A dataset provided by the European Space Agency

Name 055045
Title XMM-Newton observations of a complete sample of INTEGRAL detected AGN
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550450101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550450301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550450501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550450701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550450901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550451101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550451201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550451301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550451501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550451601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550451701
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550451801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550451901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550452001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550452501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550452601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550452701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550452801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550452901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550453001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550453101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550453201

DOI https://doi.org/10.5270/esa-6t5p3qg
Author Dr Loredana Bassani
Description We propose to observe with XMM-Newton all 22 AGN (from a complete sample of 70
INTEGRAL selected objects), for which no or limited spectral information are
available below 10 keV. XMM observations will allow us to cover the missing
information in the X-ray band and to characterize the broad band emission of
these newly discovered sources. We aim at assessing the role of absorption and
to probe other properties of AGN spectra (power law index, high energy cut-off
reprocessing features). We emphasize here the hard X-ray selection of our
sources and the unique role of INTEGRAL data in providing spectral information
above 10 keV. We estimate that an exposure of 15 ks for each source is enough to
reach the goals of this XMM Large Program proposal.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-11-18T11:41:41Z/2009-04-28T20:44:57Z
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 2010-06-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Loredana Bassani, 2010, 055045, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6t5p3qg