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6181. http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/hl_20070410.pdf
Introducing BLoCXS and Using it to Estimate Calibration Uncertainties Hyunsook Lee Warnings Flow Charts Calibration Beyond ARF Introducing BLoCXS and Using it to Estimate Calibration Uncertainties Hyunsook Lee CfA April 10, 2007 Introducing BLoCXS and Using it to Estimate Calibration Uncertainties Hyunsook Lee Warnings Flow Charts Calibration Beyond ARF Acknowledgement and Warnings Ї Vinay Kashyap and BLoCXS developers! ... Prior to this, thorough understanding BLoCXS is a must. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/hl_20070410.pdf -- 514.8 Кб -- 10.04.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310MM_VI_VII/hl_20070410.pdf -- 514.8 Кб -- 10.04.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310MM_VI_VII/hl_20070410.pdf -- 514.8 Кб -- 10.04.2007
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6182. http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/detail.ps
Separate Bkg counts Yes parameters Re-estimate Bkg GLM Draw Bkg Parameters Fit Bkg Separate lines and continuum Lines >0 Yes No No Remove RMF Blurring Sample ARF Compute Loglikelihood Begin MCMC Done? Yes No End MCMC Restore absorbed counts Draw Continuum and Metropolis-Hastings Algorithm Deround photon energy from lines Absorption Parameters with Draw line parameters (location, scale, and intensities)
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/detail.ps -- 14.2 Кб -- 10.04.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310MM_VI_VII/detail.ps -- 14.2 Кб -- 10.04.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310MM_VI_VII/detail.ps -- 14.2 Кб -- 10.04.2007
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6183. http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/blocxs.ps
Counts Spectrum FILTER Transformation for GLM Set Priors Background Continuum Line Absorption PowerLaw Bremsstrahlung BrokenPowerLaw xsabs expabs EM Effective Area Blurring Matrix Exposure Time Background Source Counts Spectrum - procedures Delta Lorentzian Gaussian BlackBody Model Specification Model Parameter Estimates Channel vs. Counts MCMC draws for parameters LogLikelihood LogLikelihood Filter Indicator Energy vs. ARF Channel vs. Counts Energy vs. ARF OUTPUT: OUTPUT: Filter Indicator MCMC
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/blocxs.ps -- 17.7 Кб -- 10.04.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310MM_VI_VII/blocxs.ps -- 17.7 Кб -- 10.04.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310MM_VI_VII/blocxs.ps -- 17.7 Кб -- 10.04.2007
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6184. http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/analysis.ps
Begin EM Maximize to update Yes No Converge Condt'l Expectation of Begin MCMC Data Augmentation Draw Parameters Aug. Data Loglikelihood No Yes Data Augmentation Aug. Data Loglikelihood parameters End MCMC Done? End EM
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310MM_VI_VII/analysis.ps -- 9.0 Кб -- 10.04.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310MM_VI_VII/analysis.ps -- 9.0 Кб -- 10.04.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310MM_VI_VII/analysis.ps -- 9.0 Кб -- 10.04.2007
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6185. http://hea-www.harvard.edu/ChandraSNR/SNRJ0519.5-6902/118/work/aa5_fit.par
abs02 * vray054) xswabs[ abs02 ] ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.3298 1e-07 10 10^22/cm^2 Xspec function name: xsabsw. xsvraymond[vray054] ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.3689 0.0808 80 keV 2 He thawed 1.6780 0 10000 with respect to Solar 3 C thawed 8.1943e-08 0 ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0519.5-6902/118/work/aa5_fit.par -- 2.6 Кб -- 04.04.2007
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6186. http://hea-www.harvard.edu/ChandraSNR/SNRJ0519.5-6902/118/work/snr_fit1.par
abs03 * (vray01 + vray054)) xswabs[abs03] ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.2446 1e-07 10 10^22/cm^2 Xspec function name : xsabsw. xsvraymond [vray01] ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT frozen 0.6419 0.0808 80 keV 2 He frozen 0 0 10000 with respect to Solar 3 C frozen 0 0 10000 with ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0519.5-6902/118/work/snr_fit1.par -- 3.9 Кб -- 04.04.2007
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6187. http://hea-www.harvard.edu/ChandraSNR/SNRJ0519.5-6902/118/work/aaa01.par
abs01 * vray01) xswabs[ abs01 ] ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.2283 1e-07 10 10^22/cm^2 Xspec function name: xsabsw. xsvraymond[vray01] ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.6419 0.0808 80 keV 2 He frozen 0 0 10000 with respect to Solar 3 C frozen 0 0 10000 with ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0519.5-6902/118/work/aaa01.par -- 2.6 Кб -- 04.04.2007
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6188. http://hea-www.harvard.edu/ChandraSNR/SNR0506-68.0/2762/work/fit_detail.txt
Total: Weak internal source included. [snr.reg] pi_name=snr_0506.pi source=(xswabs * xsvmekal) par_file=snr.reg.par fit_ps_file=snr_0506.pi.fit.ps Reduced statistic=9.565976 Goodness: computed with Chi-Squared Gehrels DataSet 1: 245 data points -- 239 degrees of freedom. Statistic value = 2286.27 Probability [Q-value] = 0 Reduced statistic = 9.56598 --end--
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNR0506-68.0/2762/work/fit_detail.txt -- 1.4 Кб -- 04.04.2007
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6189. http://hea-www.harvard.edu/ChandraSNR/SNRJ0526.0-6604/747/work/ee1.2.par
(abs01 * pow01) xswabs[abs01] (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.3391 1e-07 10 10^22/cm^2 Xspec function name: xsabsw. powlaw1d[pow01] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 2.7603 -10 10 2 ref frozen 1 0.3869 9.9791 3 ampl thawed 0.0009 3.5415e-06 0.0354
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0526.0-6604/747/work/ee1.2.par -- 1.7 Кб -- 02.04.2007
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6190. http://hea-www.harvard.edu/ChandraSNR/SNRJ0526.0-6604/747/work/ee1.1.par
(abs01 * pow01) xswabs[abs01] (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.4528 1e-07 10 10^22/cm^2 Xspec function name: xsabsw. powlaw1d[pow01] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 2.9773 -10 10 2 ref frozen 1 0.3869 9.9791 3 ampl thawed 0.0011 3.5415e-06 0.0354
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0526.0-6604/747/work/ee1.1.par -- 1.7 Кб -- 02.04.2007
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6191. http://hea-www.harvard.edu/ChandraSNR/SNRJ0526.0-6604/747/work/ee3.reg.par
abs01 * (ray11 + ray12)) xswabs[abs01] ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH frozen 0.3373 1e-07 10 10^22/cm^2 Xspec function name : xsabsw. xsraymond [ray11] ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.8424 0.0080 64 keV 2Abundanc frozen 0.3000 0 5 3Redshift frozen 0 0 5 4 norm ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0526.0-6604/747/work/ee3.reg.par -- 2.3 Кб -- 02.04.2007
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6192. http://hea-www.harvard.edu/ChandraSNR/SNRJ0540.1-6919/119/work/shell.par
abs02 * ((ray01 + ray02) + ray03)) xswabs[abs02] ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH frozen 0.4591 1e-07 10 10^22/cm^2 Xspec function name : xsabsw. xsraymond [ray01] ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.1929 0.0080 64 keV 2Abundanc frozen 1 0 5 3Redshift frozen 0 0 5 4 norm ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0540.1-6919/119/work/shell.par -- 2.8 Кб -- 02.04.2007
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6193. http://hea-www.harvard.edu/ChandraSNR/SNRJ0540.1-6919/119/work/cc1.par
(abs01 * pow01) xswabs[abs01] (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.4591 1e-07 10 10^22/cm^2 Xspec function name: xsabsw. powlaw1d[pow01] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 1.8656 -10 10 2 ref frozen 1 0.4088 9.6287 3 ampl thawed 0.0001 2.9081e-07 0.0029
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0540.1-6919/119/work/cc1.par -- 1.7 Кб -- 02.04.2007
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6194. http://hea-www.harvard.edu/ChandraSNR/SNRJ0540.1-6919/119/work/cs1.par
(abs02 * pow02) xswabs[abs02] (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.4737 1e-07 10 10^22/cm^2 Xspec function name: xsabsw. powlaw1d[pow02] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 1.7110 -10 10 2 ref frozen 1 0.4599 9.3951 3 ampl thawed 0.0021 8.2699e-06 0.0827
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0540.1-6919/119/work/cs1.par -- 1.7 Кб -- 02.04.2007
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6195. http://hea-www.harvard.edu/ChandraSNR/SNRJ0540.1-6919/119/work/cs2.par
(abs02 * pow02) xswabs[abs02] (integrate: off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH frozen 0.4591 1e-07 10 10^22/cm^2 Xspec function name: xsabsw. powlaw1d[pow02] (integrate: on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 gamma thawed 1.6791 -10 10 2 ref frozen 1 0.4599 9.3951 3 ampl thawed 0.0020 8.2699e-06 0.0827
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0540.1-6919/119/work/cs2.par -- 1.7 Кб -- 02.04.2007
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6196. http://hea-www.harvard.edu/~bradw/letgcoves/Deron/poster.pdf
... Е?5 Е2?F?13BF?DЕ?? ... B??31ED4t???&?r31?h?C&4?Е?3?74d6?? Е7?fЕЕ?3@6Е?1?@ ... 2Еe 1 ? ... 3G3Е?5d3?3q&06?r%?4?CC34?? ... 1Cqt&ABF!Е?#65Е6?@?3?dBx5??31?pЕ23$3?43?64?CC6!C6? ... 3Е?d?1ЕЕ5 3Е43?? ... R??F Е?9?3CЕ?DЕЕF?Е??? ... 3Е26?136)ЕЕ?' ... 3?Е31 ABSTRACT Note: uniforms will be obligatory starting 11/12/2006 Jeremy interviewing prospective replacements The Calibration of Young Pease Coves, et al. ...
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Ссылки http://hea-www.harvard.edu/~bradw/letgcoves/Deron/poster.pdf -- 1747.8 Кб -- 15.03.2007
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6197. http://hea-www.harvard.edu/~pgreen/spitzer.pdf
Binary Quasars, P.J. Green et al. ... 2005). ... The parent sample of binary quasars was tiny, and extremely heterogeneous. ... 1.4 Sp ectral Energy Distributions (SEDs) We will compare our sample quasar properties to the large and growing archival sample of single quasars similarly imaged by both Spitzer and Chandra. ... P. J. Green, T. L. Aldcroft, S. Mathur, B. J. Wilkes & M. Elvis 2001, ApJ, 558, 109, A Chandra Survey of Broad Absorption Line Quasars Binary Quasars, P.J. Green et al. ...
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Ссылки http://hea-www.harvard.edu/~pgreen/spitzer.pdf -- 307.5 Кб -- 10.03.2007
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6198. http://hea-www.harvard.edu/PINTofALE/ardb/chandra_letg_ao9.par
... We use as the temperature grid !LOGT. ... For a scripted example with less details, see the companion thread ; on the low-resolution spectrum generation. ... To work around this, we use the mid- bin values ;cstr.midWVL, and mid2bound(), which gives intelligent bin -boundary ;values given the mid- bin values: CWB =mid2bound(cstr_c.midWVL) CDW= CWB [1:*]- CWB conint_c=conint_c*CDW ;[ph/s/ Ang ]*[ Ang ] CWB =mid2bound(cstr_a.midWVL) CDW= CWB [1:*]- CWB conint_a=conint_a*CDW ;[ph/s/ Ang ]*[ ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/ardb/chandra_letg_ao9.par -- 18.7 Кб -- 01.03.2007
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6199. http://hea-www.harvard.edu/PINTofALE/pro/bamabs.pro
... nw=n_elements(w) if np eq 0 then ok='Insufficient parameters' else $ if nw eq 0 then ok='W is undefined' if ok ne 'ok' then begin print,'Usage: sigabs=bamabs(w, abund = abund ,/ikeV,/Fano,noHeH=noHeH,verbose=v)' print,' return photoelectric absorption cross-sections following' print,' Balucinska-Church McCammon 1992 update to Morrison McCammon 1983' if np ne 0 then message,ok,/info return,-1L endif ; inputs nrg=[float(abs(w))] nab=n_elements( ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/bamabs.pro -- 17.3 Кб -- 01.03.2007
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6200. http://hea-www.harvard.edu/ChaMPlane/papers/0612-draft-xavier-magellan.pdf
Investigating Chandra X-ray sources in the Galactic Bulge with Magellan LDSS2 sp ectra Xavier Ko enig,1 Jonathan E. Grindlay,1 Maureen van den Berg,1 Silas Layco ck,1 Ping Zhao,1 JaeSub Hong1 and Eric M. Schlegel2 ABSTRACT We have carried out optical and X-ray spectral analysis on a sample of Xray detected optical sources found in five Galactic-bulge fields included in our Chandra Multi-wavelength Plane Survey. ... Almost all X-ray sources in Table 4 have only one candidate optical counterpart. ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/papers/0612-draft-xavier-magellan.pdf -- 603.0 Кб -- 27.02.2007
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