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7101. http://hea-www.harvard.edu/~fine/Tech/shadow.bdf
... SLANT R SETWIDTH_NAME Normal SPACING c CHARSET_REGISTRY ISO-8859 CHARSET_ ENCODING 1 FONT_ASCENT 14 FONT_DESCENT 4 ENDPROPERTIES CHARS 156 STARTCHAR C040 ENCODING 32 SWIDTH 923 0 DWIDTH 12 0 BBX 12 18 0 -4 BITMAP 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 ...
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Ссылки http://hea-www.harvard.edu/~fine/Tech/shadow.bdf -- 28.0 Кб -- 26.03.2004
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7102. http://hea-www.harvard.edu/~fine/Tech/shadow-bold.bdf
... SLANT R SETWIDTH_NAME Normal SPACING c CHARSET_REGISTRY ISO-8859 CHARSET_ ENCODING 1 FONT_ASCENT 14 FONT_DESCENT 4 ENDPROPERTIES CHARS 156 STARTCHAR C040 ENCODING 32 SWIDTH 923 0 DWIDTH 12 0 BBX 12 18 0 -4 BITMAP 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 ...
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Ссылки http://hea-www.harvard.edu/~fine/Tech/shadow-bold.bdf -- 28.0 Кб -- 26.03.2004
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7103. http://hea-www.harvard.edu/~fine/Tech/radon.bdf
... SLANT R SETWIDTH_NAME Normal SPACING c CHARSET_REGISTRY ISO-8859 CHARSET_ ENCODING 1 FONT_ASCENT 10 FONT_DESCENT 2 ENDPROPERTIES CHARS 190 STARTCHAR C040 ENCODING 32 SWIDTH 615 0 DWIDTH 8 0 BBX 8 12 0 -2 BITMAP 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 ENDCHAR ...
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Ссылки http://hea-www.harvard.edu/~fine/Tech/radon.bdf -- 27.9 Кб -- 26.03.2004
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7104. http://hea-www.harvard.edu/~fine/Tech/radon-wide.bdf
... ;Medium SLANT R SETWIDTH_NAME Wide SPACING c CHARSET_REGISTRY ISO-8859 CHARSET_ ENCODING 1 FONT_ASCENT 10 FONT_DESCENT 2 ENDPROPERTIES CHARS 95 STARTCHAR C040 ENCODING 32 SWIDTH 692 0 DWIDTH 9 0 BBX 9 12 0 -2 BITMAP 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 ENDCHAR ...
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Ссылки http://hea-www.harvard.edu/~fine/Tech/radon-wide.bdf -- 14.8 Кб -- 26.03.2004
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7105. http://hea-www.harvard.edu/~fine/Tech/inkblot.bdf
... SLANT R SETWIDTH_NAME Normal SPACING c CHARSET_REGISTRY ISO-8859 CHARSET_ ENCODING 1 FONT_ASCENT 10 FONT_DESCENT 3 ENDPROPERTIES CHARS 96 STARTCHAR C040 ENCODING 32 SWIDTH 692 0 DWIDTH 9 0 BBX 9 13 0 -3 BITMAP 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 0000 ENDCHAR ...
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Ссылки http://hea-www.harvard.edu/~fine/Tech/inkblot.bdf -- 15.3 Кб -- 26.03.2004
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7106. http://hea-www.harvard.edu/~fine/Tech/atari-small.bdf
... ENCODING 63 SWIDTH 1 0 DWIDTH 4 0 BBX 4 8 0 -1 BITMAP 00 40 a0 20 40 00 40 00 ENDCHAR STARTCHAR @ ENCODING 64 SWIDTH 1 0 DWIDTH 4 0 BBX 4 8 0 -1 BITMAP 00 40 a0 a0 80 80 60 00 ENDCHAR STARTCHAR A ENCODING 65 SWIDTH 1 0 DWIDTH 4 0 BBX 4 8 0 -1 BITMAP 00 40 a0 a0 e0 a0 a0 00 ENDCHAR STARTCHAR B ENCODING 66 SWIDTH 1 0 DWIDTH 4 0 ...
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Ссылки http://hea-www.harvard.edu/~fine/Tech/atari-small.bdf -- 14.3 Кб -- 26.03.2004
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7107. http://hea-www.harvard.edu/PINTofALE/ardb/chandra_acis_ao6.par
chandra_acis_ao6.par ; generate an ACIS spectrum for a source using a DEM , ; and optionally rescale the DEM to produce the same ; counts as a ROSAT / PSPC observation ; ;calling sequence ; .run initale ; @chandra_acis_ao6.par ; ;(LL/VK; modified from chandra_acis_ao5.par, Feb04) ;- ... density [cm^-3] T_components = [6.9, 7.4] ;log(T[K]) components in the EM EM_components = [5.1d12, 6.1d12] ;Emission Measure [cm^-3] obs_rate = 0.1 ; ROSAT / ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/ardb/chandra_acis_ao6.par -- 5.6 Кб -- 02.03.2004
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7108. http://hea-www.harvard.edu/PINTofALE/ardb/chandra_hetg_ao6.par
... We use as the temperature grid !LOGT. ... Also, we will ; construct spectra at two different densities: ne = 1e12 and 1e9 [cm-3] ;make input theoretical spectrum grid dwvl=float((!WMAX-!WMIN)/nwbin) wgrid =findgen(nwbin+1L)*dwvl+!WMIN ; read in gARFs if strlowcase(file_ARFp) ne 'none' then $ effar_p=rdarf(file_ARFp,ARSTRp) else $ effar ... $ effar_n=fltarr(nwbin) if n_tags(ARSTRp) gt 0 then $ wvlar_p=!fundae.KEVANG/(0.5*(ARSTRp.ELO+ARSTRp.EHI)) else $ wvlar_p=0.5*( wgrid [1:*]+ ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/ardb/chandra_hetg_ao6.par -- 18.1 Кб -- 02.03.2004
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7109. http://hea-www.harvard.edu/PINTofALE/papers/linl_PINTofALEMarkov.pdf
Package for the Interactive Analysis of Line Emission: Markov-Chain and Monte Carlo Methods LiWei Lin, Vinay L. Kashyap, Jeremy J. Drake Smithsonian Astrophysical Observatory 60 Garden St., Cambridge, MA 02138 pintofale@head.cfa.harvard.edu Abstract We describe the implementation of Monte Carlo methods in the Package for Interactive Analysis of Line Emission (PINTofALE), which is a collection of IDL-based programs designed to analyze astrophysical spectra. ... Monte Carlo methods in PINTofALE 4.1. ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/papers/linl_PINTofALEMarkov.pdf -- 634.5 Кб -- 24.02.2004
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7110. http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.1/readme
JaeSub Hong, 2003-2004 Quantile analysis routines: 3 independent platforms (will) be available - IDL , perl , and C IDL : quantile.pro : main program, read the usage in the begining of the file example .pro : example of using quantile.pro perl : quantile.pl : main program, read the usage in the begining of the file src.txt : example src file bkg .txt : example bkg ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.1/readme -- 1.7 Кб -- 19.02.2004
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7111. http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.0/readme
JaeSub Hong, 2003-2004 Quantile analysis routines: 3 independent platforms (will) be available - IDL, perl, and C IDL: quantile.pro : main program, read the usage in the begining of the file example.pro : example of using quantile.pro perl: quantile.pl : main program, read the usage in the begining of the file src.txt : example src file bkg.txt : example bkg file C: quantile.c (will be coming) Please report any problem or suggestion at jaesub@head.cfa.harvard.edu
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.0/readme -- 1.5 Кб -- 10.02.2004
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7112. http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.0/example.pro
range = [ 0.3 ,8.0] ; 0.3 - 8.0 keV frac = [0.25, 0.33, 0.50, 0.67, 0.75] ;--------------------------------------------------------- ; example of simple source photons src = randomu ( seed , 100 ) * ( range [1]- range [0]) + range [0] qt = quantile( frac , src , range = range , err_qt = err_qt ) print , frac print ,qt print , ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.0/example.pro -- 1.7 Кб -- 10.02.2004
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.1/example.pro -- 1.7 Кб -- 10.02.2004
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7113. http://hea-www.harvard.edu/PINTofALE/papers/lkd_2004_itcc.ps.gz
Package for the Interactive Analysis of Line Emission: MarkovґChain and Monte Carlo Methods LiWei Lin, Vinay L. Kashyap, Jeremy J. Drake Smithsonian Astrophysical Observatory 60 Garden St., Cambridge, MA 02138 pintofale@head.cfa.harvard.edu Abstract We describe the implementation of Monte Carlo methґ ods in the Package for Interactive Analysis of Line Emisґ sion (PINTofALE), which is a collection of IDLґbased proґ grams designed to analyze astrophysical spectra. ... The analysis of XUV emission lines. ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/papers/lkd_2004_itcc.ps.gz -- 373.2 Кб -- 24.01.2004
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7114. http://hea-www.harvard.edu/~pgreen/Papers/ChaMP_X2.pdf
... Utilizing only near - on-axis X-ray - bright sources (to avoid problems caused by incompleteness and the Eddington bias), we derive the log N log S relation in soft (0.5 - 2 keV) and hard (2 - 8 keV) energy bands. ... Subject headings: galaxies: active -- surveys -- X-rays: galaxies On-line material: color figures 1. ... In this paper we present the results of X-ray source properties by producing the log N log S relation and X-ray colors and by comparing with data at other wavelengths. ... 1022 cmР2...
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Ссылки http://hea-www.harvard.edu/~pgreen/Papers/ChaMP_X2.pdf -- 698.7 Кб -- 22.01.2004
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7115. http://hea-www.harvard.edu/~pgreen/Papers/ChaMP_X1.pdf
... I. FIRST X-RAY SOURCE CATALOG D.-W. Kim, R. A. Cameron, J. J. Drake, N. R. Evans, P. Freeman, T. J. Gaetz, H. Ghosh, P. J. Green, F. R. Harnden, Jr., ... On the other hand, the chance of missing a real source is rather complex, depending on the source counts, off-axis distance (or PSF), and background rate. ... To take full advantage of the rich data set available in the Chandra public archive, we have initiated a serendipitous X-ray source survey, the Chandra Multiwavelength Project (ChaMP). ...
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Ссылки http://hea-www.harvard.edu/~pgreen/Papers/ChaMP_X1.pdf -- 1387.3 Кб -- 22.01.2004
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7116. http://hea-www.harvard.edu/~pgreen/dec2903.pdf
... rass rass rass rass rass pspc pspc pspc pspc rass rass rass rass OBSID HOSC Time Event ------------------------------------------ 2003 :363:09:31:37.589 MANV -- start 2003 :363:09:50:28.212 SIM -- start 2003 :363:09:57:08.343 MANV - end 2003 :363:09:57:08.343 SIM - end 2003 :363:10:00: 00.000 COM -- start 04918 2003 :363:10:01:38.343 M87 -- start 2003 :363:11:24:58.343 M87 -- end ...
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Ссылки http://hea-www.harvard.edu/~pgreen/dec2903.pdf -- 52.8 Кб -- 22.12.2003
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7117. http://hea-www.harvard.edu/~pgreen/refresponse.txt
REFEREE REPORT: %% %% %% As made clear by the title of the paper and the observational %% evidence presented, the authors believe that the correct %% identification of HS1216+5032 is as a physical quasar pair, albeit %% with one component showing the rather unusual combination of %% BAL troughs and significant radio luminosity. ... Removed most of the discussion of dark lenses and cosmology, and deleted the section on BALQSOs. ... The paper now totals 5.5 pages, down from 10. ...
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Ссылки http://hea-www.harvard.edu/~pgreen/refresponse.txt -- 7.1 Кб -- 14.12.2003
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7118. http://hea-www.harvard.edu/~alexey/emulateapj/apjfonts.sty
... MM: I found experimantally that textfont9 is the first unused font) \def\@tempa{9} % Tell TeX where cmmi is. ... 026A % \ mathcode `\}= 5267 \ mathchardef \ldotp= 602E % ldot as a punctuation mark % Put back the missing lowercase Greek characters. \ mathchardef \alpha= 0\@ tempa 0B \ mathchardef \beta= 0\@ tempa 0C \ mathchardef \gamma= 0\@ tempa 0D \ mathchardef \delta= 0\@ tempa 0E \ mathchardef \epsilon= 0\@ tempa 0F \ mathchardef \zeta= 0\@ tempa 10 \ mathchardef \eta= 0\@ tempa 11 \ ...
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Ссылки http://hea-www.harvard.edu/~alexey/emulateapj/apjfonts.sty -- 13.2 Кб -- 04.11.2003
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7119. http://hea-www.harvard.edu/~pgreen/post_FOS_WWW/paper.ps
To appear in ApJS Preprint typeset using L A T E X style emulateapj EMISSION LINE PROPERTIES OF AGN FROM A POST-COSTAR FOS HST SPECTRAL ATLAS Joanna K. Kuraszkiewicz, Paul J. Green Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge ... EMISSION LINE MEASUREMENTS In Table 4 we present the rest frame emission line mea- surements for one example object NGC 3516 (spectrum 1106+7234oe). ... 8 Emission Line Properties of AGN from a post-COSTAR FOS HST Spectral Atlas Fig. ...
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Ссылки http://hea-www.harvard.edu/~pgreen/post_FOS_WWW/paper.ps -- 1305.5 Кб -- 06.10.2003
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7120. http://hea-www.harvard.edu/CHAMP/PUBLICATIONS/jds_paper03FINAL.ps
... Printed DISCOVERY A z 4.93, XнRAY -- SELECTED QUASAR THE CHANDRA MULTIWAVELENGTH PROJECT (ChaMP) John Silverman, Paul Green, 1 DongнWoo Kim, 1 Belinda J. Wilkes, 1 Robert A. Cameron, 1 David Morris ... Infante, Paul Smith, 7 Buell T. Jannuzi, 8 Smita Mathur Received January accepted 2002 February published 2002 March ABSTRACT present Xнray and optical observations of CXOMP J213945.0 # 234655 , a highнredshift ) quasar z discovered through ... CHANDRA DISCOVERY 4.93 QUASAR 1.- ...
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Ссылки http://hea-www.harvard.edu/CHAMP/PUBLICATIONS/jds_paper03FINAL.ps -- 458.4 Кб -- 23.09.2003
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