A dataset provided by the European Space Agency

Name 020713
Title THE MOST X-RAY LUMINOUS QSOS FROM THE ROSAT BRIGHT SURVEY
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0207130201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0207130401

DOI 10.5270/esa-l8yuoou
Author Dr GEORG LAMER
Description The QSOs RBS 1423 (z=2.26) and RBS 825 (z=1.57) are the most X-ray luminous radio quiet AGN in the ROSAT bright source catalogue. No radio quiet QSOs of comparable X-ray flux and luminosity have so far been observed by XMM-Newton or Chandra. We propose to obtain high quality EPIC spectra for both QSOs in order to investigate the reprocessing of the primary X-ray emission in high luminosity AGN. Due to the redshift of the objects important spectral features as the 6.4 keV iron fluorescence line, the iron 7.11 keV absorption edge and the Compton reflection hump are redshifted to favourable energies.
Publication Strange magnification pattern in the large separation lens SDSS J1004+4112 from optical to X-rays . Lamer, G., Schwope, A., et all. . A&A . 454-493 . 2006 . 2006A&A...454..493L ,
RBS1423 - a new QSO with relativistic reflection from an ionised disk . Krumpe, M., Lamer, G., et all. . A&A . 470-497 . 2007 . 2007A&A...470..497K ,
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 Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars . Young, M., Elvis, M., . ApJ . 708-1388 . 2010 . 2010ApJ...708.1388Y ,
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 ,
New constraints on the X-ray spectral properties of type 1 active galactic nuclei . Scott, A. E., Stewart, G. C., et all. . MNRAS . 417-992 . 2011 . 2011MNRAS.417..992S ,
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 ,
A combined optical and X-ray study of unobscured type 1 active galactic nuclei - I. Optical spectra and spectral energy distribution modelling . Jin, Chichuan, Ward, Martin, et all. . MNRAS . 420-1825...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-04-20T02:58:18Z/2005-02-11T22:25:44Z
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 2006-07-08T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-07-08T00:00:00Z, 020713, 17.56_20190403_1200. https://doi.org/10.5270/esa-l8yuoou