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5801. http://hea-www.harvard.edu/AstroStat/Stat310_1112/jx_20120207.pdf
Outline Background Problem description Methodology Research New Results Two concerns New Results of Fully Bayesian JIN XU UCI February 7, 2012 JIN XU New Results of Fully Bayesian Outline Background Problem description Methodology Research New Results Two concerns Background Problem description Calibration Samples ... Our goal is to incorporate the uncertainty by Bayesian Methods. ... JIN XU New Results of Fully Bayesian ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1112/jx_20120207.pdf -- 1915.4 Кб -- 07.02.2012
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_1112/jx_20120207.pdf -- 1915.4 Кб -- 07.02.2012
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_1112/jx_20120207.pdf -- 1915.4 Кб -- 07.02.2012
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5802. http://hea-www.harvard.edu/~garcia/cv2012.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/cv2012.pdf -- 119.6 Кб -- 06.02.2012
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5803. http://hea-www.harvard.edu/~garcia/ixo/high_rate_agn_v3.pdf
Smithsonian Astrophysical Observatory Memorandum To : From Date: Re: M. Cappi, Strong Gravity SDT/YB Team, XMS team : M. Garcia April 14, 2010 XMS high/mid/low resolution event rates for bright AGN mrg-2010-02v2 This memo arises out of the concern that the bright AGN that will be used to observed strong gravity effects ґ in particular those for which time-resolved measurements of test particle orbits will be made ґ may generate counting rates in the XMS that are sufficient to overwhelm it. ...
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Ссылки http://hea-www.harvard.edu/~garcia/ixo/high_rate_agn_v3.pdf -- 204.4 Кб -- 31.01.2012
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5804. http://hea-www.harvard.edu/~pgreen/educ/Collabs.list
... Bryan Penprase penprase @krishna.physics.hmc.edu Shauna Sallmen shauna@critters.physics.uwlax.edu $ Eric Sandquist erics@apollo.astro.nwu.edu $ Edward G Schmidt eschmidt@unlserve.unl.edu N! Eric Schulman eschulma@NRAO.EDU e Stephen E. Schneider schneider@astro.umass.edu N selected questions included already onto WWW pages $ consent by email to book publ N declined book publ e helped edit or provided feedback on conceptests . ...
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Ссылки http://hea-www.harvard.edu/~pgreen/educ/Collabs.list -- 3.3 Кб -- 11.01.2012
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5805. http://hea-www.harvard.edu/~deluca/DeLuca_Resume_2012_onepage.pdf
58 60 Garden St. Cambridge, MA 02138 T 617-496-7725 F 617-496-7577 edeluca@cfa.har vard.edu EDUCATION Ph.D. Astrophysics, 1986, University of Colorado, Boulder, CO B.A. Astronomy, 1979, Wesleyan University , Middletown, CT APPOINTMENT Smithsonian Astrophysical Observatory, Cambridge, MA Senior Astrophysicist PREVIOUS APPOINTMENTS 2012 - present SAO , Cambridge, MA - Supervisory Astrophysicist SAO , Cambridge, MA - Astrophysicist IfA, ... Hinode is a strategic solar mission in low earth orbit. ...
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Ссылки http://hea-www.harvard.edu/~deluca/DeLuca_Resume_2012_onepage.pdf -- 508.0 Кб -- 04.01.2012
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5806. http://hea-www.harvard.edu/~kim/pap/2011_ASSL_chapter5.pdf
Chapter 5 Metal Abundances in the Hot ISM of Elliptical Galaxies Dong-Woo Kim Abstract X-ray spectroscopy provides a powerful tool to measure various elemental abundances in the hot ISM and the measured abundances in turn can be compared with galaxy chemical evolution models to constrain important astrophysical quantities and to help our understanding of the formation and evolution of elliptical galaxies and their ISM. In this chapter, I will address various technical issues involved in X-ray spectral
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Ссылки http://hea-www.harvard.edu/~kim/pap/2011_ASSL_chapter5.pdf -- 1176.6 Кб -- 22.12.2011
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5807. http://hea-www.harvard.edu/~kim/pap/2011_ASSL.pdf
Hot Interstellar Matter in Elliptical Galaxies For further volumes: http://www.springer.com/series/5664 Astrophysics and Space Science Library EDITORIAL BOARD Chairman W. B. BURTON, National Radio Astronomy Observatory, Charlottesville, Virginia, U.S.A. (bburton@nrao.edu); University of Leiden, The Netherlands (burton@strw.leidenuniv.nl) F. BERTOLA, University of Padua, Italy J. P. CASSINELLI, ... Giuseppina Fabbiano 1 21 55 83 2 Hot Gas Flows on Global and Nuclear Galactic Scales .. ...
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Ссылки http://hea-www.harvard.edu/~kim/pap/2011_ASSL.pdf -- 82.7 Кб -- 22.12.2011
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5808. http://hea-www.harvard.edu/~pgreen/CfP/CfP_Cycle14_updated_12-7-11-d.doc
The Chandra X-ray Observatory (CXO) Research Program Call for Proposals Cycle 14 Due Date: 15 March 2012, 6 p.m. EDT Prepared by: Chandra X-ray Center 60 Garden Street, Cambridge, MA 02138 15 December 2011 The Chandra X-ray Center is operated for NASA by the Smithsonian Astrophysical Observatory Table of Contents Chapter 1 - General Information 2 1.1 The Chandra Program: Call for Proposals (CfP) 2 1.2 Proposal Review Process: Deadlines and Schedule 2 1.3 Summary of the CfP 3 1.3.1 Types of Science Research
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Ссылки http://hea-www.harvard.edu/~pgreen/CfP/CfP_Cycle14_updated_12-7-11-d.doc -- 632.5 Кб -- 07.12.2011
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5809. http://hea-www.harvard.edu/~pgreen/Papers/wsqps11.pdf
... Printed in the U.S.A. A MULTIWAVELENGTH STUDY OF BINARY QUASARS AND THEIR ENVIRONMENTS Paul J. Green1 ,7 , Adam D. Myers2 ,7 , Wayne A. Barkhouse3 ,7 , Thomas L. Aldcroft1 , Markos Trichas1 , Gordon ? ... While larger binary QSO samples with richer far-IR and submillimeter multiwavelength data might better reveal signatures of merging and triggering, optical color selection of QSO pairs may be biased against such signatures. ... 2009). ... 2006, 2010; Myers et al. ... 2010, ApJ, 722, 1180 Green et...
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Ссылки http://hea-www.harvard.edu/~pgreen/Papers/wsqps11.pdf -- 742.4 Кб -- 23.11.2011
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5810. http://hea-www.harvard.edu/AstroStat/Stat310_1112/et_20111115.pdf
... Life arose very quickly on the early Earth. ... P[B|A] = probability of the data given the model = the likelihood (what we can obtain from a forward calculaCon) Pprior[A] = a priori probability the model is true/correct = the prior (oeen requires arbitrary judgment calls, source of controversy) P[B] = probability of the data (typically unknown, but only needed for normalizaCon) A Uniform Rate (Poisson) Model = rate of abiogenesis per Gyr per Earth like planet t = age of the ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1112/et_20111115.pdf -- 2466.2 Кб -- 15.11.2011
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_1112/et_20111115.pdf -- 2466.2 Кб -- 15.11.2011
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_1112/et_20111115.pdf -- 2466.2 Кб -- 15.11.2011
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5811. http://hea-www.harvard.edu/tanagra/etc/jpb_Hinode5_96.pdf
... The performance of each algorithm on the simulated lightcurves is scored accor ding to the rates of false positive (Type I) and false negative (Type II) errors. ... Combined: threshold normalization = 5 в 10 -4 References Ї Aschwanden, M.J., Nightingale, R.W. Tarball, T.D., & Wolfson, C.J. 2000, Ap J , 5 3 5 , 1 0 2 7 Ї Hudson, H.S. 1991, SoPh, 133, 357 Figure 3 Calibrating the event detection algorithms to optimize false positives, using the simulated lightcurves with zero events. ...
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Ссылки http://hea-www.harvard.edu/tanagra/etc/jpb_Hinode5_96.pdf -- 147.8 Кб -- 11.10.2011
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5812. http://hea-www.harvard.edu/~saku/MollyInstructions.pdf
... Type 'help' or '?' for a command list. ... Open files for editing 1]: 1 1]: 2 (Where 1 2 are the first and last file numbers to edit) del -- Delete header item. ren -- Rename header item. quit -- Quit edit file Enter filename [header]: molly .info Variable Variable Variable Variable Variable Variable Variable Variable Variable edit Quit 1 2 3 4 5 6 7 8 9 name: name: name: name: name: name: name: name: name: Object UTC RA Dec Equinox Dwell Day Month Year , type : C , type : D , ...
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Ссылки http://hea-www.harvard.edu/~saku/MollyInstructions.pdf -- 80.1 Кб -- 04.10.2011
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5813. http://hea-www.harvard.edu/~kim/pap/2010_N4278_LMXB_sp.pdf
... 5" 5" Figure 2. ... 2, 2010 FIELD AND GC LMXBs IN NGC 4278 1829 Figure 4. ... Luminous Field LMXBs The results of the spectral analysis of three B09 field sources, S146, S158, and S184, each with average B09 luminosity of 5.0 в 1038 erg s-1 over the six observations (Figure 4), are 1832 FABBIANO ET AL. ... 2, 2010 FIELD AND GC LMXBs IN NGC 4278 1835 Figure 10. 1 and 2 confidence contours for two interesting fit parameters for the co-added individual field sources: left, PO model; right, DBB model. ...
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Ссылки http://hea-www.harvard.edu/~kim/pap/2010_N4278_LMXB_sp.pdf -- 1617.5 Кб -- 14.09.2011
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5814. http://hea-www.harvard.edu/~kim/pap/2010_N3379_LMXB_sp.pdf
... Printed in the U.S.A. THE X-RAY SPECTRA OF THE LUMINOUS LMXBs IN NGC 3379: FIELD AND GLOBULAR CLUSTER SOURCES N. J. Brassington1 , G. Fabbiano1 , S. Blake2 ,3 , A. Zezas1 ,4 ,5 , L. Angelini6 , R. L. Davies3 , J. Gallagher7 , V. Kalogera8 ... Only the best-fit values derived from the = 1.7 simulations are presented. ... Decision tree summarizing how the best-fit absorption values from the PO and DBB single-component models from the simulations can be used to determine spectral source states. ...
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Ссылки http://hea-www.harvard.edu/~kim/pap/2010_N3379_LMXB_sp.pdf -- 1056.6 Кб -- 14.09.2011
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5815. http://hea-www.harvard.edu/tanagra/etc/jpb_HEAD2011_1005.pdf
HEAD 2011: Poster 10.05 Project Tanagra: Stellar Flares in Chandra High-Resolution Spectra Jennifer Posson-Brown, Vinay Kashyap, Steven Saar & Jeremy Drake (Harvard-Smithsonian Center for Astrophysics) Abstract We introduce Project Tanagra: Timing Analysis of Gratings Data, a uniform study of archival Chandra gratings observations of active l ow-mass coronal stars. ... See Kashyap et al. 2002, 2011 and Saar et al. 2011.) ... High resolution spectra from MEG and HEG first order, and ze roth order. ...
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Ссылки http://hea-www.harvard.edu/tanagra/etc/jpb_HEAD2011_1005.pdf -- 792.0 Кб -- 06.09.2011
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5816. http://hea-www.harvard.edu/AstroStat/Stat310_1112/ab_20110906.pdf
Taste of astrostatistics A taste of astrostatistics: problems, opportunities, & connections Alexander W Blocker 2011 Sep 06 Taste of astrostatistics Outline Outline 1 2 Astrostatistics in broad strokes Stacking: statistical challenges can come in small packages Problem Model Computation Data Results Lessons Event detection: massive, messy data Problem Method Results Lessons Connections 3 4 Taste of astrostatistics Astrostatistics in broad strokes What is astrostatistics? ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1112/ab_20110906.pdf -- 1327.9 Кб -- 06.09.2011
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_1112/ab_20110906.pdf -- 1327.9 Кб -- 06.09.2011
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_1112/ab_20110906.pdf -- 1327.9 Кб -- 06.09.2011
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5817. http://hea-www.harvard.edu/~zhao/champlane_chandra_GC_1deg.rdb
7N 5N 7N 38S 2N 11S 11S 10N 10N 9N 9N 19S 7N 28S 8S 11S 8S 7S 12N 12N 20N 21N 6N 7N 7N 7N 7N 7N 30S 17N 19N 17N 17N 19N 17N 36 ctio03 GC2 17:43:33.12 -29:01: 48.0 17:43:48.33 -29:01:47.5 17:43:49.61 -29:02: 33.6 265.956708 -29.042667 359.70422 0.27872 11.749 6.814 47.311 36.115 27.051 17.299 00242 600002 SGR_A -1 17:45:40.00 -29:00:28.0 266.416667 -29.007778 -0.05585 -0.04594 1999-09-21T02:43:00 50.000 PROF_GORDON_GARMIRE ACIS-I ACIS-012367 NONE ...
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Ссылки http://hea-www.harvard.edu/~zhao/champlane_chandra_GC_1deg.rdb -- 73.4 Кб -- 26.08.2011
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5818. http://hea-www.harvard.edu/~zhao/champlane_chandra_GC_1deg.tbl
----------------------- ----------- ----------- --------- --------- ------ -------- ------- ------------------- ------ 36 00242 SGR_A 17:45: 40.00 -29:00: 28.0 - 0.05585 - 0.04594 56.497 ACIS-I 50.000 1999-09-21T02:43:00 ctio03 35 00658 1E_1740.7-2942 17:43:54.85 -29:44:42.8 -0.88409 -0.10575 29.096 ACIS-I 9.600 2000-08-30T16:59:32 ctio03 37 00944 SGR_B2 17:47:06.70 -28:26:47.3 0.58833 -0.02490 81.200 ...
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Ссылки http://hea-www.harvard.edu/~zhao/champlane_chandra_GC_1deg.tbl -- 21.4 Кб -- 26.08.2011
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5819. http://hea-www.harvard.edu/~zhao/mosaic_chandra_anticen.rdb
MID Mosaic Field object obsid RA Dec l b Exp detector NHe22 date_obs 3N 6S 7S 22S 5N 11S 11S 9N 9N 7N 8S 5N 19S 1 ctio00 A0620 A0620-00 00095 06:22:44.50 -00:20:44.7 209.95633 -6.53984 43.500 ACIS-S 0.283 2000-02-29T03:32:24 1 ctio00 A0620 A0620-00 05479 06:22:44.50 -00:20:45.0 209.95639 -6.53988 40.000 ACIS-S 0.283 2005-08-20T08:36:46 2 ctio00 PKS0745 PKS_0745-191 00508 07:47:31.10 -19:17:47.0 236.44261 3.02756 28.200 ACIS-S 0.304 2000-08-28T22:15:31 2 ...
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Ссылки http://hea-www.harvard.edu/~zhao/mosaic_chandra_anticen.rdb -- 5.7 Кб -- 26.08.2011
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5820. http://hea-www.harvard.edu/~zhao/mosaic_chandra_anticen.tbl
- ------- ---------------------- ----- ----------- ----------- --------- --------- ------- -------- ----- ------------------- 1 ctio00 A0620 A0620-00 00095 06:22:44.50 -00:20:44.7 209.95633 -6.53984 43.500 ACIS-S 0.283 2000-02-29T03:32:24 1 ctio00 A0620 A0620-00 05479 06:22:44.50 -00:20:45.0 209.95639 -6.53988 40.000 ACIS-S 0.283 2005-08-20T08:36:46 2 ctio00 PKS0745 PKS_0745-191 00508 07:47:31.10 -19:17:47.0 236.44261 3.02756 28.200 ACIS-S ...
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Ссылки http://hea-www.harvard.edu/~zhao/mosaic_chandra_anticen.tbl -- 7.0 Кб -- 26.08.2011
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