A dataset provided by the European Space Agency

Name 055096
Title Disclosing the X-ray properties of Type 2 QSO
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550960101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550960301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550960601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550960801

DOI 10.5270/esa-twfa5at
Author Dr Roberto Della Ceca
Description The study of the X-ray spectral properties of type 2 QSO has fundamental consequence on several hot topics related to the AGN physics. The understanding of their X-ray spectral properties is, however, still limited. We propose XMM-Newton observations of 7 QSO2 belonging to the XMM Bright Survey. This QSO2 sample is unique at the moment: the objects are bright (both in X-ray and in the optical), they belong to a complete survey, and multi-wavelength data have been already accumulated. In particular for 5 objects we have Spitzer proprietary data (allowing us for a detailed investigation to characterize their infrared properties), while good optical spectra are available for all the objects (enabling for a detailed investigation of the AGN narrow line region as well as its host galaxy).
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The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
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X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation . Molham, Mona, Clerc, Nicolas, et all. . MNRAS . 494-161 . 2020 . 2020MNRAS.494..161M ,
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks . Kosiba, Matej, Lieu, Maggie, et all. . MNRAS . 496-4141 . 2020 . 2020MNRAS.496.4141K ,
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-11-26T17:48:24Z/2009-02-02T03:00:48Z
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 2010-03-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-03-06T00:00:00Z, 055096, 17.56_20190403_1200. https://doi.org/10.5270/esa-twfa5at