A dataset provided by the European Space Agency

Name: An XMM Mini-survey of Ultraluminous IR Galaxies
Published: 2004-01-25T00:00:00Z

Proposal ID	008134
Title	An XMM Mini-survey of Ultraluminous IR Galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081340901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081341001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081341101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0081341401
DOI	https://doi.org/10.5270/esa-hlsff99
Principal Investigator, PI	Dr Alberto Franceschini
Abstract	We propose XMM observations of 11 ultra-luminous IRAS galaxies (ULIRG) recentlyobserved with ISO. The specific aim of our project is to test in hard X-ray thiswell defined, well studied sample of bright ULIRGs. The observation of the hardX-ray flux and of the FeK line properties will open a new prospective onimportant questions, like the understanding of the mechanism of primary energyproduction, the estimate of the X-ray emissivity of absorbed AGNs present in thenucleus and the evaluation of their contribution to the cosmic X-ray background.A physical knowledge of such local sources will be also crucially informativeabout the nature of their distant, high-z counterparts, likely to originate therecently discovered far-IR/sub-mm background.
Publications	XMM-Newton observations of ULIRGs: A Compton-thick AGN in IRAS 19254-7245 \|Braito V. Franceschini A. et al. \| A&A \| 398-107 \| 2003 \| 2003A&A...398..107B \| http://ui.adsabs.harvard.edu/#abs/2003A&A...398..107B The XMM-Newton and BeppoSAX view of the Ultra Luminous Infrared Galaxy MKN 231 \|Braito V. Della Ceca R. et al. \| A&A \| 420-79 \| 2004 \| 2004A&A...420...79B \| http://ui.adsabs.harvard.edu/#abs/2004A&A...420...79B Exploring the X-ray sky with the XMM-Newton bright serendipitous survey \|Della Ceca R. Maccacaro T. et al. \| A&A \| 428-383 \| 2004 \| 2004A&A...428..383D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...428..383D The XMM-Newton Needles in the Haystack Survey: the local X-ray luminosity function of normal galaxies \|Georgantopoulos I. Georgakakis A. \| MNRAS \| 360-782 \| 2005 \| 2005MNRAS.360..782G \| http://ui.adsabs.harvard.edu/#abs/2005MNRAS.360..782G X-QUEST: A Comprehensive X-ray Study of Local ULIRGS and QSOs \|Teng Stacy H. Veilleux Sylvain \| ApJ \| 725-1848 \| 2010 \| 2010ApJ...725.1848T \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725.1848T High-precision multi-band measurements of the angular clustering of X-ray sources \|Ebrero J. Mateos S. et al. \| A&A \| 500-749 \| 2009 \| 2009A&A...500..749E \| http://ui.adsabs.harvard.edu/#abs/2009A&A...500..749E The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Normal galaxies in the XMM-Newton fields. X-rays as a star formation indicator \|Rovilos E. Georgantopoulos I. et al. \| A&A \| 502-85 \| 2009 \| 2009A&A...502...85R \| http://ui.adsabs.harvard.edu/#abs/2009A&A...502...85R The X-ray Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars \|Young M. Elvis M. \| ApJ \| 708-1388 \| 2010 \| 2010ApJ...708.1388Y \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...708.1388Y An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy \|Levan A. J. Tanvir N. R. et al. \| Sci \| 333-199 \| 2011 \| 2011Sci...333..199L \| http://ui.adsabs.harvard.edu/#abs/2011Sci...333..199L The XMM-Newton Wide Angle Survey (XWAS): the X-ray spectrum of type-1 AGN \|Mateos S. Carrera F. J. et al. \| A&A \| 510-35 \| 2010 \| 2010A&A...510A..35M \| http://ui.adsabs.harvard.edu/#abs/2010A&A...510A..35M Average Fe Kalpha emission from distant AGN \|Corral A. Page M. J. et al. \| A&A \| 492-71 \| 2008 \| 2008A&A...492...71C \| http://ui.adsabs.harvard.edu/#abs/2008A&A...492...71C New constraints on the X-ray spectral properties of type 1 active galactic nuclei \|Scott A. E. Stewart G. C. et al. \| MNRAS \| 417-992 \| 2011 \| 2011MNRAS.417..992S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.417..992S X-ray absorption in distant type II QSOs \|Krumpe M. Lamer G. et al. \| A&A \| 483-415 \| 2008 \| 2008A&A...483..415K \| http://ui.adsabs.harvard.edu/#abs/2008A&A...483..415K The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project \|Fassbender R. Bohringer H. et al. \| NJPh \| 13-125014 \| 2011 \| 2011NJPh...13l5014F \| http://ui.adsabs.harvard.edu/#abs/2011NJPh...13l5014F Warm-hot intergalactic medium contribution to baryonic matter \|Soltan A. M. \| A&A \| 460-59 \| 2006 \| 2006A&A...460...59S \| http://ui.adsabs.harvard.edu/#abs/2006A&A...460...59S Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M X-ray Emission from Optically Selected Radio-intermediate and Radio-loud Quasars \|Miller B. P. Brandt W. N. et al. \| ApJ \| 726-20 \| 2011 \| 2011ApJ...726...20M \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...726...20M An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters \|Baldi A. Ettori S. et al. \| A&A \| 537-142 \| 2012 \| 2012A&A...537A.142B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...537A.142B X-ray colour-colour selection for heavily absorbed active galactic nuclei \|Brightman Murray Nandra Kirpal \| MNRAS \| 422-1166 \| 2012 \| 2012MNRAS.422.1166B \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422.1166B The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M An XMM-Newton hard X-ray survey of ultraluminous infrared galaxies \|Franceschini A. Braito V. et al. \| MNRAS \| 343-1181 \| 2003 \| 2003MNRAS.343.1181F \| http://ui.adsabs.harvard.edu/#abs/2003MNRAS.343.1181F The Serendipitous XMM-Newton Cluster Athens Survey (SEXCLAS): sample selection and the cluster logN-logS \|Kolokotronis V. Georgakakis A. et al. \| MNRAS \| 366-163 \| 2006 \| 2006MNRAS.366..163K \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.366..163K The XMM-SSC survey of hard-spectrum XMM-Newton sources - I. Optically bright sources \|Page M. J. Lehmann I. et al. \| MNRAS \| 378-1335 \| 2007 \| 2007MNRAS.378.1335P \| http://ui.adsabs.harvard.edu/#abs/2007MNRAS.378.1335P A Suzaku observation of the ULIRG IRAS19254-7245: discerning the AGN component \|Braito V. Reeves J. N. et al. \| A&A \| 504-53 \| 2009 \| 2009A&A...504...53B \| http://ui.adsabs.harvard.edu/#abs/2009A&A...504...53B The Difference in Narrow Fe Kalpha Line Emission Between Seyfert 1 and Seyfert 2 Galaxies \|Liu Teng Wang Jun-Xian \| ApJ \| 725-2381 \| 2010 \| 2010ApJ...725.2381L \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725.2381L X-ray spectral properties of Seyfert galaxies and the unification scheme \|Singh V. Shastri P. \| A&A \| 532-84 \| 2011 \| 2011A&A...532A..84S \| http://ui.adsabs.harvard.edu/#abs/2011A&A...532A..84S X-ray Insights into the Physics of Mini-BAL Quasar Outflows \|Gibson Robert R. Brandt W. N. et al. \| ApJ \| 696-924 \| 2009 \| 2009ApJ...696..924G \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...696..924G The XMM-Newton HBS28 sample: Studying the obscuration in hard X-ray selected AGNs \|Caccianiga A. Severgnini P. et al. \| A&A \| 416-901 \| 2004 \| 2004A&A...416..901C \| http://ui.adsabs.harvard.edu/#abs/2004A&A...416..901C 2-10 keV luminosity of high-mass binaries as a gauge of ongoing star-formation rate \|Persic M. Rephaeli Y. et al. \| A&A \| 419-849 \| 2004 \| 2004A&A...419..849P \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..849P X-ray spectra of XMM-Newton serendipitous medium flux sources \|Mateos S. Barcons X. et al. \| A&A \| 433-855 \| 2005 \| 2005A&A...433..855M \| http://ui.adsabs.harvard.edu/#abs/2005A&A...433..855M XMM-Newton data processing for faint diffuse emission. Proton flares exposure maps and report on EPIC MOS1 bright CCDs contamination \|Pradas J. Kerp J. \| A&A \| 443-721 \| 2005 \| 2005A&A...443..721P \| http://ui.adsabs.harvard.edu/#abs/2005A&A...443..721P Searching for X-ray luminous normal galaxies in 2dFGRS \|Tzanavaris P. Georgantopoulos I. \| A&A \| 454-447 \| 2006 \| 2006A&A...454..447T \| http://ui.adsabs.harvard.edu/#abs/2006A&A...454..447T The XMM-Newton EPIC background and the production of background blank sky event files \|Carter J. A. Read A. M. \| A&A \| 464-1155 \| 2007 \| 2007A&A...464.1155C \| http://ui.adsabs.harvard.edu/#abs/2007A&A...464.1155C The XMM-Newton serendipitous survey. III. The AXIS X-ray source counts and angular clustering \|Carrera F. J. Ebrero J. et al. \| A&A \| 469-27 \| 2007 \| 2007A&A...469...27C \| http://ui.adsabs.harvard.edu/#abs/2007A&A...469...27C BLOX: the Bonn lensing optical and X-ray selected galaxy clusters. I. Cluster catalog construction \|Dietrich J. P. Erben T. et al. \| A&A \| 470-821 \| 2007 \| 2007A&A...470..821D \| http://ui.adsabs.harvard.edu/#abs/2007A&A...470..821D The XMM-Newton serendipitous survey. IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS) \|Barcons X. Carrera F. J. et al. \| A&A \| 476-1191 \| 2007 \| 2007A&A...476.1191B \| http://ui.adsabs.harvard.edu/#abs/2007A&A...476.1191B The cosmological properties of AGN in the XMM-Newton Hard Bright Survey \|Della Ceca R. Caccianiga A. et al. \| A&A \| 487-119 \| 2008 \| 2008A&A...487..119D \| http://ui.adsabs.harvard.edu/#abs/2008A&A...487..119D High precision X-ray log N - log S distributions: implications for the obscured AGN population \|Mateos S. Warwick R. S. et al. \| A&A \| 492-51 \| 2008 \| 2008A&A...492...51M \| http://ui.adsabs.harvard.edu/#abs/2008A&A...492...51M XMM-Newton Observation of Fe Kalpha Emission from a Broad Absorption Line Quasar: Markarian 231 \|Turner T. J. Kraemer S. B. \| ApJ \| 598-916 \| 2003 \| 2003ApJ...598..916T \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...598..916T Variation in the Scattering Shroud Surrounding Markarian 231 \|Gallagher S. C. Schmidt Gary D. et al. \| ApJ \| 633-71 \| 2005 \| 2005ApJ...633...71G \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...633...71G Are Optically Selected Quasars Universally X-Ray Luminous? X-Ray-UV Relations in Sloan Digital Sky Survey Quasars \|Gibson Robert R. Brandt W. N. \| ApJ \| 685-773 \| 2008 \| 2008ApJ...685..773G \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...685..773G The Reddest DR3 SDSS/XMM-Newton Quasars \|Young M. Elvis M. \| ApJ \| 688-128 \| 2008 \| 2008ApJ...688..128Y \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...688..128Y The Correlation Between X-ray and UV Properties of BAL QSOs \|Fan Lu Lu Wang Hui Yuan et al. \| ApJ \| 690-1006 \| 2009 \| 2009ApJ...690.1006F \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...690.1006F The XMM-Newton serendipitous survey. VI. The X-ray luminosity function \|Ebrero J. Carrera F. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2001-03-30T09:06:52Z/2002-11-19T11:43:30Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2004-01-25T00:00:00Z
Last Update	2025-01-27
Keywords	"absorbed agns", "cosmic xray background", "ultraluminous ir galaxy", "hard xray", "crucially informative", "z counterparts", "sub mm background", "bright ulirg", "xmm mini survey", "xray emissivity", "fek line properties", "XMM", "hard xray flux", "physical knowledge", "primary energy production", "local sources"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Alberto Franceschini, 2004, 'An XMM Mini-survey of Ultraluminous IR Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hlsff99