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На этой странице приведены все страницы сервера hea-www.harvard.edu ,которые мы индексируем. Показаны документы 6001 - 6020 из 7508.

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6001. http://hea-www.harvard.edu/AstroStat/Stat310_1011/vk_20101109.pdf
logN-logS A Measuring Stick for the Universe Vinay Kashyap (CfA) Tuesday , November 9, 2010 log10(N S)-log10(S) cumulative number of sources detectable at a given telescopic sensitivity S = [ergs s-1 cm-2] N = number of sources brighter than S Tuesday , November 9, 2010 simple example uniformly distributed source population all sources have same intrinsic luminosity for telescope sensitivity S, ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1011/vk_20101109.pdf -- 108.1 Кб -- 09.11.2010
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/talks_1011/vk_20101109.pdf -- 108.1 Кб -- 09.11.2010
[ Текст ]  Ссылки http://hea-www.harvard.edu/astrostat/talks_1011/vk_20101109.pdf -- 108.1 Кб -- 09.11.2010
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6002. http://hea-www.harvard.edu/AstroStat/etc/ADASS2010_skvcpr+.pdf
... 548, 224 A DA S S No v. 8 , 2 0 1 0 A n e ta S i e m i g i n o wska 2 Low Counts X-ray Data Ї Ї Ї Ї Ї Ї Ї Standard X-ray analysis in XSPEC or Sherpa Parameterized Forward Fitting of the data Assuming statistics - typically 2 Modified/weight 2 to account for low counts Bias when the distributions are not norm al. Poisson data - need to use the Poisson likelihood (e.g. Cash) MCMC methods probe the entire parameter space and do not get stuck in local minima (i.e. it can get out). ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/etc/ADASS2010_skvcpr+.pdf -- 1216.1 Кб -- 08.11.2010
[ Текст ]  Ссылки http://hea-www.harvard.edu/astrostat/etc/ADASS2010_skvcpr+.pdf -- 1216.1 Кб -- 08.11.2010
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6003. http://hea-www.harvard.edu/~fine/OSX/com.adamgerson.QuotaMonitorMenu.plist
<?xml version="1.0" encoding="UTF-8"?> <!DOCTYPE plist PUBLIC "-//Apple//DTD PLIST 1.0//EN" "http://www.apple.com/DTDs/PropertyList-1.0.dtd"> <plist version="1.0"> <dict> <key>KeepAlive</key> <false/> <key>Label</key> <string>com.adamgerson.QuotaMonitorMenu</string> <key>ProgramArguments</key> <array> <string>/Library/Application Support/QuotaMonitorMenu/QuotaMonitorMenu.app/Contents/MacOS/QuotaMonitorMenu</string> </array> <key>RunAtLoad</key> <true/> </dict> </plist>
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~fine/OSX/com.adamgerson.QuotaMonitorMenu.plist -- 1.5 Кб -- 01.11.2010
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6004. http://hea-www.harvard.edu/AstroStat/pyBLoCXS/_sources/index.txt
... Mixture of Metropolis and Metropolis-Hastings Jumping Rules * *defaultprior* -- Boolean to indicate that all parameters have the default flat prior. * *inv* -- Boolean or array of booleans indicating which parameters are on the inverse scale . * * log * -- Boolean or array of booleans indicating which parameters are on the logarithm scale (natural log ). * *originalscale* -- Array of booleans indicating which parameters are on the original ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/pyBLoCXS/_sources/index.txt -- 14.5 Кб -- 29.10.2010
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/astrostat/pyBLoCXS/_sources/index.txt -- 14.5 Кб -- 29.10.2010
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/astrostat/pyblocxs/_sources/index.txt -- 14.5 Кб -- 29.10.2010
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6005. http://hea-www.harvard.edu/ChandraSNR/G068.7+02.8/1984/work/ctb80_sou.pi.par
xswabs[xswabs] (XSPEC model name: wabs) (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.3341 1e-07 10 10^22/cm^2 powlaw[pow] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 1.7804 -10 10 2 ref frozen 1 0.438 6.8255 3 ampl thawed 1.8201e-03 7.4205e-06 7.4205e-02 END_SHOW_MODELS_BLOCK
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G068.7+02.8/1984/work/ctb80_sou.pi.par -- 1.7 Кб -- 26.10.2010
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6006. http://hea-www.harvard.edu/ChandraSNR/G006.4-00.1/2828/work/w28_sou.pi.par
xswabs[xswabs] (XSPEC model name : wabs) ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.5434 1e-07 10 10^22/cm^2 xsvmekal[xsvmekal] (XSPEC model name : vmekal) ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.5951 1e-03 100 keV 2 nH frozen 1 1e-06 1e+20 per cm**3 3 He frozen 1 0 1000 with respect to ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G006.4-00.1/2828/work/w28_sou.pi.par -- 2.8 Кб -- 26.10.2010
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6007. http://hea-www.harvard.edu/~pgreen/figs/Conversions.pdf
... A(A) A(A) 1 104A 108 ,\ 3.00x 1018/v 12.4/E 108 /WN 1.99x 1O-8/E A(Jlm) 10-4 ,\ 1 104A 3.00x1014/v 1.24 x 1O-3/E 104/WN 1.99x 10-12 /E j A(cm) 10-8,\ 10-4 ,\ 1 3.00x101°lv 1.24 x 10-7 l/WN .99x 10-16 v(Hz) 3.00x1018/A 3.00x 1014/ A 3.00x 1010/ A 1 E( keV ) 12.4/ A 1.24 X WN(cm-1) 108 /,\ 104/,\ 1/,\ 3.34x lO-ltv 8.07x106E 1 5.03x 1015E E(erg) 1.99x 10-8/ A 1.99 x 10-12/,\ 1.99x10-16/,\ ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/figs/Conversions.pdf -- 1547.6 Кб -- 20.10.2010
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6008. http://hea-www.harvard.edu/~pgreen/figs/Constants.pdf
... Solar mass M0 = 1.989x 1033 gm Solar radius Solar luminosity Earth mass Earth equatorial radius Gravity at earth's surface Ї Astronomical unit parsec light year Rayleigh Jansky steradian R0 L0 MEjl REjl gEjl AU pc lyr Ry ~ sr = 6.960x 1010 cm 3.826x 1033 erg s-1 5.976x 1027 gm 6.378 X 103 km 9.807x 102 cm s-2 1.496x 1013 cm 3.262 light years 3.086x 1018 cm 9.461x 1017 cm (1/411") X 106 photons/cm2/s/sr 10-26 watts/m2/Hz 3.283 X 103 deg2 1.182 X 107 arcmin2 4.255 X 1010 arcsec2 1. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/figs/Constants.pdf -- 1301.8 Кб -- 20.10.2010
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6009. http://hea-www.harvard.edu/~pgreen/figs/RaDecGal.pdf
RIGHT ASC~SION <,10' 2~ :z:l 22 120'" \ \0' ~ 2J 20 I'" J8 I7 I () 15 14 I:, 30' 12 (hr) IJ 10 '" K 7 h 5 1 :\ Ї. ... I I - 2 J" '~ I -I w~-L 50.1 ~. ... X\ L~tJt-1 ~(I" DEC~, l>/y.t/SiX v!J) \/\ Y0()</1T70'" \>(,0,J1,N /~/Oi. NY X \/(1\1~L!,l pEe o ~~ 0 ~>\ 0.x Xrv r ~', y" x"J.. ... I r~XL Iii \ \ ~ -so' '-.. ... 24 Z3 22 21 IJ 20 ~~ 19 III 17 I ----./ ... 1 I --- --'t,~-=.s _" ---.11 7----,--===l-KII" I" I :10 I -'Ill" -Ie," 13 -, II RIGHT ASCENSION (hr) (1950.0) s (;; r- A V _\ V- J (, \. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/figs/RaDecGal.pdf -- 1920.7 Кб -- 20.10.2010
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6010. http://hea-www.harvard.edu/ChandraSNR/G109.1-01.0C/6730/work/psr_sou.pi.par
xswabs[xswabs] (XSPEC model name: wabs) (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.8307 1e-07 10 10^22/cm^2 powlaw[pow] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 3.184 -10 10 2 ref frozen 1 0.657 2.7813 3 ampl thawed 7.0393e-04 7.8009e-07 7.8009e-03 END_SHOW_MODELS_BLOCK
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G109.1-01.0C/6730/work/psr_sou.pi.par -- 1.7 Кб -- 20.10.2010
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6011. http://hea-www.harvard.edu/ChandraSNR/G266.2-01.2/3846/work/g266_sou.pi.par
xswabs[xswabs] (XSPEC model name: wabs) (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.384 1e-07 10 10^22/cm^2 powlaw[pow] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 2.3504 -10 10 2 ref frozen 1 0.4161 3.2777 3 ampl thawed 3.1566e-03 1.2638e-05 0.1264 END_SHOW_MODELS_BLOCK
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G266.2-01.2/3846/work/g266_sou.pi.par -- 1.7 Кб -- 20.10.2010
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6012. http://hea-www.harvard.edu/~jcm/asc/docs/coords/coords5.ps
ASC Coordinates: Rev 5.0 SDSґ2.0 Jonathan McDowell 1999 Apr 4 Contents I Part 1: Missionґindependent formulation 6 1 General Introduction 6 1.1 Update notes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 1.2 Notational conventions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 1.2.1 Pixel convention . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 1.2.2 Vector and coordinate notation . . . . . . . . . . . . . . . . . . . . . . . . .
[ Текст ]  Ссылки http://hea-www.harvard.edu/~jcm/asc/docs/coords/coords5.ps -- 855.4 Кб -- 18.10.2010
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6013. http://hea-www.harvard.edu/~pgreen/Papers/SDSSJ1004_06.pdf
... In particular, we propose that variable spectral differences seen only in component A of the widest separation lens SDSS J1004+4112 are due to differential absorption along the sight lines. The absorber properties required by this hypothesis are akin to known broad absorption line ( BAL) outflows but must have a broader, smoother velocity profile. ... Subject headingg gravitational lensing -- quasars: absorption lines -- quasars: individual (SDSS J1004+4112) s: Online material: color figure 1. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/SDSSJ1004_06.pdf -- 567.6 Кб -- 13.10.2010
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6014. http://hea-www.harvard.edu/~pgreen/Morph/MMTmergers_sj2.aux
relax \@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces \relax \fontsize {8}{9.5}\selectfont Images of SDSS J1254+0846. LEFT: The optical image (1$^{\prime \prime }$\, seeing in r band with Magellan/IMACS) shows the two bright quasar nuclei, and reveals the tidal arms of a host galaxy merger. ... 2010). ... L_X$ for our general sample of Chandra/SDSS galaxies and AGN, with optical morphological classifications. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/Morph/MMTmergers_sj2.aux -- 2.8 Кб -- 12.10.2010
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6015. http://hea-www.harvard.edu/ChandraSNR/G340.6+00.3/10704/work/g340_sou.pi.par
xswabs[xswabs] (XSPEC model name : wabs) ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 5.0774 1e-07 10 10^22/cm^2 xsvmekal[xsvmekal] (XSPEC model name : vmekal) ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.8324 1e-03 100 keV 2 nH frozen 1 1e-06 1e+20 per cm**3 3 He frozen 1 0 1000 with respect to ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G340.6+00.3/10704/work/g340_sou.pi.par -- 2.8 Кб -- 06.10.2010
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6016. http://hea-www.harvard.edu/ChandraSNR/SNRJ0539.9-6944/3849/work/snr0540_sou.pi.par
xswabs[xswabs] (XSPEC model name : wabs) ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.3797 1e-07 10 10^22/cm^2 xsvmekal[xsvmekal] (XSPEC model name : vmekal) ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.6193 1e-03 100 keV 2 nH frozen 1 1e-06 1e+20 per cm**3 3 He frozen 1 0 1000 with respect to ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0539.9-6944/3849/work/snr0540_sou.pi.par -- 2.8 Кб -- 01.10.2010
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6017. http://hea-www.harvard.edu/ChandraSNR/G293.8+00.6/3924/work/g293_sou.pi.par
xswabs[xswabs] (XSPEC model name: wabs) (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.2631 1e-07 10 10^22/cm^2 powlaw[pow] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 1.4201 -10 10 2 ref frozen 1 0.4307 3.3507 3 ampl thawed 8.6012e-05 4.6063e-07 4.6063e-03 END_SHOW_MODELS_BLOCK
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G293.8+00.6/3924/work/g293_sou.pi.par -- 1.7 Кб -- 28.09.2010
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6018. http://hea-www.harvard.edu/ChandraSNR/G326.3-01.8/1965/work/g326_sou.pi.par
xswabs[xswabs] (XSPEC model name: wabs) (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.4988 1e-07 10 10^22/cm^2 powlaw[pow] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 1.9854 -10 10 2 ref frozen 1 0.6278 3.5551 3 ampl thawed 1.7393e-04 6.5276e-07 6.5276e-03 END_SHOW_MODELS_BLOCK
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G326.3-01.8/1965/work/g326_sou.pi.par -- 1.7 Кб -- 27.09.2010
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6019. http://hea-www.harvard.edu/ChandraSNR/G018.9-01.1/10098/work/g18.9_sou.pi.par
xswabs[xswabs] (XSPEC model name : wabs) ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.495 1e-07 10 10^22/cm^2 xsvmekal[xsvmekal] (XSPEC model name : vmekal) ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 1.0961 1e-03 100 keV 2 nH frozen 1 1e-06 1e+20 per cm**3 3 He frozen 1 0 1000 with respect to ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/G018.9-01.1/10098/work/g18.9_sou.pi.par -- 2.8 Кб -- 27.09.2010
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6020. http://hea-www.harvard.edu/AstroStat/Stat310_1011/haiku_ksm_20100927.pdf
Hierarchical Bayesian Models for Type Ia SN Light Curves, Dust and Cosmic Distances Kaisey S. Mandel Harvard University 27 September 2010 Monday, September 27, 2010 1 Hierarchical Brings deep knowledge from data Distant star glows, fades. Bob Kirshner Monday, September 27, 2010 2 Cosmological Energy Content Monday, September 27, 2010 3 !" ... 7 Monday, September 27, 2010 AAS 215 AAS 215 *+,+-./ ... Host Galaxy Dust: extinction and reddening. ... 19 Monday, September 27, 2010 19 ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1011/haiku_ksm_20100927.pdf -- 1968.3 Кб -- 27.09.2010
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/talks_1011/haiku_ksm_20100927.pdf -- 1968.3 Кб -- 27.09.2010
[ Текст ]  Ссылки http://hea-www.harvard.edu/astrostat/talks_1011/haiku_ksm_20100927.pdf -- 1968.3 Кб -- 27.09.2010
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