A dataset provided by the European Space Agency

Name: STUDIES OF COMPLEX FE-LINE EMISSION IN LLAGN AND LINERS
Published: 2004-07-01T00:00:00Z

Proposal ID	011284
Title	STUDIES OF COMPLEX FE-LINE EMISSION IN LLAGN AND LINERS
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112840101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112840201
DOI	https://doi.org/10.5270/esa-i45dj38
Principal Investigator, PI	Prof RICHARD GRIFFITHS
Abstract	GT - We propose to determine whether complex, possibly ionized Fe-K emissionis present in M81, NGC4579 and M51 as suggested by examination ofASCA data. We will constrain the energy of the line centroid and thus resolve whether the line-emitting gas is ionized. The line E.W. will be used as a diagnostic to discriminate between various models for the originof the Fe-K lines. Constraints on the line profiles will be used toindicate the extent of any relativistic line broadening or line complexity.
Publications	Long-term Spectral Variations of Ultraluminous X-ray Sources in the Interacting Galaxy Systems M 51 and NGC 4490/85 \|Yoshida Tessei Ebisawa Ken et al. \| ApJ \| 722-760 \| 2010 \| 2010ApJ...722..760Y \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...722..760Y Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton \|Matsushita K. \| A&A \| 527-134 \| 2011 \| 2011A&A...527A.134M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.134M 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 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 Studying the X-ray/UV Variability of Active Galactic Nuclei with data from Swift and XMM archives \|Turriziani Sara \| JPhCS \| 280-12005 \| 2011 \| 2011JPhCS.280a2005T \| http://ui.adsabs.harvard.edu/#abs/2011JPhCS.280a2005T 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 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 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 On the nature of high X-ray luminosities in Sloan Digital Sky Survey galaxies \|Jackson F. E. Roberts T. P. et al. \| MNRAS \| 422-2 \| 2012 \| 2012MNRAS.422....2J \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422....2J 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 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 2XMM ultraluminous X-ray source candidates in nearby galaxies \|Walton D. J. Roberts T. P. et al. \| MNRAS \| 416-1844 \| 2011 \| 2011MNRAS.416.1844W \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.416.1844W X-ray spectral survey with XMM-Newton of a complete sample of nearby Seyfert galaxies \|Cappi M. Panessa F. et al. \| A&A \| 446-459 \| 2006 \| 2006A&A...446..459C \| http://ui.adsabs.harvard.edu/#abs/2006A&A...446..459C Iron Kalpha Emission from the Low-Luminosity Active Galaxies M81 and NGC 4579 \|Dewangan G. C. Griffiths R. 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N. \| ApJ \| 685-773 \| 2008 \| 2008ApJ...685..773G \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...685..773G 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 Statistics of relativistically broadened Fe Kalpha lines in AGN \|Guainazzi M. Bianchi S. \| AN \| 327-1032 \| 2006 \| 2006AN....327.1032G \| http://ui.adsabs.harvard.edu/#abs/2006AN....327.1032G Ultra-luminous sources in nearby galaxies \|Mushotzky Richard \| AdSpR \| 38-2793 \| 2006 \| 2006AdSpR..38.2793M \| http://ui.adsabs.harvard.edu/#abs/2006AdSpR..38.2793M A large catalogue of ultraluminous X-ray source candidates in nearby galaxies \|Walton D. J. Gladstone J. C. et al. \| AN \| 332-354 \| 2011 \| 2011AN....332..354W \| http://ui.adsabs.harvard.edu/#abs/2011AN....332..354W An XMM-Newton spectral survey of 12 mum selected galaxies - I. 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Caccianiga A. \| A&A \| 542-46 \| 2012 \| 2012A&A...542A..46S \| http://ui.adsabs.harvard.edu/#abs/2012A&A...542A..46S The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L CAIXA: a catalogue of AGN in the XMM-Newton archive. III. Excess variance analysis \|Ponti G. Papadakis I. et al. \| A&A \| 542-83 \| 2012 \| 2012A&A...542A..83P \| http://ui.adsabs.harvard.edu/#abs/2012A&A...542A..83P Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Detectability of low-energy X-ray spectral components in type 1 active galactic nuclei \|Scott A. E. Stewart G. 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Alonso-Herrero A. et al. \| MNRAS \| 426-3271 \| 2012 \| 2012MNRAS.426.3271M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426.3271M Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau F.-X. Motch C. et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi J. A. Albacete Colombo J. F. et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 \|Ballo L. Heras F. J. H. et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B X-Ray Properties of the Northern Galactic Cap Sources in the 58 Month Swift/BAT Catalog \|Vasudevan Ranjan V. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2003-01-15T13:12:55Z/2003-06-12T15:09:47Z
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	2004-07-01T00:00:00Z
Last Update	2025-01-27
Keywords	"relativistic line broadening", "line centroid", "NGC4579", "line complexity", "ionized fe", "asca data", "M81", "line profiles", "line emitting gas"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof RICHARD GRIFFITHS, 2004, 'STUDIES OF COMPLEX FE-LINE EMISSION IN LLAGN AND LINERS', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-i45dj38