A dataset provided by the European Space Agency

Name 010386
Title Probing the unification model of AGN TS22
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103860901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861101
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103861901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103862001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103862101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103862401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103862501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103862601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103862701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103862801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103862901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103863001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103863101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0103863201

DOI https://doi.org/10.5270/esa-9at2z1v
Author Dr Bernd Aschenbach
Description GT-Unification models assume the same physical emission process in the center of
active galaxies and explain spectral differences with different viewing angles
and obscuration by a dense gas torus. The hard X-ray continua of active galaxies
are expected to show the canonical value of 1.9 known from Seyfert 1 galaxies
and QSOs. We intent to check this hypothesis by our RASS selected sample. We
propose Seyfert 1, Seyfert1.2, 1.5, 1.8, 1.9, 2, NLS1 and LINERs for detailed
spectral analysis primarily in the hard but also in the soft band using the EPIC
cameras as prime instrument. As a side product we will be able to explore a
possible spatial extent (halo), time variability, presence of warm absorbers and
spectra of gaseous components.
Publication No observations found associated with the current proposal
Instrument EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage 2000-08-29T21:06:09Z/2002-12-20T00:49:06Z
Version PPS_NOT_AVAILABLE
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 2004-04-13T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Bernd Aschenbach, 2004, 010386, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-9at2z1v