A dataset provided by the European Space Agency

Proposal ID 094506
Title X-EDFF
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060131
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060132
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060133
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060134
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060135
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060136
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060137
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060138
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0945060139

DOI https://doi.org/10.57780/esa-6zn2ipd
Principal Investigator, PI Dr Marguerite Pierre
Abstract The 10 deg2 Euclid Deep Fornax Field (EDFF) will be the foremost extragalacticmedium-area deep field due to its unique multi-lambda coverage. We aim toprovide the X-ray view by mapping the entire EDFF at 40ks depth for untoldlegacy value. The XMM data and associated surveys will enable major advances inthe study of AGN and galaxy clusters, including: deep characterisation of Euclidclusters and their selection function; robust measures of cluster scalingrelations to z=1.5 and the group regime; the study of rare clusters and AGN in avariety of environments; and revealing the link between AGN feedback and starformation to z>3. We will deliver a complete, validated multi-lambda legacydataset that will greatly enhance the AGN and cluster science from the 15,000 deg2 Euclid Wide survey.
Publications No publications found for current proposal!
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2024-08-21T23:32:39Z/2024-08-23T00:32:21Z
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 2024-08-22T00:00:00Z
Last Update 2025-01-27
Keywords XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Marguerite Pierre, 2024, 'X-EDFF', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.57780/esa-6zn2ipd