A dataset provided by the European Space Agency

Name 050620
Title The drop structure in the 1H 0707-495: Revealing the physics behind the phenomen
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506200201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506200301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506200401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506200501

DOI 10.5270/esa-eie74o9
Author Dr Luigi Gallo
Description The Narrow-Line Seyfert 1 galaxy (NLS1) 1H 0707-495 exhibits a sharp spectral feature at energies around 7 keV. Both blurred ionised disc reflection and partial-covering can be used to explain the observed broad-band properties of 1H 0707-495, as both models reproduce very similar spectra in low-flux states. However, long term monitoring and a single deep observation will distinguish the correct, physically motivated AGN model, and permit us to probe the physics at work. We propose to examine 1H 0707-495 for 400 ks. A combination of monitoring (4 x 40 ks) and a deep pointing (1 x 240 ks) will be used.
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An XMM-Newton Survey of the So...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-05-14T02:19:28Z/2007-07-06T22:34:29Z
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 2008-12-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-12-12T00:00:00Z, 050620, 17.56_20190403_1200. https://doi.org/10.5270/esa-eie74o9