A dataset provided by the European Space Agency

Name 000681
Title An XMM Study of the Bright Narrow-Line Seyfert 1 Galaxy Arakelian 564
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0006810101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0006810201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0006810301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0006810401

DOI 10.5270/esa-41a2yud
Author Prof William Brandt
Description X-ray observations of Narrow-Line Seyfert 1 galaxies (NLS1) continue to drive our understanding of the Seyfert phenomenon, and physical models for NLS1 suggest that they have extreme values of mass accretion rate or nuclear orientation. We propose an XMM study of Akn 564, one of the X-ray brightest and most interesting NLS1, that will test these NLS1 models. We will study the shape and variability of its energetically dominant soft X-ray excess to determine its origin and test the idea that NLS1 are characterized by high mass accretion rates. We will also study spectral features at low energy to determine if they originate in an ionized accretion disk. We will use the broad FeK line profile to constrain the inner disk inclination and test nuclear orientation models.
Publication Exploring the X-ray sky with the XMM-Newton bright serendipitous survey . Della Ceca, R., Maccacaro, T., et all. . A&A . 428-383 . 2004 . 2004A&A...428..383D ,
Arakelian 564: an XMM-Newton view . Vignali, Cristian, Brandt, W. N., et all. . MNRAS . 347-854 . 2004 . 2004MNRAS.347..854V ,
Exploring the nuclear environment of the NLS1 galaxy Arakelian 564 with XMM-Newton RGS . Smith, R. A. N., Page, M. J., . A&A . 490-103 . 2008 . 2008A&A...490..103S ,
High-precision multi-band measurements of the angular clustering of X-ray sources . Ebrero, J., Mateos, S., et all. . A&A . 500-749 . 2009 . 2009A&A...500..749E ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
Investigating the nature of narrow-line Seyfert 1 galaxies with high-energy spectral complexity . Gallo, L. C., . MNRAS . 368-479 . 2006 . 2006MNRAS.368..479G ,
Spe...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-06-17T03:48:06Z/2001-06-09T11:55:56Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2003-01-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-01-22T00:00:00Z, 000681, 17.56_20190403_1200. https://doi.org/10.5270/esa-41a2yud