A dataset provided by the European Space Agency

Name 055391
Title The XMM-LSS Survey: re-observation of AO5 LP pointings affected by radiation
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553910901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911101
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553911901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553912001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553912101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553912201

DOI https://doi.org/10.5270/esa-0cytdkr
Author Dr Marguerite Pierre
Description We propose to re-observe 19 XMM-LSS AO5 fields significantly affected by radiation during AO5 operations. They are part of the XMM Large Programme dedicated to full coverage of the Spitzer SWIRE legacy survey. Given the modest nominal observing time per pointing (10 ks), full exposure and low background over the entire area are necessary to fulfil the survey goals: studies of cluster number counts, the evolution of clusters and cluster galaxies, the AGN correlation function, and multi-lambda analysis of the AGN population.
Publication No observations found associated with the current proposal
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2010-01-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-01-27T00:00:00Z, 055391, 17.56_20190403_1200. https://doi.org/10.5270/esa-0cytdkr