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7021. http://hea-www.harvard.edu/~fine/POV/src/water_bottle.pov
declare water_bottle = union { torus { 1.25 0.2 translate 0.2 *y } cylinder { 0, 0.2 ,0 0,5,0 1.45 texture { whitepaint } //texture { //pigment { image_map { gif irtc-logo-wide.gif // map_type 2 transmit 0,1 once } // rotate 180*y scale 1,2,1 translate 0,1.75,0 } //finish { diffuse 0.8 specular 0.2 } //} } torus { 0.75 0.7 translate 5*y } difference { ...
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Ссылки http://hea-www.harvard.edu/~fine/POV/src/water_bottle.pov -- 3.5 Кб -- 01.11.2004
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7022. http://hea-www.harvard.edu/~fine/POV/src/push_pin.demos.pov
default { finish { ambient 0.4 } } camera { up 0, 1, 0 right 1, 0, 0 location -4,2,1 look_at 0,0,0 angle 20 } #include colors.inc # declare chrome = texture { pigment { color rgb 0.6,0.6,0.6 } finish { specular 0.5 reflection 0.7 roughness 0.005 metallic } } # declare clearred = texture { pigment { color rgbf 0.75,0,0, 0.7 } ...
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Ссылки http://hea-www.harvard.edu/~fine/POV/src/push_pin.demos.pov -- 2.6 Кб -- 01.11.2004
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7023. http://hea-www.harvard.edu/~fine/POV/src/push_pin.pov
#declare push_pin = union { cylinder { <0,0,-0.3> <0,0,0.25> 0.018 texture { chrome } } sphere { <0,0,0> 0.05 scale <1,1,0.1 > translate <0,0,-0.3> texture { chrome } } cone { <0,0,0.25> 0.018 <0,0,0.375> 0 texture { chrome } } difference { sphere { <0,0,0.01> 0.17 scale <1,1,0.8> } box { <-1,-1,0> <1,1,1> } } cylinder { <0,0,-0.01> <0,0,-0.4> .09 } cone { <0,0,-0.375> .11 <0,0,-0.44> .125 } difference { sphere { <0,0,0.275> 0.3 } box { <-1,-1,0> <1,1,1> } translate <0,0,-0.44> } interior { ior 1.5 } }
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Ссылки http://hea-www.harvard.edu/~fine/POV/src/push_pin.pov -- 1.5 Кб -- 01.11.2004
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7024. http://hea-www.harvard.edu/~fine/POV/src/bolt_cup.demos.pov
default { finish { ambient 0.4 } } camera { up 0, 1, 0 right 1, 0, 0 location -4,9,-16 look_at 0,2,0 angle 20 } #include colors.inc # declare greenpaint = texture { pigment { color rgb 0 1 0 } finish { specular 0 reflection 0 diffuse 0.7 } } # declare offwhitepaint = texture { pigment { color rgb 0.9 0.9 0.8 } finish { specular 0 reflection 0 diffuse ...
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Ссылки http://hea-www.harvard.edu/~fine/POV/src/bolt_cup.demos.pov -- 2.2 Кб -- 01.11.2004
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7025. http://hea-www.harvard.edu/~fine/POV/src/pov_pen.pov
ink pen #declare pov_pen = union { cylinder { 0,0,0 4.875,0,0 0.14 texture { whiteplastic } } cone { 0,0,0 0.14 - 0.125 ,0,0 0.12 texture { blueplastic } } cone { - 0.125 ,0,0 0.12 -0.375,0,0 0.09 texture { blueplastic } } difference { sphere { 4.71,0,0 0.22 } box { 4.875,-1,-1 4,1,1 } texture { blueplastic } } ...
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Ссылки http://hea-www.harvard.edu/~fine/POV/src/pov_pen.pov -- 3.0 Кб -- 01.11.2004
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7026. http://hea-www.harvard.edu/~fine/POV/src/pov_pen.demos.pov
default { finish { ambient 0.4 } } camera { up 0, 1, 0 right 1, 0, 0 location -4,4,-20 look_at 2,0,0 angle 20 } #include colors.inc #include metals.inc # declare dkbeigepaint = texture { pigment { color rgb 0.6,0.5,0.4 } finish { diffuse 0.8 specular 0.2 } } # declare whiteplastic = texture { pigment { color rgb 0.95,0.95,0.95 } ...
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Ссылки http://hea-www.harvard.edu/~fine/POV/src/pov_pen.demos.pov -- 2.8 Кб -- 01.11.2004
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7027. http://hea-www.harvard.edu/~fine/POV/src/bolt_cup.pov
include functions.inc //coffee cup #declare bolt_cup = union { //cup difference { cylinder { 0,0.6,0 0,3.75,0 1.625 } cylinder { 0,0.9,0 0,3.8,0 1.375 } cone { 0,3,0 1.3 0,3.8,0 1.5 } //round the transition between cone and cylinder #declare trans_rad=1; //intersection of cone and cylinder above occurs at y=3.3 difference { ...
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Ссылки http://hea-www.harvard.edu/~fine/POV/src/bolt_cup.pov -- 4.3 Кб -- 01.11.2004
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7028. http://hea-www.harvard.edu/~pgreen/vita_short04.ps
VITA: PAUL J. GREEN Harvard-Smithsonian Center for Astrophysics, MS-4 60 Garden St., Cambridge, MA 02138 Phone: 617-495-7057 pgreen@cfa.harvard.edu http://hea-www.harvard.edu/~ pgreen/ EDUCATION: Ph.D. in Physics, 1992 , University of Washington - \Faint High Latitude Carbon Stars , Advisor: Bruce Margon M.S. in Physics, 1989, University of Washington B.A. in Physics, 1981, Oberlin College RESEARCH EMPLOYMENT: Astrophysicist ...
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Ссылки http://hea-www.harvard.edu/~pgreen/vita_short04.ps -- 103.2 Кб -- 18.10.2004
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7029. http://hea-www.harvard.edu/PINTofALE/ardb/Astro-E2_xrs_xis_ao1.par
... Typically, a 2-temperature ; model is used. ... A] Read in line cooling emissivities and calculate line intensities help,lconf,linint ;B] Read in line cooling emissivities and calculate line intensities help,cconf,conint ;C] Correct for inter-stellar absorption help,ltau,ltrans,linflx,ctau,ctrans,conflx ;D] Bin spectra and fold in effective area EMAX = !fundae.kevang/!WMIN EMIN = !fundae.kevang/!WMAX dnrg = float((EMAX-EMIN)/nwbin) ; bin size egrid = findgen(nwbin+1L)*dnrg+EMIN ;...
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Ссылки http://hea-www.harvard.edu/PINTofALE/ardb/Astro-E2_xrs_xis_ao1.par -- 17.1 Кб -- 15.10.2004
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7030. http://hea-www.harvard.edu/AstroStat/HEAD2004/presentation_aneta.pdf
Sherpa Aneta Siemiginowska 1 SHERPA CIAO's Modeling and Fitting Application Aneta Siemiginowska CXC Astrostatistics Workshop, HEAD meeting , New Orleans, Septemter 2004 Sherpa Aneta Siemiginowska 2 Modeling and Fitting Software XSPEC - analysis of 1D X-ray data (imaging + grating) ISIS and Pint of Ale- primarily for analysis of highresolution (ie grating) X-ray data ... Jointmode data: spatialspectral, spatialtiming Use scripts based on Sherpa only commands. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/presentation_aneta.pdf -- 740.0 Кб -- 14.10.2004
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/presentation_aneta.pdf -- 740.0 Кб -- 14.10.2004
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/presentation_aneta.pdf -- 740.0 Кб -- 14.10.2004
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7031. http://hea-www.harvard.edu/~pgreen/BOOTES/pgreen2.ps
... Date: September 30, 2003 Category: Active Galaxies The Hardest X-ray Sources Unveiled PI: Paul J. Green Status: P Aфl.: ... NOAO Chris Kochanek Bill Forman Arjun Dey Brian McNamara Kate Brand Abstract of Scienti c Justi cation (will be made publicly available for accepted proposals): The hard Cosmic X-ray Background (CXRB) has been resolved into point sources by the Chandra deep eld exposures as predominantly low luminosity objects at z < 1, and the nature of these AGNs is not well understood. ...
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Ссылки http://hea-www.harvard.edu/~pgreen/BOOTES/pgreen2.ps -- 627.3 Кб -- 28.09.2004
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7032. http://hea-www.harvard.edu/~pgreen/BOOTES/nprop29.sty
... Page sizes are at the end of the file. \ def \baselinestretch{0.98} % Tighten up baselines a little. \ def \ps@kpprophead{\ def \@oddfoot{}\ def \@evenfoot{} \ def \@oddhead{\ hbox to\ textwidth {\small\sl \prop@phead \ ifx \@ empty \@rcptdate\phantom{, received Dec 31 1999} \ else , received \@rcptdate\fi \ hfill Page \thepage \ hfill \prop@pidbox}}\let\@evenhead\@oddhead \ ... Phys.~A}} \def\physrep{\ref@jnl{Phys.~Rep.}} \def\physscr{\ref@jnl{Phys.~Scr}} \def\planss{\ref@jnl{Planet.~ ...
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Ссылки http://hea-www.harvard.edu/~pgreen/BOOTES/nprop29.sty -- 29.5 Кб -- 28.09.2004
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7033. http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_jchiang.txt
Questions to Jim Chiang (paraphrasing): From Randall Smith: Q: Have you considered parallelizing the calculations to make the execution for the fitting faster? A: The present code hasn't been written with parallelization in mind, but this is something worth considering. Certain parts of the calculation have been factored out and precomputed outside of the parallelization. ... Where does it come from? A: It comes from the n_k! that you see in the Poisson likelihood (viz. p11) ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_jchiang.txt -- 1.6 Кб -- 22.09.2004
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_jchiang.txt -- 1.6 Кб -- 22.09.2004
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_jchiang.txt -- 1.6 Кб -- 22.09.2004
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7034. http://hea-www.harvard.edu/AstroStat/HEAD2004/abstract_jchiang.txt
Challenges in Analyzing Data from the GLAST Large Area Telescope J. Chiang (GLAST Science Support Center, UMBC/GSFC) The Large Area Telescope (LAT) aboard GLAST promises greater than an order of magnitude better sensitivity, a much larger field-of-view, significantly better angular resolution, and broader energy coverage than its predecessor in the gamma-ray band, EGRET. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/abstract_jchiang.txt -- 2.6 Кб -- 21.09.2004
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/abstract_jchiang.txt -- 2.6 Кб -- 21.09.2004
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/abstract_jchiang.txt -- 2.6 Кб -- 21.09.2004
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7035. http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_sourlas.pdf
... r !E r 1y " 'P p h -15.5 -15.0 -14.5 log10(Flux) -14.0 -13.5 -13.0 0.0 BU ЕA T ? ... е !f C ?ч чцх "b WP DG Еs r db Wf ? ... 0.2 0.0 0.5 1.0 log10(N S) 1.5 2.0 2.5 3.0 0.4 1-pi(.) 0.6 0.8 i ЖЕ ЕЖ Number of Sources above Flux S Number of Sources above Flux S З ЗЗЗЗЗ ЗЗЗ ЗЗЗЗЗ ЗЗЗ ЗЗЗЗЗ ЗЗЗ З ЗЗЗЗЗЗ З ЗЗЗЗЗЗ ЗЗ З З ЗЗЗЗЗ З ЗЗЗЗЗ ЗЗЗЗЗ ЗЗЗ ЗЗЗЗ ЗЗЗ ЗЗЗ ЗЗЗ ЗЗЗ ЗЗ ЗЗ ЗЗ ЗЗ З З З З З З З 0 5 10 15 20 25 -12 0.5 1.0 1.5 2.0 2.5 3.0 З ЗЗЗЗЗ ЗЗЗ ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_sourlas.pdf -- 486.2 Кб -- 20.09.2004
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/poster_sourlas.pdf -- 486.2 Кб -- 20.09.2004
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/poster_sourlas.pdf -- 486.2 Кб -- 20.09.2004
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7036. http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_bestmethod.txt
... The person next to Brad (don't recall who it was) spoke to what an important general question that was. But I also,later, thought of a slightly better answer for Brad: If you DO have some kind of good parametrized physical model (e.g. light-curve formed by two stars of type X and Y, at such and such inclination, with hot-spot and oddly stretched atmosphere, etc etc) then "forward fitting" to make a good likelihood ratio is ALWAYS going to be the most powerful, most sensitive test. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_bestmethod.txt -- 1.9 Кб -- 16.09.2004
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_bestmethod.txt -- 1.9 Кб -- 16.09.2004
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_bestmethod.txt -- 1.9 Кб -- 16.09.2004
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7037. http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_posterior.txt
From Keith Arnaud: The reactions I recall to my comments about saving posterior distributions were that Jeff Scargle was very sceptical about using other peoples posterior distributions as priors since it would lead to errors propagating. He preferred neutral priors. ... If you took posteriors on two parameters from different experiments and combined them as a prior and the two experiments themselves used the same prior then you would include this prior twice. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_posterior.txt -- 1.5 Кб -- 16.09.2004
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_posterior.txt -- 1.5 Кб -- 16.09.2004
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_posterior.txt -- 1.5 Кб -- 16.09.2004
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7038. http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_badastrostat.txt
Randall Smith> A "Bad AstroStatistics" web page will be a very useful thing. People will read it. They will not only understand the issues better, but it will also be a useful resource for referees. [cheers, hosannas, enthusiastic clapping] ______________________________________________________________________ paraphrased by Vinay Kashyap
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_badastrostat.txt -- 1.3 Кб -- 15.09.2004
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_badastrostat.txt -- 1.3 Кб -- 15.09.2004
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_badastrostat.txt -- 1.3 Кб -- 15.09.2004
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7039. http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_consult.txt
... A panel could visit it on a regular basis and answer questions. ... David van Dyk (UC Irvine)> Not practical, because it is hard to understand the problem until one spends a lot of time thinking about it, and it may be months before one finds the time to do so and give a useful response. Ashish Mahabal> Also, such websites often get the same questions again and again. ... Besides, questions typically get asked when people want qucik response, say in 2-3 days. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/discuss_consult.txt -- 2.1 Кб -- 15.09.2004
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_consult.txt -- 2.1 Кб -- 15.09.2004
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/discuss_consult.txt -- 2.1 Кб -- 15.09.2004
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7040. http://hea-www.harvard.edu/AstroStat/HEAD2004/abstract_meng.txt
An Introductory Overview of Statistical Methods for Discrete Time Series Xiao-li Meng (Harvard University) A number of statistical problems encounted in astrophysics are concerned with discrete time series, such as photon counts with variation in source intensity over time. This talk provides an introductory overview of the current state-of-the-art methods in statistics, including Bayesian methods aided by Markov chain Monte Carlo, for modeling and analyzing such data. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/abstract_meng.txt -- 1.6 Кб -- 13.09.2004
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/abstract_meng.txt -- 1.6 Кб -- 13.09.2004
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/astrostat/HEAD2004/abstract_meng.txt -- 1.6 Кб -- 13.09.2004
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