We propose to re-observe 19 XMM-LSS AO5 fields significantly affected byradiation during AO5 operations. They are part of the XMM Large Programmededicated to full coverage of the Spitzer SWIRE legacy survey. Given the modestnominal observing time per pointing (10 ks), full exposure and low backgroundover the entire area are necessary to fulfil the survey goals: studies ofcluster number counts, the evolution of clusters and cluster galaxies, the AGNcorrelation function, and multi-lambda analysis of the AGN population.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2008-07-03T07:32:33Z/2009-01-04T06:15:12Z
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.
European Space Agency, Dr Marguerite Pierre, 2010, 'The XMM-LSS Survey: re-observation of AO5 LP pointings affected by radiation', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0cytdkr
