A dataset provided by the European Space Agency

Name 011179
Title X-ray spectroscopy of the narrow emission line Seyfert 1 galaxy NGC7314
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111790101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111790201

DOI 10.5270/esa-46rwp0o
Author Dr Bert Brinkman
Description GT - NGC7314 is a narrow emission line galaxy known to exhibit rapid, large amplitude X-ray variability. The RGS and EPIC data will be used to characterise the components of its X-ray spectrum and to study their behaviour over time, while the OM will monitor its optical-UV spectrum. Rapid variability in the Fe K line profile has also been observed, and its behaviour in relation to the continuum X-ray flux will be investigated in detail with the EPIC data.
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Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-05-02T06:31:55Z/2001-05-02T21:58:38Z
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 2002-06-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-06-30T00:00:00Z, 011179, 17.56_20190403_1200. https://doi.org/10.5270/esa-46rwp0o