A dataset provided by the European Space Agency

Name 067012
Title Definitive Observations of an Accretion Disk Wind in the Quasar MR 2251-178
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670120201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670120301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670120401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670120501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670120601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670120701

DOI 10.5270/esa-je4486x
Author Dr James Reeves
Description The bright, nearby QSO MR 2251-178 was the first AGN where a warm absorber was detected. Subsequent observations have shown that there are at least two warm absorber components; a low ionisation soft X-ray absorber and a putative high velocity (0.07c) wind. We propose a deep (336 ks total) observation of MR 2251-178 in order to determine the origin of the outflow. Our goals are; (i) to establish the nature of the high ionisation absorber, e.g. as part of a disk wind, through high S-N observations in the iron K band and (ii) obtain a high resolution RGS spectrum of the soft X-ray absorber. Together with our recently approved large Chandra-HST project, this will allow us to deduce the kinematics, location and energetics of the outflow to unprecedented accuracy.
Publication A High Resolution View of the Warm Absorber in the Quasar MR 2251-178 . Reeves, J. N., Porquet, D., et all. . ApJ . 776-99 . 2013 . 2013ApJ...776...99R ,
The puzzling X-ray continuum of the quasar MR 2251-178 . Nardini, E., Reeves, J. N., et all. . MNRAS . 440-1200 . 2014 . 2014MNRAS.440.1200N ,
Warm absorbers in X-rays (WAX), a comprehensive high-resolution grating spectral study of a sample of Seyfert galaxies - I. A global view and frequency of occurrence of warm absorbers. . Laha, Sibasish, Guainazzi, Matteo, et all. . MNRAS . 441-2613 . 2014 . 2014MNRAS.441.2613L ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
X-ray spectral parameters for a sample of 95 active galactic nuclei . Vasylenko, A. A., Zhdanov, V. I., . Ap&SS . 360-71 . 2015 . 2015Ap&SS.360...71V ,
Warm absorbers in X-rays (WAX), a comprehensive high-resolution grating spectral study of a sample of Seyfert Galaxies - II. Warm absorber dynamics and feedback to galaxies . Laha, Sibasish, Guainazzi, Matteo, et all. . MNRAS . 457-3896 . 2016 . 2016MNRAS.457.3896L ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-11-11T17:51:33Z/2011-11-17T07:38:34Z
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 2012-12-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-12-15T00:00:00Z, 067012, 17.56_20190403_1200. https://doi.org/10.5270/esa-je4486x