsec NW, V-shaped, Oddeven
APO: 10 arcsec NE
APO: 10 arcsec E
APO
APO
APO: 6 arcsec S
Binary
APO: 8 arcsec N
APO: 8 arcsec S
APO: 8 arcsec W
APO
Spurious Detection
APO Binary
Binary
Binary
98
608.01
613.01
615.01
616.01
619.01
621.01
630.01
631.01
634.01
636.01
637.01
642.01
643.01
646.01
648.01
5562784
6960456
8374580
9714696
10384962
12251650
4659405
4742414
4861736
5090690
5098444
5181817
5309353
5384802
5596440
125.90668
104.55631
125.50459
102.84973
103.7099
107.18212
104.92727
106.78138
105.57831
109.63508
110.97822
104.43335
102.73079
103.49023
105.11995
25.337283
5.074714
176.239818
1.433356
2.879242
17.762041
4.532367
15.458069
6.277803
12.011655
26.948407
4.350379
1.376372
3.041456
10.474877
2035
566
6046
415
49699
22623
425
4358
1838
13445
16053
183
309
19146
2184
74
23
100
28
232
466
41
693
162
1336
162
20
26
1237
81
651.01
653.01
656.01
668.01
669.01
675.01
677.01
681.01
690.01
696.01
699.01
702.01
705.01
706.01
713.01
715.01
724.01
726.01
727.01
729.01
731.01
742.01
744.01
748.01
754.01
761.01
768.01
770.01
789.01
792.01
793.01
796.01
5796186
5893123
5966660
6805146
6960445
7385509
7466863
7598128
8409588
8869680
8908102
9053112
9300285
9426071
9640985
9834719
10005020
10157573
10191070
10225800
10259031
10419211
10480982
10583180
10848459
11152159
11442465
11463211
12459725
2440757
2445129
3114661
137.12803
102.632
103.06339
111.68746
104.56468
102.54614
104.07983
121.49531
102.70818
107.15636
107.60562
102.867
103.18743
115.60821
104.22897
103.35853
107.70358
106.26507
103.58189
102.67394
102.86523
103.83978
117.55132
103.73521
103.3066
103.69418
119.67371
103.9971
104.49591
103.40219
106.31213
102.86259
42.559655
1.125969
1.906628
13.7797
5.074351
1.655473
11.971853
44.258089
1.360839
7.033951
5.414584
1.27484
1.012676
28.714155
2.178174
1.621665
6.970892
5.11578
1.213737
1.423802
7.061031
11.52139
19.221399
2.696436
1.736957
2.701326
33.93387
1.506357
14.180511
1.433833
10.318845
1.332894
2070
144
530
26160
933
1999
454
20356
1361
105
4914
359
1190
43504
410
6413
477
960
1772
2091
3608
17206
72570
383
7825
1176
8042
2287
462
1890
704
12019
82
24
110
2903
88
139
17
1032
119
20
172
82
146
1755
56
56
25
39
130
91
99
446
1554
25
331
39
170
109
7.4
75
21
87
APO
APO Binary
APO: 3 arcsec SW
Binary
Binary
Binary
APO Binary
SB1
APO Binary
SB1
SB2
APO Binary
SB2
Hierarchical triple
Secondary eclipse; radius 7 Rjup - too
large.
APO Binary
APO: 8 arcsec SW
APO Binary
Binary
APO Binary
APO: 6 arcsec W; V-shaped
APO: 4 arcsec
SB1
Binary
APO
SB1; V-shaped
APO Binary
APO Binary
Binary
Binary
SB2
APO Binary
APO: 4 arcsec E
APO Binary
APO: 2 arcsec N
APO Binary
Binary
Binary
Binary
Binary
APO: 6 arcsec NE
APO
APO: 3 arcsec NE
APO: 10 arcsec E
Binary
APO
APO: 10 arcsec S
99
798.01
803.01
807.01
808.01
819.01
820.01
3120431
3554600
3836375
3838486
4932348
4936180
104.64252
104.78318
103.50377
104.98512
129.93326
106.72046
3.34192
7.546344
1.540409
2.990307
38.03697
4.640905
1045
382
1667
646
87384
4430
33
11
54
29
1478
103
828.01
831.01
832.01
836.01
839.01
848.01
859.01
862.01
866.01
888.01
894.01
909.01
915.01
919.01
925.01
927.01
930.01
932.01
933.01
946.01
948.01
950.01
957.01
958.01
959.01
964.01
965.01
967.01
968.01
970.01
971.01
978.01
980.01
982.01
983.01
985.01
5287983
5370302
5372966
5481416
5649215
6267425
6675056
6756669
6862603
7552344
7708215
8256049
8605074
8686150
9016295
9097120
9159275
9166870
9171801
9661877
9761882
9772531
7661409
1026957
10002261
10657664
3337351
6579806
3560301
11502218
11180361
11494130
12167361
1433962
11607193
10227501
104.00036
106.39528
104.82031
104.58344
103.67139
105.00138
108.40596
106.82149
104.64695
102.96884
107.5174
105.76151
127.71347
106.53537
104.62927
121.98166
105.00944
103.68018
104.6591
109.71686
106.70756
116.40765
111.46762
99.5413
108.07184
104.23836
108.0321
106.60816
194.28976
104.01865
104.2261
195.43461
112.0942
66.91651
199.05683
194.95809
2.507109
3.904278
9.286365
2.384036
2.4467
3.166479
10.443261
5.851534
2.861178
1.000786
7.943013
16.371955
37.601454
51.426011
19.974485
23.899733
3.044891
3.855545
3.185933
20.427268
24.586099
31.201504
3.140565
21.761045
12.713795
3.273699
7.047115
9.880483
4.649301
3.988635
0.533058
18.954856
47.931219
1.592683
7.15466
2.002925
1886
16419
46813
1269
3144
4834
859
35214
1298
1889
2911
9842
64858
71051
39181
21886
1431
1497
1094
2285
984
32363
1971
933
36851
7811
41819
17819
122
729
1237
471
1826
931
985
363
64
521
1422
24
209
124
23
1170
46
107
81
178
742
1213
762
428
103
89
13
58
21
396
120
8.9
957
58
452
299
42
28
102
100
137
58
18
20
989.01
989.02
990.01
995.01
10743597
10743597
10015516
3858949
117.30935
65.83445
71.53571
87.9233
81.192668
0.817026
67.684214
25.946596
14022
2431
23489
671
72
111
39
27
Binary
APO
APO: 12 arcsec SE
APO
Binary
Binary, V-shaped, Possible ellipsoidal
variations
APO
Binary
Binary
APO: 6 arcsec E, Odd-even
APO Binary
Binary
APO: 12 arcsec SE
Binary
Binary
Binary
APO Binary
APO Binary
Binary
Binary
Binary
APO Binary, V-shaped
APO Binary
APO
APO
APO Binary
APO: 6 arcsec W
Binary
Binary
Grazing EB
White Dwarf
Possible white dwarf
APO
Binary star
Spurious Detection
Occultation
Binary
Binary
Binary
5.5-sig odd-even
Spurious Detection
Spurious Detection Poor fit to light
curve
Planet radius too large
APO Binary
Planet radius too large
Secondary eclipse; eccentric
100
996.01
997.01
3858824
2157247
87.88238
66.01327
25.952109
5.686521
1733
4902
45
113
1000.01
1004.01
1006.01
1008.01
1009.01
1011.01
1012.01
1016.01
1018.01
1021.01
1023.01
1025.01
1028.01
1034.01
1035.01
1036.01
1037.01
1038.01
1039.01
1040.01
1041.01
1042.01
1043.01
1044.01
1045.01
1046.01
1047.01
1048.01
1049.01
1055.01
2441728
2309585
5738346
1722276
892772
5728283
8127639
8176653
8183911
2558363
2445154
2574201
2166206
5899544
5963222
5982353
6205468
6153201
5802486
5817553
5982368
5816811
5816165
5802246
6066403
6209637
5988031
5820218
5876368
5866099
66.6694
285.71837
307.63528
181.92435
290.53448
116.37238
287.8211
67.06724
70.07805
111.56191
72.67279
90.33265
73.73622
287.88718
66.32803
67.35396
112.30246
287.98492
110.92264
69.44957
302.11007
67.45204
288.35413
66.74212
67.21317
66.44315
67.4955
66.17894
66.18536
66.63221
0.856917
1.838472
30.607094
300
5.092371
6.198276
1.023438
2.866656
8.307384
0.546248
8.410946
37.475525
8.0974
1.739454
1.217267
19.563101
3.722924
0.530301
1.07392
4.206046
19.564094
2.227715
0.591908
0.525157
1.303856
0.734491
2.5555
3.411778
0.525428
36.976706
97
949
4889
31943
272
51074
1603
761
160
671
702
1555
425
11695
7546
12463
2947
2537
2365
1539
3526
1457
1091
962
439
342
329
588
329
1000
22
33
28
189
8.8
1568
57
26
12
29
25
17
30
76
486
1216
204
108
133
137
71
118
34
90
75
164
41
21
37
78
1056.01
1057.01
1058.01
1062.01
5964985
6066416
6124941
6147122
66.26465
67.20831
69.20124
75.21795
1.850845
1.303879
5.670144
15.450994
117
145
607
241
27
78
29
38
1063.01
8257407
109.30531
89.69815
266763
7754
1064.01
1065.01
1068.01
1071.01
1073.01
1075.01
1076.01
8218274
8242681
8264070
8244190
8262210
10232123
10223616
66.46468
66.63778
383.76246
66.18984
111.53907
66.27522
75.16079
1.187353
4.020627
2.897046
1.092087
1.612925
1.343764
29.122922
19234
21849
1148
220
152
4752
6778
310
257
30
28
13
168
102
Secondary eclipse; eccentric
APO Binary Contact binary; transit on
nearby object
APO
APO
APO
V-shaped Binary
APO
Secondary eclipse; eccentric
APO
APO
APO
APO
APO
APO
APO
APO
APO
40-sigma secondary eclipse
APO
APO Binary 23-sigma secondary eclipse
APO
APO Binary
APO
APO
13-sigma secondary eclipse; odd-even
APO Binary 48-sigma secondary eclipse
APO Binary 11-sigma odd-even
Contact binary
APO Binary V-shaped
APO
APO Binary 7.2-sigma odd-even
APO Binary Secondary Eclipse;
eccentric binary
Contact binary
APO Binary 6-sigma secondary eclipse
APO
APO Binary Secondary eclipse;
eccentric
V-shaped Binary V-shaped; large planet
radius (2.1 RJ)
Binary
Binary
APO
APO
Contact binary
Binary
Stellar binary - TTV
101
1077.01
1079.01
1080.01
1084.01
1087.01
1088.01
1090.01
1091.01
1092.01
1093.01
1097.01
1098.01
10268907
10153827
10158990
10148521
3124412
3113266
3232859
3098184
2720309
3239636
3340070
3240706
287.58283
66.58797
66.60619
67.05846
67.36639
66.34181
71.90254
302.53435
66.20765
66.3844
75.61968
67.1046
1.103981
0.293626
1.09661
1.204265
0.948955
1.493792
8.387211
15.243206
1.240024
0.528753
10.904413
5.489896
2351
831
257
218
3595
4881
5448
2244
1636
463
647
517
62
68
27
22
200
99
220
48
57
72
22
19
1100.01
1104.01
1105.01
1107.01
1119.01
1120.01
1121.01
1122.01
1123.01
1124.01
1125.01
1126.01
1130.01
1132.01
1133.01
1134.01
1134.02
1135.01
1136.01
1138.01
1139.01
1140.01
1143.01
1147.01
1153.01
1154.01
1155.01
1156.01
1157.01
1158.01
1167.01
1171.01
1172.01
1173.01
1178.01
3228824
2851100
3130300
3228959
3003992
6307537
6359798
6311681
6365321
6301035
6292162
6307521
8279765
8330548
8374494
8414907
8414907
8397446
8386035
8415745
8378634
8397675
8312852
8299955
10351767
10295951
10342041
10514770
10342065
10352945
10485179
10485069
10341913
10480921
3869825
288.9061
66.2646
66.31262
66.70972
72.09994
90.41441
73.69733
67.21665
66.58381
76.27948
290.51705
90.4045
68.23281
67.64426
290.32645
210.0594
389.85157
381.592
67.51314
299.70512
67.70132
66.44743
67.76284
67.25617
67.01944
69.04584
66.38725
67.36536
66.38704
289.38614
66.97753
66.52966
67.31822
66.616
67.36948
0.730941
0.890105
5.765791
0.730867
7.244998
29.744338
14.154037
0.844784
0.848485
11.991361
7.815272
29.743666
2.757787
1.91416
5.251691
200.611031
200.622704
0.986617
1.634815
31.827907
3.629444
0.553259
7.440416
2.682674
0.635073
6.810826
0.933744
1.872422
0.933747
6.471815
0.445263
0.445267
0.933753
2.037225
4.800633
240
426
378
212
72
161172
58683
2986
1856
1982
2065
585
37543
7236
6185
23227
12103
2226
948
4644
628
1146
592
132
36772
14832
2797
2964
1474
583
206
182
122
111
13791
13
15
22
14
21
451
441
189
116
75
45
25
362
122
151
188
109
69
82
51
90
120
23
21
273
713
469
112
377
26
42
21
55
16
132
APO Likely a blend
Contact binary
APO 4.7-sigma secondary
APO Binary 3.8-sigma secondary
APO Binary Blend; eccentric binary
APO
APO
APO Secondary eclipse; eccentric
APO Contact binary
APO 12-sigma odd/even
APO Binary
APO Binary Secondary eclipse;
eccentric
Contact binary
APO Binary Secondary eclipse
APO
Contact binary
APO
Stellar binary
Binary
APO Binary Stellar binary
Binary
APO
Secondary eclipse
APO
Secondary eclipse
APO
APO
APO
APO
APO
APO
APO
APO
Binary occultation
APO
APO
Binary
Binary occultation
APO
Binary occultation
Binary grazing binary
APO
APO
Binary contact binary
APO
APO
Binary phase linked variations
102
1179.01
1180.01
1181.01
1182.01
1183.01
1184.01
1185.01
1186.01
1188.01
1189.01
1190.01
1196.01
1197.01
1200.01
1211.01
1213.01
1217.01
1223.01
1224.01
1225.01
1228.01
1229.01
1231.01
1232.01
1233.01
1234.01
1235.01
1237.01
1243.01
1247.01
1248.01
1250.01
1251.01
1252.01
1253.01
1254.01
1256.01
1259.01
1260.01
1262.01
1263.01
1265.01
1267.01
1269.01
1272.01
1277.01
1280.01
1284.01
3655332
4042026
3344419
3865567
3544689
4037164
3443790
3966912
3860441
3765771
3557341
3348082
3853673
3557493
3858704
3556220
3542588
6613006
6606653
6620003
6387450
6432059
6462874
6665223
6545358
6390824
6546528
6531491
6677256
8801343
8488878
8620565
8616873
8737796
8462258
8454250
8848271
8823426
8766222
8703884
8560840
8552583
8519253
8757910
8552498
8552565
8509361
10960993
73.65674
96.01592
66.11162
66.09875
67.65783
67.18271
66.86259
89.34976
66.26721
66.22795
111.58633
68.5425
66.98158
66.3066
68.64523
66.08445
66.75171
66.93373
69.33242
66.31535
68.26916
66.29515
88.08445
165.64948
111.59514
66.49873
66.88287
297.38226
289.40143
67.54977
290.45296
67.02127
67.10443
67.48073
290.24997
70.25924
70.44893
111.18663
110.97695
292.82951
66.88154
66.84451
69.53055
66.17576
66.84806
66.84725
68.52649
66.12539
15.066423
34.820008
0.651782
11.116227
1.922868
0.635445
1.665782
55.659966
2.988155
2.783865
0.393729
3.981818
0.643798
0.393732
3.003592
0.796712
3.47124
7.388831
2.698025
1.714272
3.661328
0.769738
22.342917
238.814686
1.171542
0.973544
3.053602
14.325861
3.126045
2.739874
5.801871
0.782044
0.576082
0.885763
3.611524
5.082704
9.991579
1.506477
5.296678
14.170888
31.971634
1.061949
5.938123
0.655003
0.530968
1.061938
6.099026
1.558546
25123
18755
4689
5904
2214
2951
1707
2702
845
898
727
510
478
424
139
132
105
11651
7480
28197
17248
10490
3039
18640
1366
1442
459
772
261
22189
20730
14820
9222
4247
2157
2168
3415
739
997
2374
1074
407
834
382
201
161
225
8533
163
488
188
127
56
122
108
54
37
43
34
19
33
41
38
35
15
777
50
668
376
210
45
289
48
75
33
13
13
455
495
195
383
281
71
58
167
47
30
45
27
39
35
87
60
46
25
426
APO
Binary eccentric binary
APO
APO
APO
APO
Binary occultation
APO
APO
APO
Binary contact binary
APO
APO
Binary contact binary
APO
APO
APO
APO
Binary
Binary
Binary occultation
Binary occultation
APO
Binary (large radius)
APO
APO
APO
APO
APO
Binary (phased locked variations)
APO
APO
Binary
APO
APO
APO
APO
APO
APO
APO
Binary eccentric binary
APO
APO
APO
Binary 12 sigma odd-even
APO
APO
Binary
103
1286.01
1289.01
1290.01
1291.01
1292.01
1293.01
1294.01
1295.01
1296.01
1297.01
1313.01
1318.01
1319.01
1321.01
1322.01
1324.01
1326.01
1327.01
1330.01
1333.01
1334.01
1340.01
1343.01
1345.01
1346.01
1348.01
1349.01
1350.01
1352.01
1354.01
1365.01
1368.01
1371.01
1373.01
1374.01
1380.01
1381.01
1383.01
1384.01
1386.01
1388.01
1389.01
1390.01
1392.01
1394.01
1400.01
1414.01
1415.01
10879208
10748393
10874226
10661771
10924853
10874926
10549562
10666230
10971674
10676923
10785538
4070376
4078157
4480676
4079535
4551328
4639868
4372768
4150539
4285107
4150624
4386059
4570931
7284688
7199774
6866228
6847018
7220322
6956233
6891543
7174351
7357531
6878167
6863839
7296086
7025526
9451127
8953257
8971432
9143254
9346253
9002237
9288786
9040849
8937021
9157908
8916492
11193447
111.2802
287.53941
77.77651
66.0339
67.3941
66.72149
72.07875
66.30807
68.32449
66.9362
66.74787
66.96805
300.69473
67.22337
289.79691
66.1377
68.97114
292.04613
67.32308
66.44838
67.29188
112.84431
66.5491
66.6039
70.07146
70.56335
75.18696
67.04433
291.16441
67.47279
66.9749
163.02483
66.6844
66.7014
67.56837
66.84556
67.58585
69.14077
66.04537
66.80499
83.45355
67.79932
67.50781
290.25992
66.88839
75.33007
69.24279
66.80918
0.668484
4.88778
11.973776
1.231376
2.102421
11.703074
9.089494
1.577794
2.380863
1.031112
0.522466
1.634614
16.025273
0.711965
17.726895
0.522059
53.100926
15.642622
8.65258
2.24301
8.653379
2.900473
1.54492
0.32302
4.708125
7.702363
16.662103
0.752164
4.818807
1.752572
1.487105
251.059866
0.833971
1.926129
0.890732
1.074081
5.117403
3.221787
0.62438
1.137524
34.064261
4.350087
1.744101
4.118762
5.663653
9.414682
4.02365
0.312943
3332
3142
3485
980
1783
3999
1023
684
34583
384
184
19619
20671
6016
16147
1448
13485
1720
688
277
510
206
138
48165
52057
16949
22623
5591
3700
771
408
6255
216
185
218
65
64104
45922
38858
16933
28776
21642
9692
1838
2236
783
34
34162
126
26
78
129
78
88
64
51
1371
39
40
195
218
245
276
113
847
25
19
28
15
18
20
262
318
93
107
130
124
66
13
89
28
19
28
28
411
317
415
537
684
162
124
57
53
70
20
250
APO
APO
Binary
APO
APO
Binary occultation
APO
Binary occultation
Binary occultation
APO
APO
Binary
APO
Binary
APO
Binary 24 sigma odd-even
Binary
APO
APO
APO
APO
APO
APO
Contact Binary
Binary occultation
Binary
Binary
APO
APO
APO
APO
APO
APO
APO
APO
APO
Binary occultation
Binary occultation
Binary occultation
Binary
Binary
Binary
Binary
APO
APO
Binary
APO
Contact Binary
104
1416.01
1443.01
1446.01
1447.01
1447.02
1449.01
1450.01
1451.01
1453.01
1454.01
1455.01
1460.01
1461.01
1462.01
1464.01
1467.01
1469.01
1471.01
1482.01
1485.01
1487.01
1490.01
1492.01
1497.01
1500.01
1504.01
1509.01
1513.01
1514.01
1524.01
1538.01
1539.01
1542.01
1548.01
1550.01
1551.01
1554.01
1555.01
1556.01
1559.01
1562.01
1565.01
1566.01
1568.01
1571.01
1575.01
1578.01
1579.01
11517719
11197126
12506351
7622486
7622486
7802136
7532973
9632895
7842610
7830637
4760746
7751571
9579499
11913013
7838655
7770450
7543649
11858748
7812167
9692345
12062667
9602514
12108312
11774387
9719634
9641018
9535080
9784222
9520668
4826110
9963461
8081482
8113154
9940565
8111381
5444549
9899355
12644774
9902856
9899280
5308663
5636648
5564247
5210475
5557821
5553652
5629985
9898364
68.335
67.77461
66.78619
94.30528
66.63923
70.1369
66.98404
92.74682
66.85321
70.3035
296.54861
296.97389
73.70776
288.31141
289.32963
287.74883
288.51958
110.82595
298.35756
66.66256
66.72336
66.51884
66.80535
111.15178
67.27943
67.1991
86.04295
66.96052
66.61153
67.18301
116.00779
66.8696
66.81655
68.06092
67.72031
348.94868
287.58427
312.12282
210.32841
66.37641
288.58306
66.97062
288.36227
287.85676
289.29149
74.04144
67.78972
67.47018
2.495801
4.494499
1.227759
40.246662
2.279999
10.980248
2.144631
27.322068
0.971933
121.590891
15.068135
17.041841
7.946693
3.747881
2.113152
1.157752
3.581956
1.780979
17.792773
0.687895
2.929223
3.556617
0.705449
0.520205
3.351587
2.178178
49.644312
1.197304
1.399319
1.333363
10.581586
2.819448
2.586873
2.13933
2.233799
31.138459
1.332604
41.077414
135.913711
1.332583
0.784473
0.466743
1.727256
1.008933
2.928799
24.329742
2.272058
7.132434
26075
232
44429
148151
15260
49724
18255
78850
9596
11369
13227
5115
5706
2747
1991
1040
1168
881
1545
517
427
324
490
430
486
346
650
319
276
189
115934
72512
26617
5437
2966
9975
911
4286
10827
621
905
837
649
432
473
1217
255
695
154
28
235
303
205
929
225
1241
344
35
143
110
68
25
92
47
54
35
30
38
50
40
57
26
34
41
64
31
15
13
982
205
162
114
197
122
49
60
95
66
33
72
14
19
19
15
36
64
Binary
APO
Binary
V-shaped Binary
Binary Brown Dwarf
Binary
Binary
Binary occultation
APO
Binary occultation
APO
APO
Binary
APO
APO
APO
APO
APO
APO
APO
APO
APO
APO
APO
APO
APO
Binary phased locked variations
APO
APO
APO
Eccentric Binary
Binary
Binary
Binary
APO Binary Secondary eclipse
APO
APO Binary Secondary eclipse
APO
APO
APO
APO
APO
APO
APO
APO
APO Eccentric Binary
APO
APO
105
1580.01
1592.01
1594.01
1600.01
1604.01
1607.01
1610.01
5193400
5217586
9895709
4860932
10033279
5477805
5474733
80.18576
76.14359
66.12217
67.76764
72.77578
67.53825
66.60625
21.382619
26.06809
1.818944
3.091207
72.491574
5.006818
0.883781
418
681
325
235
1267
232
122
18
30
21
17
49
20
17
APO
APO
APO
APO
APO
APO
APO
106
107
108
109
Table 5. Candidates in or near the Habitable Zone (sorted by Teq)
KOI
!"#$%&'
&+"*$%&'
&%*!$%&'
&+%#$%&'
&%,,$%&'
"+)$%&'
)##$%*'
&)"!$%&'
(%&$%#'
#+&$%&'
,%*$%&'
*&&$%&'
&)*#$%&'
&)*,$%&'
&#!&$%&'
"($%&'
&#,$%&'
*!"$%&'
&)(*$%&'
+#!$%&'
"%!$%&'
&#(+$%&'
"&*$%#'
"!+$%&'
#+&$%*'
+&$%&'
&+,!$%*'
)&!$%*'
!**$%&'
+++$%*'
&+()$%&'
#*!$%&'
(%$%#'
&*!&$%&'
&+*($%&'
&#*"$%&'
+!)$%*'
&)("$%&'
Kp
(mag)
&#$(&'
&+$)'
&)$(+'
&)$"#'
&+$))'
&+$"+'
&)$,*'
&+$+&'
&#$(#'
&#$"'
&+$(+'
&)$,,'
&+$()'
&+$+#'
&)$,,'
&&$!!'
&#$),'
&%$+!'
&+$%!'
&)$+'
&+$)'
&#$(&'
&+$,+'
&+$%,'
&#$"'
&#$(!'
&+$&!'
&)$*,'
&)$,#'
&)$(!'
&)$!'
&*$,!'
&*$+'
&+$&*'
&)$""'
&+$!('
&)$"+'
&*$)+'
Rp
(R! )
)$&)'
)$))'
&$(('
*$!"'
#$!+'
&$,&'
&#$#('
"$)#'
&$(#'
"$)"'
+$!!'
,$+"'
)$*"'
)$&+'
*$*'
*$)*'
+$!+'
&$(+'
#$+('
*$,('
"$,('
&($""'
*$&*'
+$,)'
!'
)$("'
#$))'
*$"*'
,$*"'
*$*('
+$(+'
%$"+'
&$,!'
!$*+'
)$")'
)$"&'
)$,('
#$(#'
Period
(days)
*("$&*'
&"!$#"'
,)$&'
&+%$*)'
&!&$+#'
+!$%+'
#*"$*)'
*+)$+!'
&**$#,'
##&$!+'
"#$,'
#(*$&&'
&*)$)*'
*%+$,#'
+,$""'
*",$"!'
**)$(,'
&&%$#('
"+$#+'
&!*$#)'
&)#$&"'
#*&$**'
)!$&,'
&&,$%*'
*&%$)+'
&%$)#'
&%+$#!'
""$*+'
&++$%+'
"!$+'
&&)$(#'
"$,('
(($!&'
&##$)!'
&,*$!('
"%$,('
&*($",'
(!$&#'
Teff
(K)
+!*)'
+#")'
#"%*'
+#+!'
+!!+'
#()#'
+*#('
+!""'
)"!,'
!&%#'
)#&*'
!%(*'
+*""'
++,+'
)%+%'
+!%!'
+,*&'
)"%"'
+)++'
+!&)'
+*%!'
!&!,'
)%,('
++!%'
!&%#'
#*)%'
)!+!'
+%"#'
+&(&'
+*&"'
++#('
#*)%'
+#)*'
+(!%'
+)(%'
+)*+'
+!"!'
+))&'
R*
( R !)
%$("'
%$!)'
%$!"'
%$+!'
%$++'
%$),'
&$%"'
%$"#'
%$!"'
%$,)'
%$!+'
&$%,'
%$!!'
%$"!'
%$+,'
&$&)'
%$,'
%$(,'
%$+!'
%$")'
%$""'
&$&('
%$+('
%$(#'
%$,)'
%$*('
%$,"'
%$(+'
&$&('
%$("'
%$"+'
%$*('
%$('
%$,'
&$#&'
%$(*'
%$,#'
%$('
Teq
(K)
*#,'
*)%'
*)*'
*)*'
*))'
*)"'
*),'
*+!'
*!*'
*!!'
*(%'
*(#'
*()'
*(!'
*(,'
*"*'
*""'
*,+'
*,+'
*,!'
*,!'
#%%'
#%&'
#%!'
#%,'
#&)'
#&!'
#&('
#*('
##&'
##&'
##*'
###'
##+'
##('
##"'
#)%'
#)&'
a
(AU)
%$")'
%$!#'
%$##'
%$+)'
%$+('
%$**'
%$,)'
%$"'
%$)+'
%$,('
%$#*'
&$%+'
%$)('
%$!,'
%$*)'
%$""'
%$()'
%$)&'
%$#('
%$+,'
%$+#'
%$,!'
%$*&'
%$)('
%$(&'
%$%!'
%$)*'
%$#"'
%$+('
%$#"'
%$)('
%$%+'
%$#+'
%$+*'
%$!('
%$#!'
%$+&'
%$#+'
110
!"##$%!&
"+($%!&
+!!$%"&
**)$%(&
*!#$%!&
'*+$%!&
!+*$%!&
*%!$%(&
!#,*$%!&
!#+$%#&
",#$%!&
"+*$%!&
'#($%"&
)!+$%!&
)*+$%!&
!!#'$%!&
!#$'&
!($"'&
!"$'+&
!*$'&
!*$!!&
!#$!'&
!"$+)&
!*&
!#$('&
!"$+!&
!!$(&
!($(!&
!#$)%&
!#$*!&
!#$(%&
!#$""&
($)!&
)$**&
($,(&
"$+)&
+$+&
($+*&
($#(&
,$,&
"$%+&
"$("&
($"*&
"$""&
($*&
($!&
#$!&
#$"&
#!$'"&
!(#$,!&
!(*$#(&
*"$,(&
!,,$+'&
()$,&
#,$"#&
!,%$%!&
#"$*#&
!!)$")&
)!$+*&
!+($,+&
(($+)&
("$'+&
)%$)+&
,*$,(&
##('&
#,")&
#*))&
*(,*&
#)("&
")('&
*,#*&
#(,*&
#+%'&
#,+#&
#")'&
#)('&
"'!!&
"'%#&
#*,'&
*)),&
%$#(&
%$'#&
!&
%$+!&
!$!#&
%$,*&
%$)&
!$*&
%$#,&
!&
%$),&
!$(,&
%$#,&
%$#'&
%$))&
%$'!&
"*(&
"**&
"*#&
"*,&
"#(&
"#"&
"##&
"#+&
",%&
",!&
","&
",#&
",#&
"+%&
"+(&
"+(&
%$(+&
%$#&
%$*'&
%$(!&
%$,!&
%$!#&
%$(+&
%$#'&
%$()&
%$*)&
%$"+&
%$,"&
%$!(&
%$!"&
%$"+&
%$"%&
111