A dataset provided by the European Space Agency

Name 030238
Title A Search for Unusual X-ray Properties in High-z, High-Accretion Rate Quasars
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302380201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302380401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302380501

DOI 10.5270/esa-sprdm6g
Author Dr Ohad Shemmer
Description We propose to observe four of the most luminous quasars known, which have extremely high accretion rates and are at redshift ~2-3, using XMM-Newton EPIC PN and MOS with a total integration time of 135 ksec. We will obtain accurate measurements of the spectral slope in the quasars. ~1.5-20 keV rest-frame band and look for X-ray variations. Our prime goal is to test whether the X-ray spectral slope is an accretion-rate indicator for all AGN. Steep X-ray spectral slopes may identify our sources as the long sought high-redshift analogs of narrow-line Seyfert 1 galaxies.
Publication 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 ,
Can the Soft X-Ray Opacity Toward High-redshift Sources Probe the Missing Baryons? . Behar, Ehud, Dado, Shlomo, et all. . ApJ . 734-26 . 2011 . 2011ApJ...734...26B ,
The Hard X-Ray Spectral Slope as an Accretion Rate Indicator in Radio-quiet Active Galactic Nuclei . Shemmer, Ohad, Brandt, W. N., et all. . ApJ . 646-29 . 2006 . 2006ApJ...646L..29S ,
Statistics of relativistically broadened Fe Kalpha lines in AGN . Guainazzi, M., Bianchi, S., . AN . 327-1032 . 2006 . 2006AN....327.1032G ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Fe Kalpha line profile in AGNs: average shape and redshift dependence . Mao, Wei-Ming, Hu, Chen, et all. . RAA . 10-905 . 2010 . 2010RAA....10..905M ,
CAIXA: a catalogue of AGN in th...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-07-05T07:13:35Z/2005-11-01T06:25:41Z
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 2006-12-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-12-01T00:00:00Z, 030238, 17.56_20190403_1200. https://doi.org/10.5270/esa-sprdm6g