| Proposal ID | 005975 |
| Title | Understanding the X-ray source population through an XMM survey of ELAIS fields |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0059750101 |
| DOI | https://doi.org/10.5270/esa-5f255cw |
| Principal Investigator, PI | Dr Robert Mann |
| Abstract | We request 450ks, to survey with EPIC 3 sq. deg. we mapped with ISO at 7, 15,90 and 175 microns, and followed up in the optical, near-IR and radio, to give:(i) a sample of ~1000 X-ray galaxies, allowing selection of statisticallyrepresentative subsamples of galaxies by activity Seyfert 1, Seyfert 2,starburst, by X-ray luminosity and by degree of obscuration;(ii) X-ray spectral information for a large sample of galaxies for which there is excellent multi-wavelength data from the radio to the UV;(iii) the best opportunity of resolving, through direct IR to X-ray comparisons,the issue of dust extinction in AGN, and of determining the contributions ofstarbursts and dust-obscured AGN to the cosmic far-infrared background. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2002-04-11T18:47:07Z/2002-10-28T14:26:24Z |
| Version | PPS_NOT_AVAILABLE |
| 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 | 2005-01-01T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "", "dust obscured agn", "EPIC", "xray comparisons", "xmm survey", "175 microns", "dust extinction", "xray galaxy", "xray source population", "starburst ]", "XMM", "infrared background", "multi wavelength data", "xray luminosity", "elais fields" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Robert Mann, 2005, 'Understanding the X-ray source population through an XMM survey of ELAIS fields', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-5f255cw |