A dataset provided by the European Space Agency

Name 040538
Title X-ray Emission of Seyfert 2 Galaxies: Contribution of Star-Forming Processes
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405380201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405380301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405380501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405380701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405380801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405380901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405381001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405381101

DOI 10.5270/esa-49tn9w4
Author Dr Elena Jimenez-Bailon
Description We propose to study the SB-AGN connection in a representative sample of Seyfert 2 galaxies in which the stellar population have been analysed using state-of-the-art population synthesis models in the optical-UV. By extending the results of the optical modeling to X-rays, we can infer the amount of energy in the X band produced by the SB and compare it with the energy from the central engine. Interestingly, this will allow us to elucidate the nature of the soft X-ray emission in Seyfert 2s, which is still largely unknown. The lack of well studied samples of Seyfert 2s which explore the complementary information provided by optical-UV and X-ray observations in a consistent and well defined manner justifies further analysis using high quality data such as those proposed here.
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-02-01T11:32:43Z/2007-05-01T00:43:31Z
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 2008-05-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-05-31T00:00:00Z, 040538, 17.56_20190403_1200. https://doi.org/10.5270/esa-49tn9w4