A dataset provided by the European Space Agency

Name: Partially obscured quasars in the local universe
Published: 2007-12-12T00:00:00Z

Proposal ID	030575
Title	Partially obscured quasars in the local universe
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305750901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305751001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305751501 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305751601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0305751701
DOI	https://doi.org/10.5270/esa-uiagipw
Principal Investigator, PI	Dr Stefanie Komossa
Abstract	We propose an XMM survey of low redshift partially obscured quasars discoveredin the Sloan Digital Sky Survey (SDSS). These objects are characterized by largeBalmer decrements, stellar-light dominated continuum, luminous broad Halpha andnarrow OIII. With an estimated density similar to optical-color selected QSOs,this large population of obscured QSOs has many impacts on quasar studies, suchas the inclination oriented unification scheme. However, it is far from clearwhether they are absorbed but otherwise normal quasars, or a special class ofobjects. X-rays will provide a unique view to distinguish between thesepossibilities, and allow us to determine this objects contribution to the X-raybackground.
Publications	X-Ray Absorption and Optical Extinction in the Partially Obscured Seyfert Nucleus in Mrk 1393 \|Wang T. G. Zhou H. Y. et al. \| AJ \| 137-4002 \| 2009 \| 2009AJ....137.4002W \| http://ui.adsabs.harvard.edu/#abs/2009AJ....137.4002W 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 A New Sample of Buried Active Galactic Nuclei Selected from the Second XMM-Newton Serendipitous Source Catalogue \|Noguchi Kazuhisa Terashima Yuichi \| ApJ \| 705-454 \| 2009 \| 2009ApJ...705..454N \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...705..454N 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 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 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 A combined optical and X-ray study of unobscured type 1 active galactic nuclei - I. Optical spectra and spectral energy distribution modelling \|Jin Chichuan Ward Martin et al. \| MNRAS \| 420-1825 \| 2012 \| 2012MNRAS.420.1825J \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.420.1825J 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 Are Optically Selected Quasars Universally X-Ray Luminous? X-Ray-UV Relations in Sloan Digital Sky Survey Quasars \|Gibson Robert R. Brandt W. 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Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H A combined optical and X-ray study of unobscured type 1 active galactic nuclei - III. Broad-band SED properties \|Jin Chichuan Ward Martin \| MNRAS \| 425-907 \| 2012 \| 2012MNRAS.425..907J \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.425..907J The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page M. J. Brindle C. et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P On the Iwasawa-Taniguchi effect of radio-quiet AGN \|Bianchi S. Guainazzi M. et al. \| A&A \| 467-19 \| 2007 \| 2007A&A...467L..19B \| http://ui.adsabs.harvard.edu/#abs/2007A&A...467L..19B Using the Bright Ultrahard XMM-Newton survey to define an IR selection of luminous AGN based on WISE colours \|Mateos S. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2005-05-23T16:10:55Z/2005-12-11T04:47:24Z
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	2007-12-12T00:00:00Z
Last Update	2025-01-27
Keywords	"estimated density", "partially obscured quasars", "xmm survey", "SDSS", "obscured qsos", "local universe", "otherwise normal quasars", "special class", "luminous broad halpha", "XMM", "oiii ].", "balmer decrements", "xray background"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stefanie Komossa, 2007, 'Partially obscured quasars in the local universe', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-uiagipw