A dataset provided by the European Space Agency

Name 009303
Title Confronting the Complexity of Galaxy Clusters with Lensing, SZ, and XMM Data
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093030101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093030201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093030301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093030801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093030901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093031001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093031101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093031401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093031501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093031601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093031701
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0093031801

DOI https://doi.org/10.5270/esa-0eutyae
Author Prof John P. Hughes
Description We propose to observe with XMM a small sample of galaxy clusters to
obtain temperature maps with good precision. Our sample consists of
clusters that have SZE images, weak and/or strong gravitational
lensing maps, and are bright X-ray sources. The combination of
lensing, X-ray, and SZE data will allow us to measure the Hubble
constant, derive a model-independent value for the baryon fraction,
and test common assumptions in estimating cluster dark matter,
including hydrostatic equilibrium, spherical symmetry, and minimal
substructure.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-12-24T04:12:20Z/2004-02-07T07:38:18Z
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 2005-04-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof John P. Hughes, 2005, 009303, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0eutyae