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Berkeley - ASTRO - 00177408
# tmin tmax 0.12055600 5.38475 [ksec];instrument XRT;exposure 266.08283;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 - 00177408
Wavdetect Sources with S/N>3: # ra dec err ["] signif counts steady? -log10(Prob_steady) 054.03492117.3458570.16673.8725.0 0-323.0 154.10150117.3244240.51014.141.8 1-0.7 254.01671417.2622120.65812.338.3 1-0.1 354.155
Berkeley - ASTRO - 00177408
output00177408000_999/sw00177408000xwtw2po_cl.evtoutput00177408001_999/sw00177408001xwtw2po_cl.evtoutput00177408002_999/sw00177408002xwtw2po_cl.evtoutput00177408003_999/sw00177408003xwtw2po_cl.evtoutput00177408004_999/sw00177408004xwtw2po_cl.evt
Berkeley - ASTRO - 00177408
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 - 00177408
# Ep dEp lprob lEiso dlEiso67.040 0.054 3.49e-05 121.421 0.07467.097 0.061 3.07e-04 121.521 0.08467.163 0.070 5.88e-04 121.521 0.08467.238 0.081 8.49e-04 121.521 0.08467.325 0.092 1.10e-03 121.521 0.08467.423 0.106 1.29e-03 121.521 0.08467.537
Berkeley - ASTRO - 00177408
# Ep lEiso37.400 121.94840.123 121.88245.004 121.87446.499 121.58146.920 121.42847.877 121.33148.473 121.58348.868 121.63749.323 121.34449.341 121.34849.662 121.44650.219 121.40150.425 121.54350.808 121.47751.066 121.54551.173 121.583
Berkeley - ASTRO - 00177408
# Ep dEp lprob lNiso dlNiso67.040 0.054 3.49e-05 137.769 0.38167.097 0.061 3.06e-04 137.769 0.38067.163 0.070 5.87e-04 137.769 0.38067.238 0.081 8.65e-04 137.769 0.38067.325 0.092 1.10e-03 137.769 0.38067.423 0.106 1.29e-03 137.769 0.38067.537
Berkeley - ASTRO - 00177408
# Ep lNiso37.362 137.60340.096 137.25245.016 138.22146.520 138.10846.941 137.70147.899 137.88448.495 138.38548.881 138.62249.337 137.33249.355 137.35049.676 137.78350.234 137.58650.440 138.20350.817 137.91451.076 137.64251.182 137.219
Berkeley - ASTRO - 00177408
# x=Log_e(Beaming Fraction) y=Log_e(Egam/10^52 erg) z=Log_e(Tjet/days)# mean(x)= -4.6913 xdown= -5.0763 xup= -4.3622# mean(y)= -2.8349 ydown= -3.4214 yup= -2.2964# mean(z)= 1.8541 zdown= 1.3195 zup= 2.2750-5.9761 -3.7625 0.1152-5.8878 -3.7402
Berkeley - ASTRO - 00177408
Ep=55.60 Chi/nu= 51.27/57 (0.899)
Berkeley - ASTRO - 00177408
#file=swb15-350lc.txt dt=1.0 tstart=-10.095 tstop=113.025#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 109.000 1.932 86.000 2.765 58.000
Berkeley - ASTRO - 00177408
# S/N T1 T2 T90 T50# Estimated T100 Interval: -13.065 150.555 T90= 136.350 30.5 80.085 107.625 23.220 8.910 17.0 -7.395 19.335 23.490 9.180 5.5 124.095 150.555
Berkeley - ASTRO - 00177408
;instrument XRT;exposure 61149.182;xunit kev;bintype counts 0.0000000 0.0049999999 13.666843 1.00000 0.0049999999 0.0099999998 13.715614 1.00000 0.0099999998 0.015000000 13.764385 1.0
Berkeley - ASTRO - 00177408
# tmin tmax 10.0000 468.416 [ksec];instrument XRT;exposure 56383.773;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 - 00177408
# tmin tmax 10.0000 468.416 [ksec];instrument XRT;exposure 56383.773;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 - TMP - 00177408
Power-Law Model FitNorm@15keV 1.1934e-02 (1.0364e-02 1.3625e-02)alpha -1.7375 (-1.8620 -1.6154)Energy Fluence (15-350 keV) 2.5948e-06 (2.4156e-06 2.7852e-06) erg cm^-2Eiso (1-10^4 keV, host-frame) 1.6697e+53 (1.5405e+53 1.8461e+53) ergChi/nu=
Iowa State - DATA - 1336
Palmer Constitution 2008PreambleWe, the members of Palmer House do establish and adopt this constitution in order to form an efficient house, ensure equal representation of each resident, and secure an environment that stimulates intellectual, soci
Drexel - MK - 489
11 July 2007By: Lucian Dorneanu, Science EditorNanomachines Powered by BacteriaMicroscopic organisms can move tiny structures when stimulated with UV lightA new discovery in the field of nanotechnology could produce the smallest "engines" in th
Rose-Hulman - ME - 422
FORMULA SHEET For 1-D heat transfer problems, the general weak form is dT dT Ak dx = dx dx T AgdxFor a 2-node conduction element, when the area, conductivity, density, and internal heat generation are constant we have K= kA Le 1 -1 -1 1 2 1 1 2 1 1
Maryland - ENEE - 646
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Maryland - ENEE - 646
ENEE 646: Digital Computer DesignFall 2004 Handout #1Course Information and PolicyRoom:CHE 2108 TTh 2:00p.m. - 3:15p.m. http:/www.ece.umd.edu/class/enee646 Donald Yeung 1327 A. V. Williams (301) 405-3649 yeung@eng.umd.edu http:/www.ece.umd.edu
Maryland - ENEE - 646
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Maryland - ENEE - 646
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Maryland - ENEE - 646
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Maryland - ENEE - 646
ENEE 646: Digital Computer DesignFall 2004 Handout #11Problem Set # 2Due: October 12Pipelining and ILPProblem 1Consider the following 6-stage pipline:F D X1 X2 M WInstruction fetch Instruction decode, register read First cycle of ALU, b
Maryland - ENEE - 646
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Maryland - ENEE - 646
ENEE 646: Digital Computer DesignFall 2004 Handout #13Midterm Review 1 Time and LocationThe midterm will be given during normal class hours, 2:00p.m.-3:15p.m., on Thursday October 14th, in the normal meeting place, CHE 2108.2FormatThe midt
Maryland - ENEE - 646
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Maryland - ENEE - 646
%!PS-Adobe-2.0 %Creator: dvips(k) 5.86 Copyright 1999 Radical Eye Software %Title: midterm-sol.dvi %Pages: 5 %PageOrder: Ascend %BoundingBox: 0 0 612 792 %DocumentFonts: CMBX12 CMR10 CMBX10 CMMI10 CMMI8 CMSY10 CMSY8 %EndComments %DVIPSWebPage: (www.r
Maryland - ENEE - 646
ENEE 646: Digital Computer DesignFall 2004 Handout #17Midterm Solutions11.1Early Branch Resolution(10 points):(see Figures 1, 2, 3, and 4 for pipeline diagrams).1.2(10 points):The forwarding path from register G can be removed. Since
Maryland - ENEE - 646
%!PS-Adobe-2.0 %Creator: dvips(k) 5.86 Copyright 1999 Radical Eye Software %Title: ps3.dvi %Pages: 4 %PageOrder: Ascend %BoundingBox: 0 0 612 792 %DocumentFonts: CMBX12 CMR10 CMTT10 CMSY10 %EndComments %DVIPSWebPage: (www.radicaleye.com) %DVIPSComman
Maryland - ENEE - 646
ENEE 646: Digital Computer DesignFall 2004 Handout #20Problem Set # 3Due: November 23Complex Pipelining and CachingProblem 1H&P 3.10Problem 2In this problem, we will look at how a common vector loop runs on two processors, one that imple
Maryland - ENEE - 646
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Maryland - ENEE - 646
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Maryland - ENEE - 646
ENEE 646: Digital Computer DesignFall 2004 Handout #24Problem Set # 4Due: Dec 9Memory Performance Optimizations and Virtual MemoryProblem 1H&P 5.8Problem 2H&P 5.17Problem 3H&P 5.181
Maryland - ENEE - 646
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Maryland - ENEE - 646
ENEE 646: Digital Computer DesignFall 2004 Handout #25Programming Assignment # 3 Control SpeculationDue: December 9In this assignment, you will add control speculation to the out-of-order Tomasulo model you built in programming assignment #2.
Maryland - ENEE - 646
%!PS-Adobe-2.0 %Creator: dvips(k) 5.86 Copyright 1999 Radical Eye Software %Title: final-review.dvi %Pages: 4 %PageOrder: Ascend %BoundingBox: 0 0 612 792 %DocumentFonts: CMBX12 CMR10 CMTI10 CMTT10 CMBX10 CMSY10 %EndComments %DVIPSWebPage: (www.radic
Allan Hancock College - I - 386
Table of Errors:Most of these will prevent the hard disk from working correctly under DOS, soit's not likely that you ever get these errors.Invalid root sector signature The last two bytes of the root sector should be 55 AA (hex). This is a
Allan Hancock College - I - 386
Revision History of FIPS-version 2.0 - may 11, 1998- Official release with FAT32 support, updated documentationversion 1.5b - decemeber 22, 1997- Not an official release. Gordon Chaffee added FAT32 support to fips.Version 1.5 - august 22,
Allan Hancock College - I - 386
Technical Info on FIPS-FIPS was written in C+ V2.0 with the Turbo C+ 1.0 and Borland C+ 3.1compilers.It should compile with any newer C+ compiler (perhaps after minor changesto the BIOS calls).If you're a C+ wizard, don't look too closely at
S.F. State - GM - 310
Medjber/SeddonReading Questions for Student-Led Discussions: How Erosion Builds Mountains1) What are the three processes that interact to shape and build the world's mountain ranges? Which process seems to be the strongest of the three? 2) What wa
Iowa State - CS - 577
Solution to Assignment 1Com S 477/5771. Since p = (u , v ) is the reflection of p in , the vector (p - p) is paralle to the normal vector of , therefore the cross product of two 2-d vectors is 0. This gives us the first equation (p - p) (a, b) =
Drexel - CS - 475
From greenie at cs.drexel.edu Sun Mar 29 19:08:39 2009From: greenie at cs.drexel.edu (Rachel Greenstadt)Date: Sun, 29 Mar 2009 19:08:39 -0400Subject: [Cs475] NGR for CS 475Message-ID: <20090329230839.GG15555@tux64-01>Dear class, Several of
Drexel - CS - 123
From augendavid at hotmail.com Fri Jun 5 15:38:08 2009From: augendavid at hotmail.com (David Augenblick)Date: Fri, 5 Jun 2009 13:38:08 -0600Subject: [Cs123] CS123 - SECTION 81 STUDENTS ONLY!Message-ID: <BLU125-W10914C294D706DC53244C9C9480@phx.g
University of Illinois, Urbana Champaign - GEO - 107
PLATE TECTONICSLab #1 Aug. 25-26What is a plate? Def: a rigid section of Earth's crust Plates interact along their boundaries. Tectonic activity: earthquakes, volcanoesPlate Boundaries Convergent: plates move toward each other EQ & volcano
University of Illinois, Urbana Champaign - GEO - 107
Average Annual Global Temperature Year Temperature, oC 1880 13.75 1881 13.81 1882 13.78 1883 13.74 1884 13.69 1885 13.73 1886 13.75 1887 13.69 1888 13.76 1889 13.80 1890 13.65 1891 13.70 1892 13.64 1893 13.61 1894 13.65 1895 13.73 1896 13.84 1897 13.
University of Illinois, Urbana Champaign - GEO - 107
ShorelinesLab #10 Nov. 10 & 11Shorelines As Dynamic Environments Erosion By waves & storms Rate depends on coastal materials Deposition Source & supply of sediment CurrentsSome Shoreline FeaturesHeadlands Sea arch Sea stacksWave Base
University of Illinois, Urbana Champaign - GEO - 107
Surface temperature from 1860 until 2000 shows an overall rise of 0.9C. The future projections are following CO2 emissions and atmospheric ghg concentrations (in ppmv - parts per million by volume). The red line shows Business-as-Usual (BAU) where th
University of Illinois, Urbana Champaign - GEO - 432
Geol432 Mineralogy & Mineral OpticsMineral ListLIST OF MINERALSBold: You should know their diagnostic features in hand specimens and their chemical formulaePlain: You should know which class they below to and the major elements in themLiPag
University of Illinois, Urbana Champaign - GEO - 143
GEOLOGY 143: HISTORY OF LIFEUniversity of Illinois Fall Semester 2008Instructor: Professor Bruce W. Fouke, Room 138 NHB Office Phone: 244-5431 Email: fouke@illinois.edu Office hours: Mondays 4 5 pm, Room 138 NHB Teaching Assistants: Carly Hill, Ph
University of Illinois, Urbana Champaign - GEO - 143
GEOLOGY 143: HISTORY OF LIFEUniversity of Illinois Fall Semester, 2008Instructor: Professor Bruce W. Fouke, Room 138 NHB Phone: 244-5431 Email: fouke@illinois.edu Office Hours: Mondays 4 5 pm, Rm 138 NHB Teaching Assistants: Carly Hill, Phone: 244
University of Illinois, Urbana Champaign - GEO - 562
Tom Johnson, 8/25/08Isotope Geochem Introduction: Why isotopes?Modern geoscientists use isotope measurements for nearly every kind of study. A large fraction of the papers published involve some type of isotope data. Why is this? What are the gene
University of Illinois, Urbana Champaign - GEO - 562
Reviews in Mineralogy & Geochemistry Vol. 55, pp. 65-111, 2004 Copyright Mineralogical Society of America3Applying Stable Isotope Fractionation Theory to New SystemsEdwin A. SchaubleDepartment of Earth and Space Sciences University of Californ
University of Illinois, Urbana Champaign - GEO - 562
Tom Johnson 9/4/08Intro to Mass Dependent FractionationReading: White Ch. 27 Required Schauble, 2004 (from 2004 No-traditional Stable Isotopes RiMG volume; posted on web site) Other resources: Valley and Cole, Chapter 1, Chacko, Cole, and Horita;
University of Illinois, Urbana Champaign - GEO - 562
T. Johnson 9/9/08Kinetic Fractionation and Rayleigh ProcessesReading: Chapter 28 in White: "Kinetic Fractionation." Schauble, 2004: Part of his chapter summarizes theory on kinetic isotope fractionation. Guide Questions: - In a chemical reaction i