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6241. http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/grid.pl
... For the model names and their parameters, refer Sherpa or # xspec manual. ... The file will contains 2+n columns where n is the number of "frac" # you request. ... files from command line use Getopt::Long; GetOptions( model=s = \$model, range=s = \$range, frac =s = \$ frac , par1=s = \$par1, par2=s = \$par2, etcp =s = \$ etcp , arf =s = \$ arf , rmf =s = \$ rmf , full = \$full, sherpa =s = \$ sherpa , gridsl=s = \$gridsl, ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/grid.pl -- 9.2 Кб -- 14.01.2006
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/grid.pl -- 9.2 Кб -- 14.01.2006
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/grid.pl -- 9.2 Кб -- 14.01.2006
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6242. http://hea-www.harvard.edu/PINTofALE/ardb/Suzaku_ao2.par
... know where your local PIMMS installation ; is to do this. rd_pimms_file,get_pimms_file('chandra','acis-i',pdir=pimmsdir),$ acisi_ effar ,acisi_wvlar,/wave ; fold in effective area acisi_wmin=12.3985/acisi_emax acisi_wmax=12.3985/acisi_emin os=sort(acisi_wvlar) acisi_wvlar=acisi_wvlar[os] acisi_ effar =acisi_ effar [os] ; lwvl=abs(ae2_lstr.WVL) ow_lacisi=where(lwvl ge acisi_wmin and lwvl le acisi_wmax) effar =(interpol(acisi_ ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/ardb/Suzaku_ao2.par -- 21.7 Кб -- 06.01.2006
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6243. http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/rdrdb.pro
JaeSub Hong, 2002-2005, version 1.5 ; Please report any problem or suggestion at jaesub@head.cfa.harvard.edu ; ; ; - consider any line starting with # comments ; - speed up by pre-setting array size (default 1000, change by n_step) ; function rdrdb, filename, $ noheader=noheader, comment = comment , $ data = data , sep = sep , struct = struct , recycle=recycle, $ names = names , units=units, n_step=n_step if not keyword_set( ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/rdrdb.pro -- 3.9 Кб -- 09.12.2005
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/rdrdb.pro -- 3.9 Кб -- 09.12.2005
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/rdrdb.pro -- 3.9 Кб -- 09.12.2005
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6244. http://hea-www.harvard.edu/AstroStat/BEHR/tpark_6y.ps
... New Bayesian Method Computing Posterior Distributions of Hardness Ratios: . ... Hardness True Point estimates 95% error bar Method ratio value mode mean lower upper R 1 1.0 0.3932 1.6068 Classical C 0 0.0 ґ0.2635 0.2635 High method HR 0 0.0 ґ0.3034 0.3034 counts R 1 0.9376 1.0315 0.5622 1.5729 Bayesian C 0 0.0000 0.0000 ґ0.2590 0.2590 method HR 0 0.0000 0.0004 ґ0.2110 0.2123 R 1 1.0 ґ1.8070 3.8070 Classical C 0 0.0 ґ1.2191 1.2191 Low method HR 0 0.0 ґ1.4035 1.4035 ...
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Ссылки http://hea-www.harvard.edu/AstroStat/BEHR/tpark_6y.ps -- 323.8 Кб -- 30.11.2005
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/BEHR/tpark_6y.ps -- 323.8 Кб -- 30.11.2005
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/BEHR/tpark_6y.ps -- 323.8 Кб -- 30.11.2005
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6245. http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/grid_line.pl
... For the model names and their parameters, refer Sherpa or # xspec manual. ... source 1 = $cmod fakeit 1 K=get_pflux(1,[$low,$high]) ()=set_par( $par , value ,K.value*$reln) $rmodel EOF } if ( defined $raw) { $x_axe = channels ; $time = 1000000 unless defined $time; $timeset = fakeit time = $time ; $suffix = _raw ; $rerun .= $timeset\nfakeit 1\n ; } else ... 1\n ; } ($input = EOFINPUT ) =~ s/^\t//gm; paramprompt off INSTRUMENT 1 = RSP[instrumentA] instrumentA. rmf = $ ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/grid_line.pl -- 9.8 Кб -- 16.11.2005
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/grid_line.pl -- 9.8 Кб -- 16.11.2005
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/grid_line.pl -- 9.8 Кб -- 16.11.2005
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6246. http://hea-www.harvard.edu/~bradw/cv/papers/FeCX.ps.gz
CHARGEґEXCHANGE SPECTRA OF HYDROGENIC AND HeґLIKE IRON B. J. Wargelin, 1 P. Beiersdorfer, 2 P. A. Neill, 3 R. E. Olson, 4 and J. H. Scofield 2 Received 2005 April 27; accepted 2005 July 31 ABSTRACT We present Hґlike Fe xxvi and Heґlike Fe xxv chargeґexchange spectra resulting from collisions of highly charged iron with N 2 gas at an energy of #10 eVamu #1 in an electron beam ion trap. ... Line energy centroids, appropriate for both the beamґon and beamґoff phases, are listed in Table 1. ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/FeCX.ps.gz -- 395.1 Кб -- 15.11.2005
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6247. http://hea-www.harvard.edu/~bradw/cv/papers/FeCX.pdf
... Printed in U.S.A. CHARGE-EXCHANGE SPECTRA OF HYDROGENIC AND He-LIKE IRON B. J. Wargelin,1 P. Beiersdorfer,2 P. A. Neill,3 R. E. Olson,4 and J. H. Scofield2 Received 2005 April 27; accepted 2005 July 31 ABSTRACT We present H-like Fe xxvi and He-like Fe xxv charge-exchange spectra resulting from collisions of highly charged iron with N2 gas at an energy of $10 eV amuю1 in an electron beam ion trap. ... Line energy centroids, appropriate for both the beam-on and beam-off phases, are listed in Table 1. ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/FeCX.pdf -- 351.9 Кб -- 15.11.2005
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6248. http://hea-www.harvard.edu/~pgreen/FASTbals06a.lst
RA/DEC name i z comment Trimester ------------------------- ---- ---- ------- ---------- SDSSJ004527.69+143816.2 17.0 1.99 LoBAL Sep-Dec SDSSJ073739.96+384413.3 16.9 1.40 LoBAL `` SDSSJ085417.61+532735.3 16.9 2.42 HiBAL Jan-Apr SDSSJ090924.01+ 000211.0 16.4 1.87 HiBAL `` SDSSJ092011.34+495404.1 16.9 1.69 HiBAL `` SDSSJ093514.72+033545.7 16.9 1.82 HiBAL `` SDSSJ095929.89+633359.9 16.4 1.85 ...
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Ссылки http://hea-www.harvard.edu/~pgreen/FASTbals06a.lst -- 1.8 Кб -- 07.11.2005
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6249. http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/readme
J.E. Grindlay, 2004 ApJ 614 p508 and references therein ---------------------------------------------------------------------- Quantile analysis routines: 2 independent platforms are available - perl IDL (C version in future) perl: quantile .pl : quantile calculator src.txt : example src file bkg.txt : example bkg file grid.pl : quantile grid generator (requires sherpa) grid .sl : a sherpa-slang file required for ... Advanced routines for quantile and error calculation 2. ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/readme -- 4.5 Кб -- 25.10.2005
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/readme -- 4.5 Кб -- 25.10.2005
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/readme -- 4.5 Кб -- 25.10.2005
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6250. http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/pty_20051024.pdf
... Photon counts per unit 25 20 emission line? ... Taeyoung Park tpark@stat.harvard.edu Fitting Narrow Emission Lines in X-ray Spectra Highly Structured Multilevel Spectral Model Fitting the Spectral Model Partially Marginalized Gibbs Samplers Combining Observed Information Results of the EM-type Algorithm Table: Posterior Modes for ? Identified with the EM-type Algorithm. line profile ... Taeyoung Park < tpark@stat.harvard.edu > Fitting Narrow Emission Lines in X-ray Spectra ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/pty_20051024.pdf -- 840.5 Кб -- 25.10.2005
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_fMMV/pty_20051024.pdf -- 840.5 Кб -- 25.10.2005
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_fMMV/pty_20051024.pdf -- 840.5 Кб -- 25.10.2005
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6251. http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/map.pl
... For the model names and their parameters, refer Sherpa or # xspec manual. ... The file will contains 2+n columns where n is the number of "frac" # you request. ... ----------------------------------------------- # get the parameter files from command line use Getopt::Long; GetOptions( model =s = \$ model , range=s = \$range, frac =s = \$ frac , par1 =s = \$ par1 , par2=s = \$par2, etcp =s = \$ etcp , arf =s = \$ arf , rmf =s = \$ rmf , sherpa =s = \$ ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/map.pl -- 8.2 Кб -- 25.10.2005
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/map.pl -- 8.2 Кб -- 25.10.2005
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/map.pl -- 8.2 Кб -- 25.10.2005
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6252. http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/grid.sl
JaeSub Hong, 2003-2005, version 1.5 % Please report any problem or suggestion at jaesub@head.cfa.harvard.edu define imcounts (x,y) { variable i, n_data ; variable ans ; n_data = length (y); ans = Double_Type [ n_data ]; ans [0] = (x.hi[0]-x.lo[0])*y[0]; for (i=1;i n_data ;i++){ ans [i] = (x.hi[i]-x.lo[i])*y[i]+ ans [i-1]; } for (i=0;i n_data ;i++){ ans [i] = ans [i]/ ans [n_ data -1]; } ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/pre-release/grid.sl -- 2.9 Кб -- 21.10.2005
[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/grid.sl -- 2.9 Кб -- 21.10.2005
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[ Сохраненная копия ] Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile/grid.sl -- 2.9 Кб -- 21.10.2005
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6253. http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.7/test/this.rdb
# # ../grid.pl \ # -model "xswabs[A]*xspowerlaw[B]" \ # -range 0.1,8.0 \ # -frac 0.25,0.5,0.75 \ # -par1 A.nH:0.001,0.005,0.01,0.05,0.1,0.5,1,10:200 \ # -par2 B.PhoIndx:0,0.5,1,1.5,2,2.5,3,3.5,4:200 \ # -rmf ../example.rmf \ # -arf ../example.arf \ # gridID A_nH B_PhoIndx E25 E50 E75 S N N N N N gx0 0.001 0 1.61615 3.04923 4.62256 gx0 0.001 0.02 1.59884 3.014 4.59743 gx0 0.001 0.04 1.58165 2.97834 4.57205 gx0 0.001 0.06 1.56469 2.94236 4.54645 gx0 0.001 0.08 1.54915 2.9062 4.52065 gx0 0.001 0.1 1.53358
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.7/test/this.rdb -- 128.7 Кб -- 13.10.2005
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6254. http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.7/test/example.pro
@example.pro ; ; JaeSub Hong, 2003-2005, version 1.5 ; Please report any problem or suggestion at jaesub@head.cfa.harvard.edu ; range = [0.1,8.0] ; 0.3 - 8.0 keV frac = [0.25, 0.33, 0.50, 0.67, 0.75] nofixerror = 0 ; set 0 to fix error and 1 to not fix error ;- ... plot window xr =[-0.4,0.4] yr =[1.5,2.3] xtick =['0.6','1','2','3','4','5',' 6 keV','7'] ; top x-axis qd_setwin, xr=xr, yr=yr, range = range , xtick=xtick, stu=0.5 ; read grid data ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.7/test/example.pro -- 2.3 Кб -- 13.10.2005
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6255. http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.7/test/example.rdb
grid.pl \ # -model xszwabs[A]*xspowerlaw[B] \ # -range 0.1 ,8.0 \ # -frac 0.25,0.5,0.75 \ # -par1 A.nH: 0.01 , 0.1 ,1,10:200 \ # -par2 B.PhoIndx:0,1,2,3,4:200 \ # -etcp A.Redshift:0.0,B.norm:1.0 \ # -rmf ../example.rmf \ # -arf ../example.arf \ # gridID A_nH B_PhoIndx E25 E50 E75 S N N N N N gx0 0.01 0 1.63357 3.07156 4.63461 gx0 0.01 0.02 1.61664 3.03705 4.60982 gx0 0.01 0.04 1.59972 3.00211 4.58478 gx0 ...
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Ссылки http://hea-www.harvard.edu/ChaMPlane/quantile/quantile_1.7/test/example.rdb -- 65.8 Кб -- 13.10.2005
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6256. http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/jjs_20051011.pdf
Jiashun Jin , Purdue University , 10/11/ 2005 1 ' $ Higher Criticism: Theory and Applications in Cosmology Jiashun Jin Statistics Department Purdue Uinversity % Jiashun Jin , Purdue University , 10/11/ 2005 2 ' $ Collab orators Alphabetically: Nabila Aghanim Laura Cayon David Donoho Olivier Forni Jeau-Luc Starck Anna Treaster UniversitЄ Paris Sud e Purdue University Stanford ... Jiashun Jin, Purdue University, 10/11/2005 13 ' $ Optimal Adaptivity of Higher Criticism Theorem 2. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/jjs_20051011.pdf -- 1900.9 Кб -- 12.10.2005
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_fMMV/jjs_20051011.pdf -- 1900.9 Кб -- 12.10.2005
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_fMMV/jjs_20051011.pdf -- 1900.9 Кб -- 12.10.2005
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6257. http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/jjs_20051011_abstract.pdf
Higher Criticism Statistic: Theory and Applications in Cosmology and Astronomy Jiashun Jin Department of Statistics Purdue University October 2, 2005 Abstract Higher Criticism is a recent statistic proposed by Donoho and Jin [1] where it has been shown to be effective at resolving a very subtle testing problem: test whether n normal means are all zero versus the alternative that a small fraction is non-zero. Higher Criticism is also useful for non-Gaussian detection. ... 2004). ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/jjs_20051011_abstract.pdf -- 76.7 Кб -- 10.10.2005
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_fMMV/jjs_20051011_abstract.pdf -- 76.7 Кб -- 10.10.2005
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_fMMV/jjs_20051011_abstract.pdf -- 76.7 Кб -- 10.10.2005
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6258. http://hea-www.harvard.edu/~pgreen/Papers/PIA_AAStalk98.pdf
ConcepTests for Introductory Astronomy Smithsonian Astrophysical Observatory at the Harvard-Smithsonian Center for Astrophysics Paul J. Green large 100 students Earth to Cosmos in one semester phenomenological not conceptual well-practiced lectures, heavy on AV, graphics multiple choice exams emphasizing recall competitive grading discourages student interaction TYPICAL ASTRO 101: GETTING ... Present a ConcepTest: a short multiplechoice question tests students' understanding. ...
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Ссылки http://hea-www.harvard.edu/~pgreen/Papers/PIA_AAStalk98.pdf -- 144.6 Кб -- 23.09.2005
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6259. http://hea-www.harvard.edu/~pgreen/Papers/PIA_AAStalk98.ps
ConcepTests for Introductory Astronomy Paul J. Green Smithsonian Astrophysical Observatory at the HarvardґSmithsonian Center for Astrophysics TYPICAL ASTRO 101: ffl large (?100 students ) ffl Earth to Cosmos in one semester ffl phenomenological not conceptual ffl wellґpracticed lectures, heavy on AV, graphics ffl multiple choice exams emphasizing recall ffl competitive grading discourages student interaction GETTING STUDENTS UNINVOLVED! ... Instructor selects desired questions. ...
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Ссылки http://hea-www.harvard.edu/~pgreen/Papers/PIA_AAStalk98.ps -- 537.3 Кб -- 23.09.2005
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6260. http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/EURASIP-Paper.pdf
-91405, Orsay Cedex, France June 30, 2004 Abstract Currently, it appears that the best method for non-Gaussianity detection in the Cosmic Microwave Background ( CMB ) consists in calculating the kurtosis of the wavelet coefficients ... Max (Mn ). ... It has been shown [44] that it is also possible to separate the nonGaussian signatures associated with cosmic strings from those due to SZ effect by combining the excess kurtosis derived from these both the curvelet and the wavelet transform. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/EURASIP-Paper.pdf -- 1245.1 Кб -- 22.09.2005
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_fMMV/EURASIP-Paper.pdf -- 1245.1 Кб -- 22.09.2005
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_fMMV/EURASIP-Paper.pdf -- 1245.1 Кб -- 22.09.2005
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