Proposal ID | 072529 |
Title | The XMM-ATLAS survey: AGN - star-formation co-evolution |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0725290101 |
DOI | https://doi.org/10.5270/esa-o2ab6uc |
Principal Investigator, PI | Dr Ioannis Georgantopoulos |
Abstract | We propose to observe the 16 sq. deg. of the Herschel-ATLAS ScienceDemonstration Phase (SDP) in mosaic mode (total requested exposure 700 ks). TheH-ATLAS (PACS+SPIRE) survey covers regions with excellent qualitymulti-wavelength data, including the GAMA AAT spectroscopic survey and near- andmid-IR data from the UKIDSS and WISE surveys. The proposed observations willprovide the largest contiguous area far-IR/sub-mm survey with X-ray follow-up.This area will contain about 6000 250um and 2000 X-ray sources. The majorscientific goals are to place strong constrains on the link between AGN andstar-formation activity in the low-redshift (z<0.5) Universe, and to investigatethe effect of very luminous AGN on their hosts. |
Publications |
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Instrument | RGS1, EPN, RGS2, EMOS1, OM, EMOS2 |
Temporal Coverage | 2013-05-05T03:43:19Z/2013-05-06T11:29:58Z |
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 | 2014-05-21T00:00:00Z |
Last Update | 2025-08-04 |
Keywords | "XMM", "6000 250um", "low redshift z", "largest contiguous", "2000 xray sources", "wise surveys", "major scientific", "star formation activity", "xmm atlas survey", "atlas pacs", "luminous agn", "mid ir data", "sub mm survey" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Ioannis Georgantopoulos, 2014, 'The XMM-ATLAS survey: AGN - star-formation co-evolution', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-o2ab6uc |