A dataset provided by the European Space Agency

Proposal ID 050620
Title The drop structure in the 1H 0707-495: Revealing the physics behind the phenomen
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DOI https://doi.org/10.5270/esa-eie74o9
Principal Investigator, PI Dr Luigi Gallo
Abstract The Narrow-Line Seyfert 1 galaxy (NLS1) 1H 0707-495 exhibits a sharp spectralfeature at energies around 7 keV. Both blurred ionised disc reflection andpartial-covering can be used to explain the observed broad-band properties of 1H0707-495, as both models reproduce very similar spectra in low-flux states.However, long term monitoring and a single deep observation will distinguish thecorrect, physically motivated AGN model, and permit us to probe the physics atwork. 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.
Publications
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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Keywords "broad band properties", "1h 0707 495", "low flux", "sharp spectral", "narrow line seyfert", "drop structure", "x 240", "models reproduce", "single deep"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Luigi Gallo, 2008, 'The drop structure in the 1H 0707-495: Revealing the physics behind the phenomen', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-eie74o9