A dataset provided by the European Space Agency

Name 065557
Title Exploring obscuration in luminous type-2 quasars
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655570101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655570201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655570301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655570401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655570701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655570901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655571001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655571201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655571301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655571401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655571701
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655571801

DOI https://doi.org/10.5270/esa-uu809di
Author European Space Agency
Description The most luminous absorbed AGN (QSO2) have been predicted in considerable
numbers by cosmic X-ray background models. However, their space density
and contribution to the AGN luminosity output remain uncertain. Taking
advantage of the high throughput and good spectral resolution of the
EPIC cameras, we propose XMM-Newton observations of 16 QSO2 at
z=0.1-0.17 drawn from the Sloan Digital Sky Survey. The sample, solely
based on the high luminosity of the [OIII] 5007A line, is unbiased
against heavily absorbed AGN. We will constrain the properties of QSO2 and
investigate the effect of luminosity on the AGN obscuration.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-05-28T07:08:47Z/2011-04-27T21:12:14Z
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 2012-05-14T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012, Exploring Obscuration In Luminous Type-2 Quasars, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-uu809di