A dataset provided by the European Space Agency

Name 030258
Title Probing structure formation physics with the evolution of clusters properties
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302580301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302580401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302580501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302580701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302580901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302581101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302581301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302581501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302581601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302581801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302581901
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302582001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302582101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302582201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302582301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302582401

DOI https://doi.org/10.5270/esa-dyz3cwm
Author Dr Monique ARNAUD
Description We propose to observe a large unbiased sample of distant (zvirgul0.5) clusters. The
clusters in the sample cover the wide dynamic range in mass (kT = [2.5-12] keV)
necessary to fully assess the evolution of cluster scaling and structural
properties. This will provide unique insight into the physics of structure
formation, both for the dark matter and the baryonic components (e.g. how
non-gravitational processes drive departures from the predictions of the
simplest self-similar model of gravitational collapse). We propose that the
observations be conducted as a Public Large project.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-06-10T09:04:53Z/2006-06-03T23:07:25Z
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 2008-08-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Monique ARNAUD, 2008, 030258, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-dyz3cwm