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6141. http://hea-www.harvard.edu/PINTofALE/pro/fitting/erors.pro
... failing sometimes when input A were ; integers (VK; Mar08) ;- forward_function mpfitfun ; usage ok='ok' np=n_params() nx= n_elements (x) ny= n_elements (y) na= n_elements (a) if np lt 4 then ok='insufficient parameters' else $ if nx eq 0 then ok='Input X undefined' else $ if ny eq 0 then ok='Input Y ... else $ if nx ne ny then ok='X and Y(X) not compatible' else $ if na eq 0 then ok='model parameters undefined' if ok ne 'ok' then begin ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/fitting/erors.pro -- 18.0 Кб -- 14.03.2008
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6142. http://hea-www.harvard.edu/PINTofALE/pro/cat_ln.pro
function cat_ln,AA,B, pick = pick , ask = ask ,okeV=okeV,comm=comm, flst = flst ,$ reord = reord , _extra=e ;+ ;function cat_ln ; returns a concatenated structure of Line emissivities ; ;syntax ; C=cat_ln(A,B, pick = pick , ask = ask ,comm=comm, reord = reord ,/okev,$ ; abund=abund,/noph,effar=effar,wvlar=wvlar,dem=dem,/temp,/ikev,/regrid) ; ;parameters ; A [INPUT; required] output of RD ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/cat_ln.pro -- 13.2 Кб -- 27.02.2008
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6143. http://hea-www.harvard.edu/ChaMPlane/cgi-bin/x-ray4pub/list.pl?c1=obsid&c2=target&format=txt&target=type
Browse by ObsID . Select obsid below. Click here for more information on X-ray fields (gl, gb, sorting, etc) and here for browsing guide. Click here to go back to the main page of data archive. obsid target ----- --------------------- 00095 A0620-00 00650 GKPERSEI 00676 GROJ0422+32 00755 B2224+65 00782 NGC1569 00829 3C123 01948 3EGJ2227+6122 02218 3C129 02545 M1-16 02553 MADDALENA'SCLOUD 02787 PSRJ2229+6114 02796 PSRJ0538+2817 02802 G127.1+0.5 02803 G166.0+4.2 02810 G116.9+0.2
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Ссылки http://hea-www.harvard.edu/ChaMPlane/cgi-bin/x-ray4pub/list.pl?c1=obsid&c2=target&format=txt&target=type -- 3.7 Кб -- 22.12.2007
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6144. http://hea-www.harvard.edu/PINTofALE/pro/scrypt/PoA_constructor.pro
... once per session, and ; that it is called _first_ ; ;history ; Vinay Kashyap (FebMMI; based on suggestion by A.Maggio) ; added ! ATOMDB and ! APECDIR (VK; Jun02) ;- ivar =0 defsysv ,'!PoA', exists = ivar if ( ivar eq 0) then defsysv ,'!PoA',2.61 ivar =0 defsysv ,'!TOPDIR', exists = ivar if ( ivar eq 0) then defsysv ,'!TOPDIR','/foo/bar/PINTofALE/' ivar =0 defsysv ,'!LDBDIR', exists = ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/scrypt/PoA_constructor.pro -- 4.5 Кб -- 15.12.2007
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6145. http://hea-www.harvard.edu/AstroStat/rfits/rfits_0.2.2/INSTALL
No configuration file for you! 0) Install R and cfitsio, determine locations of fitsio.h, R.h, Rinternals.h libcfitsio.so, libR.so (Note: you may have to edit the Makefile for cfitsio to force it to make a shared library.) 1) Edit Makefile 2) "make shared" 3) Move librfits.so to desired library location 4) Edit first lines of rfits.r to point to libcfitsio.so and librfits.so 5) See rfits.API for list of RFITS functions and their arguments
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Ссылки http://hea-www.harvard.edu/AstroStat/rfits/rfits_0.2.2/INSTALL -- 1.5 Кб -- 13.12.2007
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/rfits/rfits_0.2.2/INSTALL -- 1.5 Кб -- 13.12.2007
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/rfits/rfits_0.2.2/INSTALL -- 1.5 Кб -- 13.12.2007
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6146. http://hea-www.harvard.edu/AstroStat/etc/CCW2007_109_drkeijmsv.pdf
Monte Carlo Methods for Including Calibration Uncertainties in Model Fitting Analyses Jeremy J. Drakea , Peter Ratzlaffa , Vinay Kashyapa , Richard Edgara , Rima Izemb , Diab Jeriusa , Herman ... University, Cambridge, MA 02138 MIT Kavli Institute for Astrophysics and Space Research, Cambridge, MA 02139 b c SUMMARY Ї Instrument response uncertainties almost universally ignored in astrophysical X-ray ... Limiting accuracy of Chandra ACIS reached in spectra with 10 4 counts. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/etc/CCW2007_109_drkeijmsv.pdf -- 1178.6 Кб -- 30.10.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/etc/CCW2007_109_drkeijmsv.pdf -- 1178.6 Кб -- 30.10.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/etc/CCW2007_109_drkeijmsv.pdf -- 1178.6 Кб -- 30.10.2007
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6147. http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/wp-content/uploads/2007/05/r_tutorial.pdf
... Advanced Modern Statistical Computing I Fall 2006 Department of Statistics, University of Pittsburgh Hints for Using Splus/R Taeyoung Park This is designed to give a brief overview of Splus and some of the main commands you will need to know. ... Online help: From the Splus prompt, type help.start(). ... Either z <- x+y or z x+y will assign the vector sum of x and y to a vector named z. (c) Note: To do a dot product multiplication of 2 vectors, you must type vector1%*%vector2. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/wp-content/uploads/2007/05/r_tutorial.pdf -- 65.7 Кб -- 24.10.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/slog/groundtruth.info/AstroStat/slog/wp-content/uploads/2007/05/r_tutorial.pdf -- 65.7 Кб -- 24.10.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/slog/groundtruth.info/AstroStat/slog/wp-content/uploads/2007/05/r_tutorial.pdf -- 65.7 Кб -- 24.10.2007
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6148. http://hea-www.harvard.edu/vlp_m33_public/sasaki_poster.pdf
Chandra ACIS Survey of M33 ( ChASeM33 ): The X-ray Point Source Population of M33 M. Sasaki (CfA), B. Williams (University of Washington), P. Plucinsky (CfA), W. Pietsch (MPE), T. J. Gaetz (CfA), K. S. Long (STScI ... University), F. Haberl (MPE), T. G. Pannuti (Morehead State University), P. Ghavamian (JHU), L. Bianchi (JHU), A. Tolea (JHU), and the ChASeM33 team With most of the 1.4 Ms of Chandra ACIS ... Fig. ... We interpret this as an eclipse of the X-ray source. ...
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Ссылки http://hea-www.harvard.edu/vlp_m33_public/sasaki_poster.pdf -- 1065.4 Кб -- 26.09.2007
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6149. http://hea-www.harvard.edu/vlp_m33_public/tpannuti_aas.pdf
Wavelength-Dependent Selection Effects in Searches for SNRs in Nearby Galaxies Venn diagram depicts optical, radio and X-ray (Chandra) detections of SNRs in five nearby spiral galaxies (M81, M101, NGC 2403, NGC 4736 and NGC 6946) (Limiting LX ? ... 8%) Effects of ambient density and confusion? ... XRB/SNR Associations (e.g., MF16 in NGC 6946, MF22 in M81); also, X-ray counterparts to radio and optical SNRs with "discordant" Xray colors IR (Spitzer) and Radio (Single Dish+VLA) complementary data? ...
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Ссылки http://hea-www.harvard.edu/vlp_m33_public/tpannuti_aas.pdf -- 50.3 Кб -- 26.09.2007
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6150. http://hea-www.harvard.edu/vlp_m33_public/gaetz_IAU2006.pdf
Chandra ACIS Survey of M33 (ChASeM33): X-ray Imaging and Spectroscopy of the Bright SNR M33SNR21 T.J. Gaetz, R.J. Edgar, P.P. Plucinsky, M. Sasaki (SAO), P. Ghavamian, W. P. Blair (Johns Hopkins) B. Williams (U. Washington), K.S. Long (STScI), P.F. Winkler (Middlebury College), J.P. Hughes (Rutgers) T. Pannuti (Spitzer Sci. ... The shor t axis of the M33SNR 21 X-ray axis runs through the brightest par t of the remnant, and the optical emission extends well beyond the X-ray rim in the southwest. ...
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Ссылки http://hea-www.harvard.edu/vlp_m33_public/gaetz_IAU2006.pdf -- 330.9 Кб -- 26.09.2007
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6151. http://hea-www.harvard.edu/AstroStat/Stat310_0708/ac_20070918.pdf
... Stories: Ї Ї Ї Ї Whirlwind History Sky of Many Colors Astronomy+Physics+Statistics CHASC: (brief!) ... X-Ray Sky: Ends of stars and the flickering sky ROSAT All-Sky ~1.5 KeV (Digel and Snowden): Black Holes, Neutron Stars, Active stars --and local glowing gas Gamma-Ray Sky: Pulsars, Active Galaxies, and lots of (nonthermal) glowing gas Ways of Paying Attention: Astronomy Perspective to 1980 After a good beginning, Isolated Ї Ї Ї Ї Ї Started out together (Kepler, LaPlace, .. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_0708/ac_20070918.pdf -- 2871.8 Кб -- 18.09.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0708/ac_20070918.pdf -- 2871.8 Кб -- 18.09.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0708/ac_20070918.pdf -- 2871.8 Кб -- 18.09.2007
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6152. http://hea-www.harvard.edu/PINTofALE/pro/plotem.pro
pro plotem, logT ,EM, idstr = idstr ,markmin=markmin, multid = multid ,$ lcol=lcol,lsiz=lsiz, tlog = tlog ,wdth=wdth,$ xtitle=xtitle,ytitle=ytitle,title=title,xrange=xrange,yrange=yrange,$ xstyle=xstyle,ystyle=ystyle,xlog=xlog,ylog=ylog ... _extra=e ;+ ;procedure plotem ; plots emission measures derived from the output of POTEM_TOOL ; (or other means) ; ;syntax ; plotem, logT ,EM, idstr = idstr ,markmin=markmin, multid = ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/plotem.pro -- 9.7 Кб -- 06.09.2007
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6153. http://hea-www.harvard.edu/PINTofALE/pro/potem_tool.pro
... Z and OUTID.( ION to floats in case multiple IDs have ; been collapsed to one emissivity (VK; Dec98) ; added field FLUXERR to output IDSTR (VK; Mar99) ; changed call to INITSTUFF to INICON (VK; 99May) ; no need to read in ion balance info in POTTASCH again (VK; JanMMI) ; added keyword WDTH to carry the emissivity width info outside ; (VK; SepMMVII) ;- ; usage nid=n_tags( idstr ) if nid eq 0 then begin print,'Usage: EM=potem_tool( idstr , flux , logT = logT , abund = ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/potem_tool.pro -- 10.8 Кб -- 06.09.2007
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6154. http://hea-www.harvard.edu/~fine/Tech/dagger.bdf
... SLANT R SETWIDTH_NAME Normal SPACING c CHARSET_REGISTRY ISO-8859 CHARSET_ ENCODING 1 COPYRIGHT Designer of this font retains full rights under the law FONT_ASCENT 10 FONT_DESCENT 4 ENDPROPERTIES CHARS 221 STARTCHAR C001 ENCODING 1 SWIDTH 692 0 DWIDTH 9 0 BBX 7 7 1 1 BITMAP 10 38 7c ee 7c 38 10 ENDCHAR STARTCHAR C002 ENCODING 2 SWIDTH ...
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Ссылки http://hea-www.harvard.edu/~fine/Tech/dagger.bdf -- 25.2 Кб -- 30.08.2007
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6155. http://hea-www.harvard.edu/ChandraSNR/SNRJ0046.6-7307/3904/work/snr.reg.pi.par
xswabs * xsmekal ) xswabs [ xswabs ] (XSPEC model name : wabs) ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.5778 1e-07 10 10^22/cm^2 xsmekal [ xsmekal ] (XSPEC model name : mekal) ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.1742 1e-03 100 keV 2 nH ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0046.6-7307/3904/work/snr.reg.pi.par -- 1.9 Кб -- 28.08.2007
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6156. http://hea-www.harvard.edu/AstroStat/etc/scma4_ac_dvd.pdf
... 1 Poisson Goodness-of-fit 2 Question 1: What physical model parameters b est fit the data, and what are their uncertainties; Question 2: What is the evidence for an additional comp onent of known shap e (such as a line in an an energy sp ectrum or a p oint-source in an image); Question 3: Is this b est-fit good enough; and Question 4: If the fit is not good enough how does one quantify the unknown additional structure in the image and the uncertainties in this structure? ... CGRO/EGRET data. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/etc/scma4_ac_dvd.pdf -- 881.3 Кб -- 17.08.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/etc/scma4_ac_dvd.pdf -- 881.3 Кб -- 17.08.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/etc/scma4_ac_dvd.pdf -- 881.3 Кб -- 17.08.2007
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6157. http://hea-www.harvard.edu/AstroStat/BEHR/BEHR_tutorial.txt
... BEHR" with 6 required arguments in any order. ... In addition to the required arguments , you can input 20 optional arguments that correspond to - softeff= : soft effective area. (softeff=1 by default ) - hardeff= : hard effective area. (hardeff=1 by default ) - softidx= : soft index, i.e., the shape parameter of a gamma prior dist'n for the soft source intensity. (softidx=0.5 by default ) - hardidx= : hard index, i.e., the shape parameter of a gamma prior dist'n for the ...
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Ссылки http://hea-www.harvard.edu/AstroStat/BEHR/BEHR_tutorial.txt -- 6.9 Кб -- 16.08.2007
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/BEHR/BEHR_tutorial.txt -- 6.9 Кб -- 16.08.2007
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/BEHR/BEHR_tutorial.txt -- 6.9 Кб -- 16.08.2007
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6158. http://hea-www.harvard.edu/ChandraSNR/G033.6+00.1/1982/work/fit_detail.txt
[snr.reg.pi] note01= note02= pi_name=snr.reg.pi source=(xswabs * xsvmekal) par_file=snr.reg.pi.par fit_ps_file=snr.reg.pi.fit.ps Reduced statistic=3.016446
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Ссылки http://hea-www.harvard.edu/ChandraSNR/G033.6+00.1/1982/work/fit_detail.txt -- 1.2 Кб -- 15.08.2007
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6159. http://hea-www.harvard.edu/AstroStat/etc/JSM2007_tlee.pdf
... Classification (in progress) Ї spatial complexity measure Ї separating line Future Work Ї JSM 2007 ґ p. 6/2 Our Approach Ї two main stages: detection and classification JSM 2007 ґ p. 7/2 Our Approach Ї two main stages: detection and classification Ї detection : quite simple (thanks to high image quality) JSM 2007 ґ p. 7/2 Our Approach Ї two main stages: detection and classification Ї ... similarly for black pixels: A(B ) w W l (w ) L (w ) JSM 2007 ґ p. 14/2 ( |W | ...
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Ссылки http://hea-www.harvard.edu/AstroStat/etc/JSM2007_tlee.pdf -- 199.6 Кб -- 12.08.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/etc/JSM2007_tlee.pdf -- 199.6 Кб -- 12.08.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/etc/JSM2007_tlee.pdf -- 199.6 Кб -- 12.08.2007
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6160. http://hea-www.harvard.edu/AstroStat/etc/JSM2007_dvd.pdf
Image Analysis Model-Based Methods Comparing and Evaluating Models Summary Fur ther Reading Fully Bayesian Analysis of Low-Count Astronomical Images David A. van Dyk1 Alanna Connors 2 1 Depar tment of Statistics University of California, Ir vine 2 Eurika Scientific Thanks to James Chiang, Adam Roy, and The California Har vard AstroStatistics Collaboration. ... Is our physical model sufficient to explain the data? ... Principled methods for comparing / evaluating models. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/etc/JSM2007_dvd.pdf -- 1056.3 Кб -- 08.08.2007
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/etc/JSM2007_dvd.pdf -- 1056.3 Кб -- 08.08.2007
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/etc/JSM2007_dvd.pdf -- 1056.3 Кб -- 08.08.2007
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