A dataset provided by the European Space Agency

Name 000294
Title XMM study of a sample of nuclear dust morphology selected Seyfert 2 galaxies
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002940101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002940301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002940401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002940701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002940901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002942301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002942401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0002942501

DOI 10.5270/esa-vwuwekp
Author Dr Matteo Guainazzi
Description Guainazzi et al. (1999, in preparation) recently discovered that the nuclear dust content and the optical reddening appear to be anticorrelated with the amount of X-ray absorption, leading to the suggestion that the absorbing matter in Compton-thin and -thick Seyfert 2 galaxies is qualitatively different. One of the most crucial correlation, nuclear dust versus Compton-thickness, is significant only at 1 sigma confidence level. We propose to enlarge the sample of objects for which high-resolution images of the nuclear region and X-ray measurements of the absorbing column exist, by observing further 24 objects with XMM. This will permit to establish this correlation, if true, at a confidence level >98. Total 205 ks of exposure time are requested.
Publication Chandra and XMM-Newton observations of Tololo 0109-383 . Matt, G., Bianchi, S., et all. . A&A . 399-519 . 2003 . 2003A&A...399..519M ,
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 ,
A search for changing-look AGN in the Grossan catalog . Bianchi, S., Guainazzi, M., et all. . A&A . 442-185 . 2005 . 2005A&A...442..185B ,
Suzaku observation of the Phoenix galaxy . Matt, G., Bianchi, S., et all. . A&A . 496-653 . 2009 . 2009A&A...496..653M ,
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 ,
On the origin of soft X-rays in obscured AGN: answers from high-resolution spectroscopy with XMM-Newton . Guainazzi, Matteo, Bianchi, Stefano, . MNRAS . 374-1290 . 2007 . 2007MNRAS.374.1290G ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
Average Fe Kalpha emission from distant AGN...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-01-05T05:57:30Z/2002-01-28T22:38:10Z
Version PPS_NOT_AVAILABLE
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 2010-04-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-04-09T00:00:00Z, 000294, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-vwuwekp