A dataset provided by the European Space Agency

Name 009005
Title STUDY OF A COMPLETE SAMPLE OF BROAD LINE RADIO GALAXIES
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0090050601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0090050701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0090050801

DOI 10.5270/esa-dpdabum
Author Dr Paola Grandi
Description We propose the observation of a complete sample of Broad Line Radio Galaxies (BLRG) extracted by the Wall and Peacock (1985) 2.7 GHz survey. Previous X-ray observations have shown that there is a considerable spectral variety among the BLRG and important differences respect to Seyfert 1. The cold material responsible for the fluorescence iron line and the reflection hump seems to be absent in some radio galaxies or, if present, not necessarily near to the primary X-ray source. Beamed radiation associated to a jet could also significantly contribute to the X-ray emission.
Publication 1WGA J2223.7-0206: A Narrow-Line Quasi-Stellar Object in the XMM-Newton field of view of 3C 445 . Grandi, P., Foschini, L., et all. . A&A . 418-907 . 2004 . 2004A&A...418..907G ,
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 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 ,
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 ,
X-ray colour-colour selection for heavily absorbed active galactic nuclei . Brightman, Murray, Nandra, Kirpal, . MNRAS . 422-1166 . 2012 . 2012MNRAS.422.1166B ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-03-17T09:55:01Z/2001-12-06T11:34:53Z
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 2003-01-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-01-25T00:00:00Z, 009005, 17.56_20190403_1200. https://doi.org/10.5270/esa-dpdabum