A dataset provided by the European Space Agency

Name 011263
Title High Redshift Radio-Quiet Quasars
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112630101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112630201

DOI 10.5270/esa-blt1j6e
Author Dr Martin Turner
Description GT- Observations of luminous high redshift radio-quiet quasars are proposed as part of the XMM GT programme. The aims are to probe the local environment of quasars at high redshift, by means of the intervening absorbing matter. Another goal is to learn more about the central engine from the X-ray continuum plus Fe line - reflection reprocessing. Insight can also be gained into the evolutionary properties of quasars. A specific aim with the radio-quiet quasars will be to study the properties of the central engine, through the reflection component and the properties of the iron K line. Additionally we will test whether X-ray absorption, thought to be associated with high z radio-loud quasars, is present in the radio-quiet objects.
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 ,
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 ,
The XMM-Newton Wide Angle Survey (XWAS): the X-ray spectrum of type-1 AGN . Mateos, S., Carrera, F. J., et all. . A&A . 510-35 . 2010 . 2010A&A...510A..35M ,
Average Fe Kalpha emission from distant AGN . Corral, A., Page, M. J., et all. . A&A . 492-71 . 2008 . 2008A&A...492...71C ,
X-ray absorption in distant type II QSOs . Krumpe, M., Lamer, G., et all. . A&A . 483-415 . 2008 . 2008A&A...483..415K ,
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 all. . NJPh . 13-125014 . 2011 . 2011NJPh...13l5014F ,
Warm-hot intergalactic medium contribution to baryonic matter . Soltan, A. M., . A&A . 460-59 . 2006 . 2006A&A...460...59S ,
Statistical evaluation of the flux cross-calibration of th...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-06-04T02:08:58Z/2001-06-14T19:39:24Z
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 2002-12-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-12-29T00:00:00Z, 011263, 17.56_20190403_1200. https://doi.org/10.5270/esa-blt1j6e