A dataset provided by the European Space Agency

Name 011291
Title Study of the Soft Excess - Warm Absorber in a Sample of AGN
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112910101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112910201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112910301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112910401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112910501

DOI 10.5270/esa-y30orc9
Author Dr Martin Turner
Description GT-A sample of AGN showing structure in their soft X-ray spectra is to be observed. The physics of the spectral structure may be 1) a soft excess component above the underlying power law, possibly from the emission of the accretion disk, or-and 2) selective absorption due to a warm absorber. The candidate objects have been selected by a systematic study of ROSAT PSPC spectra in comparison to hard (2-10 keV) spectra measured by HEAO-1, EXOSAT or Ginga.
Publication The history of the iron Kalpha line profile in the Piccinotti AGN ESO 198-G24 . Guainazzi, M., . A&A . 401-903 . 2003 . 2003A&A...401..903G ,
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 ,
On the variability of the iron Kalpha line in Mrk 841 . Longinotti, A. L., Nandra, K., et all. . MNRAS . 355-929 . 2004 . 2004MNRAS.355..929L ,
Unveiling the broad band X-ray continuum and iron line complex in Mrk 841 . Petrucci, P. O., Ponti, G., et all. . A&A . 470-889 . 2007 . 2007A&A...470..889P ,
High-resolution X-ray spectroscopy of the Seyfert 1 Mrk 841: insights into the warm absorber and warm emitter . Longinotti, A. L., Costantini, E., et all. . A&A . 510-92 . 2010 . 2010A&A...510A..92L ,
PKS 1502+106: A New and Distant Gamma-ray Blazar in Outburst Discovered by the Fermi Large Area Telescope . Abdo, A. A., Ackermann, M., et all. . ApJ . 710-810 . 2010 . 2010ApJ...710..810A ,
X-QUEST: A Comprehensive X-ray Study of Local ULIRGS and QSOs . Teng, Stacy H., Veilleux, Sylvain, . ApJ . 725-1848 . 2010 . 2010ApJ...725.1848T ,
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 , ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-11-29T15:00:12Z/2001-01-13T07:47:16Z
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 2002-03-22T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-03-22T00:00:00Z, 011291, 17.56_20190403_1200. https://doi.org/10.5270/esa-y30orc9