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7301. http://hea-www.harvard.edu/~dburke/PDL/hogg/distance_modulus
Compare to fig 4, of Hogg, D. W., Distance measures in cosmology , # astro -ph/9905116 # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is NOT irrelevant here! my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0, h0 = 100.0 ); my $b = Astro :: Cosmology - new ( matter = 0.05, lambda = 0.0, h0 = Astro::Cosmology v" . Astro::Cosmology->version . ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/hogg/distance_modulus -- 2.2 Кб -- 08.08.2001
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7302. http://hea-www.harvard.edu/~dburke/PDL/hogg/proper_motion
Compare to fig 1, of Hogg, D. W., Distance measures in cosmology , # astro -ph/9905116 # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is irrelevant here my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0 , h0 = 0.0 ); my $b = Astro :: Cosmology - new ( matter = 0.05, lambda = Astro::Cosmology v" . Astro::Cosmology->version . ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/hogg/proper_motion -- 2.1 Кб -- 08.08.2001
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7303. http://hea-www.harvard.edu/~dburke/PDL/hogg/comoving_volume
Compare to fig 5, of Hogg, D. W., Distance measures in cosmology , # astro -ph/9905116 # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is irrelevant here my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0 , h0 = 0.0 ); my $b = Astro :: Cosmology - new ( matter = 0.05, lambda = Astro::Cosmology v" . Astro::Cosmology->version . ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/hogg/comoving_volume -- 2.2 Кб -- 08.08.2001
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7304. http://hea-www.harvard.edu/~dburke/PDL/hogg/luminosity_distance
Compare to fig 3, of Hogg, D. W., Distance measures in cosmology , # astro -ph/9905116 # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is irrelevant here my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0 , h0 = 0.0 ); my $b = Astro :: Cosmology - new ( matter = 0.05, lambda = Astro::Cosmology v" . Astro::Cosmology->version . ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/hogg/luminosity_distance -- 2.1 Кб -- 08.08.2001
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7305. http://hea-www.harvard.edu/~dburke/PDL/hogg/lookback_time
Compare to fig 6, of Hogg, D. W., Distance measures in cosmology , # astro -ph/9905116 # # Note: # currently only do the lookback time, not the age of the universe # curves # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is irrelevant here my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0 , h0 = 0.0 ); my $b = Astro::Cosmology v" . Astro::Cosmology->version . ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/hogg/lookback_time -- 2.3 Кб -- 08.08.2001
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7306. http://hea-www.harvard.edu/~dburke/PDL/hogg/angular_diameter
Compare to fig 2, of Hogg, D. W., Distance measures in cosmology , # astro -ph/9905116 # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is irrelevant here my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0 , h0 = 0.0 ); my $b = Astro :: Cosmology - new ( matter = 0.05, lambda = Astro::Cosmology v" . Astro::Cosmology->version . ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/hogg/angular_diameter -- 2.1 Кб -- 08.08.2001
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7307. http://hea-www.harvard.edu/~dburke/PDL/cpt/differential_comoving_volume
page 514, of # Carroll, Press Turner, ARAA, 1992, 30, 499-542 # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is irrelevant here my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0 , h0 = 0.0 ); my $b = Astro :: Cosmology - new ( matter = 0.1, lambda = 0.0 , h0 = 0.0 ); my $c = Astro :: Cosmology - ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/cpt/differential_comoving_volume -- 2.6 Кб -- 08.08.2001
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7308. http://hea-www.harvard.edu/~dburke/PDL/cpt/angular_diameter
page 512, of # Carroll, Press Turner, ARAA, 1992, 30, 499-542 # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is irrelevant here my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0 , h0 = 0.0 ); my $b = Astro :: Cosmology - new ( matter = 0.1, lambda = 0.0 , h0 = 0.0 ); my $c = Astro :: Cosmology - ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/cpt/angular_diameter -- 2.6 Кб -- 08.08.2001
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7309. http://hea-www.harvard.edu/~dburke/PDL/cpt/lookback_time
page 512, of # Carroll, Press Turner, ARAA, 1992, 30, 499-542 # use strict; use PDL; use PDL::Graphics::PGPLOT::Window; use Astro :: Cosmology ; # cosmologies - h0 is irrelevant here my $a = Astro :: Cosmology - new ( matter = 1.0, lambda = 0.0 , h0 = 0.0 ); my $b = Astro :: Cosmology - new ( matter = 0.1, lambda = 0.0 , h0 = 0.0 ); my $c = Astro :: Cosmology - ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/cpt/lookback_time -- 2.6 Кб -- 08.08.2001
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7310. http://hea-www.harvard.edu/~dburke/PDL/Changelog-0.90
Release 0.90 2001-08-04 Doug Burke <djburke@cpan.org> - added more tests (thanks to Brad Holden) - more internal adjustments to the distribution (no functional changes). Hopefully more compatible with CPAN now. Release 0.84 2001-08-02 Doug Burke <djburke@cpan.org> - documentation now in Cosmology.pod so that CPAN will pick it up. No functional change to v0.83. Release 0.83 2001-08-01 Doug Burke <djburke@cpan.org> - Added version method, renamed string method to stringify. ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/Changelog-0.90 -- 1.8 Кб -- 04.08.2001
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7311. http://hea-www.harvard.edu/~dburke/PDL/README-Astro-Cosmology-0.90
... History ------- 04 Aug 2001 v0.90 more reorganisation. Hopefully CPAN-friendly now more tests (thanks Brad) 02 Aug 2001 v0.84 minor reorganisation, no change to code or docs 01 Aug 2001 v0.83 added version method, renamed string to stringify further documentation improvements improvements to test suite (thanks Brad) 29 Jul 2001 v0.82 added STERADIAN to constants improved documentation 28 Jul 2001 v0.81 renamed to Astro :: Cosmology removed need for PDL :: Astro :: Constants 19 Jul ...
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Ссылки http://hea-www.harvard.edu/~dburke/PDL/README-Astro-Cosmology-0.90 -- 6.2 Кб -- 04.08.2001
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7312. http://hea-www.harvard.edu/PINTofALE/doc/LINEID.howto
... RD_LINE: No lines in this wavelength range .% ... WVL [Ang] MATCH Z ION FLUX +- Tmax 0-----------------------------------------------------1 22.1000 : 22.1012 O VII 0.17841 +- 0.000 6.30 22.1000 : 22.1020 O VI 2.0272e-06 +- 0.000 6.25 22.1000 : -22.0970 Ca XVII 2.5012e-06 +- 0.000 6.70 22.1000 : -22.1060 Ca XVI 5.1657e-07 +- 0.000 6.60 22.1000 : -22.0939 Ar XVII 1.1069e-07 +- 0.000 7.30 22.1000 : 22.0931 Fe XXIV 3.9956e-08 +- 0.000 7.30 ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/doc/LINEID.howto -- 16.8 Кб -- 04.07.2001
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7313. http://hea-www.harvard.edu/~jcm/asc/docs/ps/ncoords.ps
... For a given detector, there may be more than one chip, each with its own chip coordinate system. ... 15 Table 2: ACIS Chip corner locations in ACIS ґI LSI coordinates Chip Corner CPC coords ACIS ґI LSI coords I0 LL ( 0.0 , 0.0 , 0.0 ) (2.361, ґ26.484, 23.088) LR (24.58, 0.0 , 0.0 ) (1.130, ґ26.546, ґ1.458) UR (24.58, 24.58, 0.0 ) (ґ0.100, ґ2.001, ґ1.458) UL ( 0.0 , 24.58, 0.0 ) (1.130, ґ1.939, 23.088) I1 LL ( 0.0 , 0.0 , 0.0 ) (1.130, 23.086, ґ1.458) LR (24.58, 0.0 , ...
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Ссылки http://hea-www.harvard.edu/~jcm/asc/docs/ps/ncoords.ps -- 812.5 Кб -- 13.05.2001
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7314. http://hea-www.harvard.edu/~pgreen/elvis_3Dmodel.pdf
F 7 ?Q e@ d і %$ ) !$ 2 d ї) ?1 R q ') ?@ ?" p) GB C) y@ ї$ ?Q r? 26 2& G" I" ?" Q 2 " G" hu Ag 6 ?" CB ?F 26 ) (s f@ '" S) ps HQ HB ?і % Cє !@ ...
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Ссылки http://hea-www.harvard.edu/~pgreen/elvis_3Dmodel.pdf -- 184.2 Кб -- 07.05.2001
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7315. http://hea-www.harvard.edu/~bradw/cv/papers/RSIspectrometer.pdf
Low energy x-ray spectrometer P. Beiersdotfer B. J. Wargelina) for an electron beam ion trap University of California, Lawrence Livermore National Laboratory, Livermore, Catifornia 94550 University of California, Department of Physics at?d Space Sciences Laboratory, Berkeley, California 94720 (Received 20 August 1993; acceptedfor publication 18 October 1993) A flat-crystal spectrometerfor analyzing ultrasoft x rays in the wavelength region 10-25 A was constructed for use on an electron beam ion trap. ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/RSIspectrometer.pdf -- 620.3 Кб -- 03.04.2001
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7316. http://hea-www.harvard.edu/RD/funtools/funcalc.sed
# cc <foo.c> 2>&1 | sed -n -f funauto.sed # Linux gcc (and others) s/.*`\([^)]*\)' undeclared (first use in this function).*/\1/p # Solaris cc s/.*undefined symbol: \([^)]*\)/\1/p # Dec Alpha/OSF cc s/.*In this statement, "\([^)]*\)" is not declared.*/\1/p # SGI cc s/.*The identifier "\([^)]*\)" is undefined.*/\1/p
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Ссылки http://hea-www.harvard.edu/RD/funtools/funcalc.sed -- 1.3 Кб -- 02.03.2001
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/funtools/funcalc.sed -- 1.3 Кб -- 02.03.2001
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/saord/funtools/funcalc.sed -- 1.3 Кб -- 02.03.2001
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7317. http://hea-www.harvard.edu/~bradw/cv/papers/HR1099.ps
... Printed in U.S.A. ENHANCED NOBLE GASES IN THE CORONAE OF ACTIVE STARS Jeremy J. Drake, 1 Nancy S. Brickhouse, 1 Vinay Kashyap, 1 J. Martin Laming, 2 David P. Huenemoerder, 3 Randall Smith, 1 and Bradford J. Wargelin 1 Received 2000 October 10; accepted 2000 November 27; published 2001 February 12 ABSTRACT We have analyzed Chandra HighґEnergy Transmission Grating spectra of the active RS CVn--type binary V711 Tauri (HR 1099; HD 22468) in order to examine the chemical composition of its coronae. ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/HR1099.ps -- 335.8 Кб -- 16.02.2001
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7318. http://hea-www.harvard.edu/~bradw/cv/papers/HR1099.pdf
... Printed in U.S.A. ENHANCED NOBLE GASES IN THE CORONAE OF ACTIVE STARS Jeremy J. Drake,1 Nancy S. Brickhouse,1 Vinay Kashyap,1 J. Martin Laming,2 David P. Huenemoerder,3 Randall Smith,1 and Bradford J. Wargelin1 Received 2000 October 10; accepted 2000 November 27; published 2001 February 12 ABSTRACT We have analyzed Chandra High-Energy Transmission Grating spectra of the active RS CVnґtype binar y V711 Tauri (HR 1099; HD 22468) in order to examine the chemical composition of its coronae. ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/HR1099.pdf -- 184.9 Кб -- 16.02.2001
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7319. http://hea-www.harvard.edu/PINTofALE/papers/d_MM_palermo.ps.gz
... Milestones in the Study of Stellar Coronae 1940 Coronal lines Temperatures of ?million K diagnosed from identified forbidden Fe lines 1949 Rocket Flight First solar Xґrays detected 1960 Rocket Flight Pinhole camera produces first Xґ ray image of solar corona 1965 Rocket Flights First images of solar coronal structure with grazing incidence optics 1973 Skylab High resolution EUV/Xґ ray images of ... Why are there no orderґofґmagnitude Xґray activity cycles in these active stars?' ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/papers/d_MM_palermo.ps.gz -- 88.0 Кб -- 12.02.2001
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7320. http://hea-www.harvard.edu/PINTofALE/pro/did2emis2em.pro
pro did2emis2em, idstr ,edens, fluxes = fluxes ,deblend=deblend, DEM = DEM , logT = logT ,$ ldir = ldir ,NH=NH, EMs = EMs ,FXs=FXs,xtitle=xtitle,ytitle=ytitle,$ title=title,verbose=verbose,n_e=n_e, _extra=e ;+ ;procedure did2emis2em ; for a specified line, read in emissivities at various densities, ; compute fluxes , and invert to get emission measure estimates at ; each density. ; ;syntax ; did2emis2em, idstr ,edens, fluxes = ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/did2emis2em.pro -- 12.5 Кб -- 09.02.2001
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