A dataset provided by the European Space Agency

Name: X-ray Emission Mechanisms in NGC 1068
Published: 2002-08-14T00:00:00Z

Proposal ID	011120
Title	X-ray Emission Mechanisms in NGC 1068
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111200101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111200201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111200301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111200401
DOI	https://doi.org/10.5270/esa-3eyhd7m
Principal Investigator, PI	Dr Albert Brinkman
Abstract	GT - The X-ray spectra of Seyfert II galaxies are rich in discrete emissionfeatures produced in a wide variety of physical conditions. Reprocessedemission may originate from the active nucleus while the host galaxy may emitthermal emission from starburst regions that may or may not be coupled withnuclear activity. We plan to observe NGC 1068, the brightest in its class, toobtain well-exposed, high resolution spectra. We will be able to distinguishthe emission mechanisms and their relative flux contributions to constrain thephysical conditions and structure of the circumnuclear environment.
Publications	The high energy emission line spectrum of NGC 1068 \|Matt G. Bianchi S. et al. \| A&A \| 414-155 \| 2004 \| 2004A&A...414..155M \| http://ui.adsabs.harvard.edu/#abs/2004A&A...414..155M 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 A revision of the X-ray absorption nature of BALQSOs \|Streblyanska A. Barcons X. et al. \| A&A \| 515-2 \| 2010 \| 2010A&A...515A...2S \| http://ui.adsabs.harvard.edu/#abs/2010A&A...515A...2S 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. 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Jiang Linhua et al. \| ApJ \| 692-758 \| 2009 \| 2009ApJ...692..758G \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...692..758G The quest for Type 2 quasars: Chandra observations of luminous obscured quasars in the Sloan Digital Sky Survey \|Vignali Cristian Alexander Dave M. \| MNRAS \| 373-321 \| 2006 \| 2006MNRAS.373..321V \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.373..321V The XMM-Newton serendipitous survey. VI. The X-ray luminosity function \|Ebrero J. Carrera F. J. et al. \| A&A \| 493-55 \| 2009 \| 2009A&A...493...55E \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493...55E Uncovering Obscured Active Galactic Nuclei in Homogeneously Selected Samples of Seyfert 2 Galaxies \|LaMassa Stephanie M. Heckman T. 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Kathy et al. \| MNRAS \| 463-1929 \| 2016 \| 2016MNRAS.463.1929M \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.1929M High-Energy Astrophysics and the Virtual Observatory \|Padovani Paolo \| ChJAS \| 6-73 \| 2006 \| 2006ChJAS...6a..73P \| http://ui.adsabs.harvard.edu/#abs/2006ChJAS...6a..73P Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>~1 and their Galaxy Populations \|Fassbender Rene \| PhDT \| 0-116 \| 2008 \| 2008PhDT.......116F \| http://ui.adsabs.harvard.edu/#abs/2008PhDT.......116F Catalogue of ionized emission line spectra in obscured AGN \|Guainazzi M. Barbarisi I. et al. \| AdSpR \| 41-1998 \| 2008 \| 2008AdSpR..41.1998G \| http://ui.adsabs.harvard.edu/#abs/2008AdSpR..41.1998G AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2000-07-29T01:05:13Z/2000-07-30T16:33:06Z
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	2002-08-14T00:00:00Z
Last Update	2025-01-27
Keywords	"nuclear activity", "physical conditions", "resolution spectra", "active nucleus", "xray spectra", "discrete emission", "NGC 1068", "starburst region", "relative flux contributions", "ngc 1068", "reprocessed emission", "seyfert ii galaxy", "emission mechanisms", "emit thermal emission"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Albert Brinkman, 2002, 'X-ray Emission Mechanisms in NGC 1068', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3eyhd7m