A dataset provided by the European Space Agency

Proposal ID 074441
Title The XMM-Newton Cluster Outskirts Project (X-COP)
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DOI https://doi.org/10.5270/esa-ukqsqpj
Principal Investigator, PI Dr Dominique Eckert
Abstract Galaxy cluster outskirts are the regions where structure formation processes areexpected to be active across the entire lifetime of these systems through theaccretion of smaller structures. After the success of a pilot XMM-Newton programtargeting the outer regions of two systems, we propose to map the outskirts of10 galaxy clusters in the redshift range 0.04-0.1. Through the synergy betweenXMM and SZ data from Planck, we will recover the thermo-dynamic properties ofthe gas out to R200 and study the accretion processes in cluster outskirts. Wewill disentangle for the first time the effects of gas clumping and non-thermalpressure support. In addition, since it will allow us to map the entire volumeof several well-known systems, our program will have an important legacy value.
Publications
Instrument RGS1, EPN, RGS2, EMOS1, OM, EMOS2
Temporal Coverage 2014-03-14T06:30:32Z/2015-12-17T11:00:38Z
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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2016-03-02T23:00:00Z
Keywords "gas clumping", "nonthermal pressure support", "accretion processes", "XMM", "galaxy cluster outskirts", "sz data", "redshift range", "galaxy cluster", "thermo dynamic properties", "structure formation processes", "XMM-Newton", "cluster outskirts", "outer region"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Dominique Eckert, 2016, 'The XMM-Newton Cluster Outskirts Project openParX-COPclosePar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ukqsqpj