Proposal ID | 050620 |
Title | The drop structure in the 1H 0707-495: Revealing the physics behind the phenomen |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0506200201 |
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 |
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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 |
Last Update | 2025-01-27 |
Keywords | "x 240", "1h 0707 495", "narrow line seyfert", "models reproduce", "low flux", "broad band properties", "sharp spectral", "drop structure", "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 |