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XRT ;exposure ;instrument 159.64227 ;xunit kev ;bintype counts 0.0000000 0.0049999999 14.506662 1.00000 0.0049999999 0.0099999998 14.558423 1.00000 0.0099999998 0.015000000 14.610183 1.00000 0.015000000 0.020000000 14.661944 1.00000 0.020000000 0.025000000 14.713704 1.00000 0.025000000 0.029999999...
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Berkeley - ASTRO - 00349931
#ra dec rmag drmag294.98160440.13237219.1600.124294.89363640.13383719.1200.115294.75677040.13614919.4110.156294.73282340.13651218.5320.070294.60228240.13848118.4250.063294.76896540.13623119.1360.131294.42581340.14147319.241
Berkeley - ASTRO - 00349931
chi^2/nu= 27.921656 / 54.0000The fit is rejectable at 0.12586167 % Confidence#index t1 t2 fade_index delta_mag_pk hindex dhindex rate1 drate1 rate2 drate2 logr dlogr 0 0.0740 0.2385 -1.61 0.0 0.08 0.35 1.22E+0
Berkeley - ASTRO - 00349931
# t1 t2 hardness error 0.074013000 0.082258000 0.37772675 0.18001959 0.082258000 0.12066200 0.15609077 0.14777033 0.12066200 0.18585300 0.41742592 0.16705802 0.18585300 0.29617400
Berkeley - ASTRO - 00349931
output00349931000_999/sw00349931000xpcw3po_cl.evtoutput00349931004_999/sw00349931004xpcw3po_cl.evtoutput00349931005_999/sw00349931005xpcw3po_cl.evtoutput00349931006_999/sw00349931006xpcw3po_cl.evtoutput00349931007_999/sw00349931007xpcw3po_cl.evt
Berkeley - ASTRO - 00349931
# t1 t2 dt rad_min rad_max cts err scl bg bg_rat wt 0.074013 0.075814 0.001801 0. 16. 9.00 3.00 0.686435 0.000000 0.322223 1 0.075814 0.078108 0.002293 0. 16. 10.36
Berkeley - ASTRO - 00349931
# t1 t2 dt rad_min rad_max cts err scl bg bg_rat wt 0.074013 0.075814 0.001801 0. 16. 9.00 3.00 0.686435 0.000000 0.322223 1 0.075814 0.078108 0.002293 0. 16. 10.36
Berkeley - ASTRO - 00349931
# tmin tmax 0.0905750 503.906 [ksec];instrument XRT;exposure 76313.869;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.000000 0
Berkeley - ASTRO - 00349931
# tmin tmax 0.0905750 503.906 [ksec];instrument XRT;exposure 76313.869;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.000000 0
Berkeley - ASTRO - 00349931
# tmin tmax 0.0740130 9.93482 [ksec];instrument XRT;exposure 156.61169;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.000000 0
Berkeley - ASTRO - 00349931
# tmin tmax 0.0740130 9.93482 [ksec];instrument XRT;exposure 156.61169;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.000000 0
Berkeley - ASTRO - 00349931
Wavdetect Sources with S/N>3: # ra dec err ["] signif counts steady? -log10(Prob_steady) 0294.94458440.2800100.28450.3375.9 1-1.0 1294.74784640.3841540.21449.2363.0 0-92.4 2294.71067040.5523550.34727.2151.7 1-2.9 329
Berkeley - ASTRO - 00349931
SIMPLE = T / file does conform to FITS standardBITPIX = 8 / number of bits per data pixelNAXIS = 0 / number of data axesEXTEND = T / FITS dataset may contain extensio
Berkeley - ASTRO - 00349931
# Ep dEp lprob lEiso dlEiso90.459 0.074 3.10e-05 -11.830 0.19590.533 0.078 -6.70e-05 -11.830 0.17190.616 0.089 -1.85e-04 -11.830 0.16990.711 0.102 -3.69e-04 -11.830 0.16990.820 0.117 -4.78e-04 -11.830 0.16890.946 0.134 -6.52e-04 -11.830 0.1689
Berkeley - ASTRO - 00349931
# Ep lEiso1.069 -11.2241.153 -11.3531.615 -10.9661.978 -11.0122.227 -11.1682.794 -11.4233.290 -11.3093.784 -11.1774.572 -11.3754.617 -11.3695.421 -11.2056.925 -11.3187.655 -11.3319.171 -11.16611.135 -11.36211.947 -11.61016.076 -11.30
Berkeley - ASTRO - 00349931
# Ep dEp lprob lNiso dlNiso90.459 0.074 3.10e-05 5.299 0.34790.533 0.078 -4.96e-05 5.299 0.34890.616 0.089 -1.84e-04 5.299 0.34890.711 0.102 -4.88e-04 5.299 0.34890.820 0.117 -5.01e-04 5.299 0.34890.946 0.134 -8.27e-04 5.299 0.34891.089 0.153
Berkeley - ASTRO - 00349931
# Ep lNiso1.069 6.9871.153 6.8061.615 7.3551.979 7.2792.228 7.0432.795 6.7893.292 7.3593.787 6.9824.577 6.7074.622 6.7115.425 6.8596.929 6.6217.658 6.8939.172 6.63111.137 6.38011.949 6.09316.072 6.28416.702 6.14918.223 5.69518.625
Berkeley - ASTRO - 00349931
Spectra Extracted from tstart=3.330 tstop=61.550(Trigger Time, GPS=924406530.600000, Redshift, z=0.0)Power-Law Model FitNorm@15keV 4.5777e-03 (2.7938e-03 6.7963e-03)alpha -1.6071 (-2.0240 -1.2150)Energy Fluence (15-350 keV) 5.9842e-07 (4.5971e
Berkeley - ASTRO - 00349931
; Instrument bat; Exposure 58.22; xunit keV; bintype counts 0.00000 10.0000 -0.00626039 0.014290246 10.0000 12.0000 0.0424353 0.046175073 12.0000 14.0000 0.0252161 0.032041994 14.
Berkeley - ASTRO - 00349931
#file=swbz_15-350lc.txt dt=0.02 tstart=3.330 tstop=61.550#t90 dt90 t50 dt50 rt90 drt90 rt50 drt50 rt45 drt45 tav dtav tmax dtmax trise dtrise tfall dtfall cts cts_err pk_rate dpk_rate band 12.160 21.296 8.500 8.187 1.840
Berkeley - ASTRO - 00349931
#file=swbz_15-350lc.txt dt=0.02 tstart=3.330 tstop=61.550#t90 dt90 t50 dt50 rt90 drt90 rt50 drt50 rt45 drt45 tav dtav tmax dtmax trise dtrise tfall dtfall cts cts_err pk_rate dpk_rate band 12.160 20.657 8.500 3.088 1.840
Berkeley - ASTRO - 00349931
#file=swb15-350lc.txt dt=1.0 tstart=3.330 tstop=61.550#t90 dt90 t50 dt50 rt90 drt90 rt50 drt50 rt45 drt45 tav dtav tmax dtmax trise dtrise tfall dtfall cts cts_err pk_rate dpk_rate band 13.000 21.525 10.000 4.197 7.000 2.
Berkeley - ASTRO - 00349931
# S/N T1 T2 T90 T50# Estimated T100 Interval: 3.330 61.550 T90= 55.901 16.1 3.430 4.570 0.980 0.380 9.3 10.930 12.850 1.780 0.640 5.9 51.790 61.550
Berkeley - ASTRO - 00349931
# tmin tmax 10.0000 503.90628 [ksec];instrument XRT;exposure 73093.715;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.00000
Berkeley - ASTRO - 00349931
;instrument XRT;exposure 73872.452;xunit kev;bintype counts 0.0000000 0.0049999999 10.350064 1.00000 0.0049999999 0.0099999998 10.387064 1.00000 0.0099999998 0.015000000 10.424065 1.0
Berkeley - ASTRO - 00349931
# tmin tmax 10.0000 503.90628 [ksec];instrument XRT;exposure 73093.715;xunit kev;bintype counts0.000000 0.010000 0.000000 0.0000000.010000 0.020000 0.000000 0.0000000.020000 0.030000 0.000000 0.0000000.030000 0.040000 0.00000
Arizona - PHYS - 141
Physics 141 Homework 5 Solutions 1. You might think that a compound pulley (as in Question 1 on the exam) violates conservation of energy. After all, if you can pull on one rope with a force of 1250 N and lift a 2500 N walrus, arent you getting energ
Mines - ESGN - 520
Hydrological Probability p There is a probability, p,that a flood greater than or equal to X (magnitude of the flood) will occur within the NEXT YEAR. (1-p) There is a probability, (1-p), also known as the reliability, that such a storm will not occu
Mines - ESGN - 520
Running Flood Frequency and Smada Programs Smada Program Run the sm16v6hydro.exe program. It will install Smada as you follow the instructions. 1. Go to your Smada directory where you have it installed, and double click on Smada6.exe. This will bring
Mines - ESGN - 520
Station Drainage Area Years Base Flow for Year 1888 1889 1890 1891 1896 1897 1898 1899 1900 1901 1920 1921 1922 1923 1924 1925 1926 1927 1928 1929 1930 1931 1932 1933 1934 1935 1936 1937 1938 1939 1940 1941 1942 1943 1944 1945 1946 1947 1948 1949 195
Mines - ESGN - 520
Station Drainage area Years Base Flow for Year 1891 1896 1897 1899 1900 1920 1921 1922 1923 1924 1925 1926 Date 5/27/1991 7/24/1996 8/4/1997 8/4/1999 7/29/2000 5/2/2020 6/3/2021 6/25/2022 8/16/2023 6/9/2023 8/6/2023 6/5/2024 8/30/2025 4/21/2026 6/3/2
Mines - ESGN - 520
Risk and Flood Frequency Exercise While constructing a bridge over Bear Creek while building C470, a large area of flood plain had to be disturbed. The design crew estimated that it would take 10 years for the vegetation to recover back to original c
Mines - ESGN - 520
Distribution Fitting Choosing a distribution The usual approach to distribution fitting is to fit as many distributions as possible and use goodnessof-fit tests to determine the best fit. This method, the empirical method, is subjective and is not al
Mines - ESGN - 520
FLUID STATICS AND DYNAMICS Turbulent vs laminar flow, REYNOLDS NUMBER, VISCOSITY, STATIC HEAD, VELOCITY HEAD, BERNOULLI'S EQUATION . Turbulent flow is a more effective transporter of sediment. Going to study FROUDE numbers to define tranquil vs rapid
Mines - ESGN - 520
The following are a group of graphics to go with the fluid mechanics notes: Hydraulically Smooth vs. Hydraulically RoughSpecific Energy; Froude NumbersFlow Profiles in Combination along a ReachHydraulic Jumps and Water Column Stability and Mixi
Mines - ESGN - 520
Program creates rectangular coordinate system with the lowest steak stake as a horizontal reference. Elevation above cross section low point is: (Maximum elevation to Horizontal Reference - absolute value of depth to Horizontal Reference)Maximum de
Mines - ESGN - 520
Solving for Downstream Depth Using the Froude Number Newtons equation for momentum change is solved simultaneously with Bernoullis equation and the continuity equation is used to define the downstream velocity in terms of the upstream velocity. The r
Mines - ESGN - 520
Water elevation above bottom of spillway, ftStorage above bottom of spillway, cu ftRate of outflow, cfsS/ t cfs 0 347 694 1041 1388 1735 2082 2429 2776 3123 3470(S/ t)-(O/2) (S/ t)+(O/2) cfs cfs 0 328 642 947 1241 1540 1824 2107 2386 2658 293
Mines - ESGN - 520
Draft Guidance for Water Quality-based Decisions: The TMDL Process (Second Edition)Disclaimer This document provides guidance to States, Territories and authorized Tribes exercising responsibility under section 303(d) of the Clean Water Act concerni
Mines - ESGN - 520
Time (minute) 0 5 10 20 30 40 50 60C (mg/L) 1/C (L/mg) 400 2.5 320 3.15 280 3.57 240 4.17 180 5.6 110 9.2 50 20 40 25ln C/C00 0.22 0.36 0.51 0.8 1.29 2.08 2.3Zero Order450 400 350 300 C, mg/L 250 200 150 100 50 0 0 10 20 30 40 50 60 70 Time,
Midwestern State University - AS - 350
AS 350 Reproductive Biotechnology Transgenic Animals Animal Cloning Embryo Transfer IVF, ICSIMay 1, 2009A transgenic animal is one that carries a foreign gene that has been deliberately inserted into its genome. Transgenic animals Mice 95% of al
Allan Hancock College - WEB - 3001
ApoAI ExperimentBINF 3001An Example Microarray Data AnalysisMatt WandConcerned with lipid metabolism and the role of the ApoAI gene.1ApoAI ExperimentApoAI ExperimentConcerned with lipid metabolism and the role of the ApoAI gene. How doe
Allan Hancock College - WEB - 3001
DisclaimerBINF 3001The R Computing EnvironmentMatt WandThe views expressed on the following slides are my personal views.12Brief History of S and R Early, 1990s: Auckland, New Zealand. Two members of Stats Dept there Ross Ihaka and Robe
Allan Hancock College - WEB - 3001
Early Landmark PapersBINF 3001Golub et al. Example of Tumor Classication with Microarray DataMatt WandScience, 1999 Proc. Nat. Acad. Sc. 1999Alon et al.Alizadeh et al. Nature, 20001 2Landmark Statistics PaperQuotes from Dudoit, Fridlya
Washington University in St. Louis - CS - 422
hpw y u pr u y wr p ~ pr y %|sprsyxt%xr2Vf%xt(VyGV}fQtUG(Vyf`|%(vyUVyG%Vrsyty yrp u y u f u ~ k yr y r t f%sCxtvyG%VkuXGsVp6UG%VfsVu(syty yrp u y u yo r u u ~ k yr y r u fsxt(VyG%Vk(%8xrVusp|spd}xGsVp6UG%(%Vfs% ty y ty{ u u ~
Arizona - MCB - 545
Need 2 students for each presentation.Jan 19, Hartwell cell cycle: Jan 31, Szostak recombination: Feb 2, Yu cohesins&condensins: Adriana & ?Molecular definition of a gene, continued.promoter Enhancer Exon 1 intron Exon 2 Enhancer Exon 3intron
Washington University in St. Louis - MEXMRS - 0524
=Upfront Notes= This "aareadme.txt" file contains the description of the naming convention that will be used for all MEX kernels. One part of them will be directly produced by an automated system located at ESTEC,PST. Consequently, we c
Washington University in St. Louis - MEXMRS - 0524
=MEX FK Files= Last Update: 12 MAY 2006 This "aareadme.txt" file describes the contents of the KERNELS/FK directory of the MEX SPICE data server. It also provides the file naming conventions used for the MEX FK kernels, and it provides id
Washington University in St. Louis - MEXMRS - 0524
=MEX CK Files= Last update: 22 NOV 2005 This "aareadme.txt" file describes the contents of the KERNELS/CK directory of the MEX SPICE data server. It also provides the file naming conventions used for the MEX CK files, and it provide
Washington University in St. Louis - MEXMRS - 0524
=MEX SPK Files= Last update: 30 MAY 2006 This "aareadme.txt" file describes the contents of the KERNELS/SPK directory of the MEX SPICE data server. It also provides the file naming conventions used for the MEX SPK kernels, and it pr
Washington University in St. Louis - MEXMRS - 0524
=MEX PCK Files= Last Update: 12 MAY 2006 This "aareadme.txt" file describes the contents of the KERNELS/PCK directory of the MEX SPICE data server. It also provides the file naming conventions used for the MEX PCK kernels, and it provides
Washington University in St. Louis - MEXMRS - 0524
=MEX LSK Files= Last update: 08 AUG 2005 This "aareadme.txt" file describes the contents of the KERNELS/LSK directory. It also provides the file naming conventions used for the MEX LSK kernels, and it provides identification of t
Washington University in St. Louis - MEXMRS - 0524
=MEX SCLK Files= Last update: 22 MAR 2004 This "aareadme.txt" file describes the contents of the KERNELS/SCLK directory of the MEX SPICE data server. It also provides the file naming conventions used for the MEX SCLK kernels, and it
Washington University in St. Louis - MEXMRS - 0524
=MEX Orbit Number Files= Last update: 11 MAY 2006 This "aareadme.txt" file describes the contents of the KERNELS/ORBNUM directory of the MEX SPICE data server. It also provides the file naming conventions used for the MEX Orbit Numbe
Uni. Worcester - RPK - 101
A short talk with Anthony LeggettTony Leggett (Anthony Leggett) is one of the three 2003 Physics Noble laureates. The award was for their pioneering contributions to the theory of superconductors and superfluids. He works in the Loomis Laboratory of
Alabama - T - 112
Cinema Antecedents, Edison, and LumiereCinema AntecedentsFirst Photograph: View from the Window at le Gras, Joseph Nicephore Nipce, June/July 1826More information. The Daguerreotype: Louis Jacques Mande Daguerre, process announced publicly 7 Jan
Uni. Worcester - RPK - 101
Uni. Worcester - RPK - 101
Uni. Worcester - RPK - 101
My Twelve Years in LASRoaming around the Kathmandu Valley from this school to that school for the job of a school teacher in the month of February 1992, I reached LAS. In fact, my teacher Madhav Dahal, who taught me in my high school for about thre