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5861. http://hea-www.harvard.edu/~garcia/m31/garcia_chandra6y_short.pdf
Our Chandra M31 Campaign Some Surprises and M31* Michael Garcia, Smithsonian Astrophysical Observatory Ben Williams (Penn St), Albert Kong(MIT), Steve Murray (HRC/GTO), Manuel Torres-Perez, Francis Primini Chandra HRC M Garcia, 6 Years of Chandra, Nov 4 2005 1 Our Campaign: ACIS Followup of Transients ЇMost transients in bulge, ACIS+HRC obs concentrated ЇAO1,2,3,5,7... 107 separate obs, =574ks! [141/814ks!! ... M Garcia, 6 Years of Chandra, Nov 4 2005 12 ...
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Ссылки http://hea-www.harvard.edu/~garcia/m31/garcia_chandra6y_short.pdf -- 1415.0 Кб -- 28.06.2011
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5862. http://hea-www.harvard.edu/~garcia/ixo/htrs_comments.pdf
Smithsonian Astrophysical Observatory Memorandum To: D. Barret Cc: J. Grady, T. Buckler, J. Bookbinder, R. Smith From: M. Garcia Date: Aug 2, 2010 Re: HTRS data rates, observing profile mrg-2010-08-02 Hi Didier: I've read over HTRS-RP-21B-019-CESR (really only the section on data rates/compression/storage). ... Compressing the data is a good idea, as is having a flexible data collection mode (ie, spectral binning ala RXTE). ... Did the one-year observing plan include also non-HTRS targets? ...
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Ссылки http://hea-www.harvard.edu/~garcia/ixo/htrs_comments.pdf -- 223.5 Кб -- 28.06.2011
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5863. http://hea-www.harvard.edu/~garcia/conx/ConX_TLRD_0107.pdf
... CONSTELLATION- X SCIENCE OBJECTIVES .. ... SPECTRAL RESOLUTION .. ... 3 Working Draft Jan 1 1,2007 Dec2006 FST Version 3.3 Spectral Accuracy From 0.3 keV to 10 keV, the energy (wavelength) accuracy shall be <20% of the energy (wavelength) resolution, with a goal of <10%. ... 3.8 Extended Source Capability The mission shall be capable of obtaining spectra; with the stated spatial and spectral resolutions, over the energy range of 1keV to 40 keV for sources larger than the HPD defined above. ...
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Ссылки http://hea-www.harvard.edu/~garcia/conx/ConX_TLRD_0107.pdf -- 64.6 Кб -- 28.06.2011
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5864. http://hea-www.harvard.edu/~garcia/conx/conx_srd_001008.pdf
CONX-RQMT-001008 Constellation-X Science Requirements Document, Version of 09/18/2007 -1- Constellation-X Science Requirements Document Version of 09/18/2007PM CONX-RQMT-001008 Constellation-X Science Requirements Document, Version of 09/18/2007 -2- TABLE OF CONTENTS 1.0 Strong Gravity and Black Holes ........................................................................................................... 8 1.1 Using Black Holes to Test GR
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Ссылки http://hea-www.harvard.edu/~garcia/conx/conx_srd_001008.pdf -- 258.4 Кб -- 28.06.2011
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5865. http://hea-www.harvard.edu/~dburke/aas218/tweetanim/aas218_anim.pde
... PImage bgImg; // set here rather than dynamically calculated since it is used in // the setup call. final int titleBorder = titleFontSize + 4; // + 4; // used to place items within the title border int [] titleBorderRange = { 4, titleBorder - 4 }; // width of the border used to display the name of the Tweeter final int nameBorder = 140; // state variables boolean animate = true; boolean showBackground = true; boolean showHelp = true; boolean showCredits ...
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Ссылки http://hea-www.harvard.edu/~dburke/aas218/tweetanim/aas218_anim.pde -- 21.2 Кб -- 06.06.2011
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5866. http://hea-www.harvard.edu/~dburke/aas218/tweetanim/Tweet.pde
Simple class for displaying a Tweet. */ static HashMap colorMap = new HashMap(); static int nearly = 0; static int nlate = 0; static int ntweets = 0; static int maxNameWidth = 0; static final int twXpos = 10; static final int rtXpos = 25; static final int spacing = 20; int get_ spacing () { return spacing ; } int get_nearly() { return nearly; } ...
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Ссылки http://hea-www.harvard.edu/~dburke/aas218/tweetanim/Tweet.pde -- 4.3 Кб -- 04.06.2011
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5867. http://hea-www.harvard.edu/~dburke/aas218/tweetanim/histogram.pde
histogram -based routines * * when dayLen = 1 day and hx1 = nameBorder+1, hx2 = width-1 * then the width of a bin is 85 seconds. */ static final int histBgColor = #99cc99; static final int histFgColor = #999966; // static final int histBgColor = #66cc66; // static final int histFgColor = #999933; static final int histHiColor = #cc3333; static final ...
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Ссылки http://hea-www.harvard.edu/~dburke/aas218/tweetanim/histogram.pde -- 5.6 Кб -- 04.06.2011
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5868. http://hea-www.harvard.edu/~fine/OSX/warranty
... serial . ... my $ ret ; open(SP, system_profiler $SPtype -xml| ); while( SP ) { if (/^\s* \?xml /) { next; } if (/^\s* !DOCTYPE /) { next; } if (/^\s* plist /) { next; } if (/^\s* \/ plist /) { next; } $ ret = makeobj($_); # print ret =$ ret -- $_\n ; } close(SP); return $ ret ; } sub makeobj { local ($_)=shift(@_); if (/\s* array /) { return ( array ); } elsif (/\s* dict /) { ...
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Ссылки http://hea-www.harvard.edu/~fine/OSX/warranty -- 8.2 Кб -- 10.05.2011
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5869. http://hea-www.harvard.edu/~garcia/cv2011.pdf
... 720W Why are X-Ray Sources in the M31 Bulge So Close to Planetary Nebulae?, ... J. McClintock (CfA), S. Murray (CfA), M. Garcia (CfA) and P. Jonker (IoA), 8 Nov 2003 ATEL 104, Magnitudes of X-ray Nova XTE J1650-500 in Quiescence , M. Garcia and B. Wilkes, 10 Aug 2002 ATEL 87, Optical Counterpart of the Millisecond Pulsar XTE J1751-305 , A.K.H. Kong, P. Challis, M.R . Garcia and R. Kirshner (Harvard-Smithsonian Center for Astrophysics), 17 Apr 2002 ATEL 83, X-ray Transients in M31 ,...
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Ссылки http://hea-www.harvard.edu/~garcia/cv2011.pdf -- 119.6 Кб -- 09.05.2011
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5870. http://hea-www.harvard.edu/AstroStat/Stat310_1011/ad_20110419.pdf
... memb ers of the CAUSTIC Group www.dfg.unito.it/ricerca/caustic Cambridge, April 19th 2011 SCIENTIFIC BACKGROUND Observations of SNae : Interpretation in the CDM model Alternative cosmological models: Conformal gravity and kinematic conformal gravity GRBs as cosmological probes: Bayesian approach BAYESIAN ANALYSIS Parameter forecasts (posterior probability): Likelihood and priors ... Constitution set of Hicken et al 2009) Bayesian parameter estimation again.. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1011/ad_20110419.pdf -- 2896.9 Кб -- 19.04.2011
[ Текст ] Ссылки http://hea-www.harvard.edu/AstroStat/talks_1011/ad_20110419.pdf -- 2896.9 Кб -- 19.04.2011
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/talks_1011/ad_20110419.pdf -- 2896.9 Кб -- 19.04.2011
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[ Текст ] Ссылки http://hea-www.harvard.edu/AstroStat/talks_1011/ad_20110419.pdf -- 2896.9 Кб -- 19.04.2011
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/talks_1011/ad_20110419.pdf -- 2896.9 Кб -- 19.04.2011
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5871. http://hea-www.harvard.edu/~saku/curgrants.pdf
Current Grants: Saeqa Dil Vrtilek (Principal Investigator) 2007-2010 "Sup erorbital Variation of LMC X-4: Exploring the Accretion Flow" NASA Suzaku Cycle 2. 23,199 2007-2010 "Inflows and Outflows in X-ray Binaries: Getting the Big Picture" NASA ROSES ADP. 223,100. 2007-2010 "The Sp ectral Energy Distributions of X-ray Binaries" Smithsonian Endowment. 41,113. 2010-2011 "Modulation tomography: imaging black hole binaries." ... Smithsonian Women's Program Committee. 10,000.00 ...
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Ссылки http://hea-www.harvard.edu/~saku/curgrants.pdf -- 17.4 Кб -- 14.04.2011
[ Текст ] Ссылки http://hea-www.harvard.edu/~saku/curgrants.ps -- 17.4 Кб -- 14.04.2011
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[ Текст ] Ссылки http://hea-www.harvard.edu/~saku/curgrants.ps -- 17.4 Кб -- 14.04.2011
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5872. http://hea-www.harvard.edu/~elvis/vigorous.pdf
... The science from both these missions contributed to three of the Nobel Prizes ґ Giacconi (2002), Mather, and Smoot (2006) - awarded for NASA-based science. ... We encourage NASA to seek new launch capabilities to fill this strategic gap in moderate lift rockets to enable the Explorer program to continue launching missions with significant science payoff but reduced costs and timescales compared to large strategic missions. ... 18 Appendix B: Explorer Missions 1989-present (From PILMSS) No . ...
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Ссылки http://hea-www.harvard.edu/~elvis/vigorous.pdf -- 359.4 Кб -- 14.04.2011
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5873. http://hea-www.harvard.edu/~elvis/QuasarScales.pdf
Scale of Quasar/AGN Components Relativistic Jet perpendicular to disk Nucleus Host Galaxy Disk Bulge Dusty wind Warped mol. disk 2000 K Failed wind Dusty molecular torus Ionized Wind Compton Wind Accretion disk continuum Black Hole Bicones log(Radius) 20 K ~10 M 7 10 kpc 1 kpc 100 pc 10 106 105 1 pc pc 104 1000 100 rs 10 1 symmetry FIR MIR cont cont 100 ?m N CO H2 ...
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Ссылки http://hea-www.harvard.edu/~elvis/QuasarScales.pdf -- 326.1 Кб -- 13.04.2011
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5874. http://hea-www.harvard.edu/~elvis/quasarsed.pdf
Radio IR Opt-UV EUV X-ray Radioloud mmbreak (~100m) BigBlueBump (0.1~1m) 1m inflec<on Compton Hump (~1030keV) So3Excess (~0.1keV) Radioquiet L=3(dust) Elvis et al., 1994, ApJS, 95, 1
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Ссылки http://hea-www.harvard.edu/~elvis/quasarsed.pdf -- 85.1 Кб -- 13.04.2011
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5875. http://hea-www.harvard.edu/~elvis/quasarsed.ps
Elvis et al., 1994, ApJS, 95, 1 # IR# OptґUV# ############## ########## ########### ########### #### ######## # ######### ######### Radio# ######## ######### ########### # ###### ## ######## EUV# ########### ############ Xґray#
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Ссылки http://hea-www.harvard.edu/~elvis/quasarsed.ps -- 283.9 Кб -- 13.04.2011
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5876. http://hea-www.harvard.edu/~elvis/ref_papers.ps
... 30 1985 The Diversity of Soft Xґray Spectra in Quasars (M. Elvis, B.J. Wilkes, and H. Tananbaum) The Astrophysical Journal, volume 292, 357. ... 40 1987 Quasar Energy Distributions: I. Soft Xґray Spectra of Quasars (B.J. Wilkes and M. Elvis), The Astrophysical Journal, volume 323, 243. ... 74 1994 The Complex Soft Xґray Spectrum of LowґRedshift RadioґQuiet Quasars I: The Xґray Data (F. Fiore, A Siemiginowska, M. Elvis, B.J. Wilkes, and J.C. McDowell), Ap.J., 431 515. ...
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Ссылки http://hea-www.harvard.edu/~elvis/ref_papers.ps -- 73.3 Кб -- 13.04.2011
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5877. http://hea-www.harvard.edu/~elvis/nonref.ps
... 1990 The Soft Xґray Excess in Einstein Quasar Spectra (B.J. Wilkes, J.ґL. Masnou, M. Elvis, J. McDowell, and K. Arnaud), in ``Xґray Astronomy'', proceedings of the 23rd ESLAB Symposium [Noordwijk: ESA], ed. N.E. White, p.1081. ... 1993 Absorption in the ROSAT Xґray Spectra of Quasars (B.J. Wilkes, M. Elvis, F. Fiore, and J. McDowell), in ``The Nature of Compact Objects in Active Galactic Nuclei'', eds. A. Robinson and R.J. Terlevitch [Cambridge: CUP], p . ...
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Ссылки http://hea-www.harvard.edu/~elvis/nonref.ps -- 53.4 Кб -- 13.04.2011
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5878. http://hea-www.harvard.edu/~elvis/primer.ps
Broad Absorption Lines BAL Broad Emission Lines BEL Narrow Absorption Lines NAL X-ray Warm Absorber XWABS OVII, OVIII edges A Structure for Quasars A Quasar Primer OVI CIV Ly H H a b a ultraviolet (UV) optical Fall 2001 primer.fig 0.1 1 10 E (keV) 1000 3000 7000A l FeK Hump Compton Absorber a=1 Compton hump Reflection Features Fe-K Optical, Ultraviolet X-ray Warm Highly Ionized Gas (WHIG) Warm 1-5%c 2-10%c Dv
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Ссылки http://hea-www.harvard.edu/~elvis/primer.ps -- 47.5 Кб -- 13.04.2011
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5879. http://hea-www.harvard.edu/~elvis/leicester_sept04_sum_nobk.pdf
Tori & Winds, Leicester 14 September 2004 Disk Winds - tests? ... Tori & Winds, Leicester 14 September 2004 Elvis 2000: pluses, minuses q UV/X-ray connection Ї FUSE, STIS partial covering, transverse; broader abs = edge-on [Kriss, Kaastra] Ї location: disk or torus [M.E., Kriss, Kaastra] Ї WA variability. ... BELR in wind? ... Fabian] Tori & Winds, Leicester 14 September 2004 Black Hole Evolution q Obscured population, vs z. [Simpson] Just a phase black holes go through? q Star formation in disk. ...
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Ссылки http://hea-www.harvard.edu/~elvis/leicester_sept04_sum_nobk.pdf -- 2660.0 Кб -- 13.04.2011
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5880. http://hea-www.harvard.edu/~elvis/GenX_SPIE06.pdf
Active X-ray Optics for Generation-X, the Next High Resolution X-ray Observatory Martin Elvisa , R.J. Brissendena , G. Fabbianoa , D.A. Schwartza , P. Reida , W. Podgorskia , M. Eisenhowera , M. Judaa , J. Phillipsa , L. Cohena , S. Wolka , a Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge MA 02138, USA ABSTRACT X-rays provide one of the few bands through which we can study the epoch of reionization, when the first galaxies, black holes and stars were born. ... Figure 1. ...
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Ссылки http://hea-www.harvard.edu/~elvis/GenX_SPIE06.pdf -- 317.3 Кб -- 13.04.2011
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