A dataset provided by the European Space Agency

Name 074441
Title The XMM-Newton Cluster Outskirts Project (X-COP)
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744410901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411101
...
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744411901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744412901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744413901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744414001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744414101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744414201

DOI 10.5270/esa-ukqsqpj
Author Dr Dominique Eckert
Description Galaxy cluster outskirts are the regions where structure formation processes are expected to be active across the entire lifetime of these systems through the accretion of smaller structures. After the success of a pilot XMM-Newton program targeting the outer regions of two systems, we propose to map the outskirts of 10 galaxy clusters in the redshift range 0.04-0.1. Through the synergy between XMM and SZ data from Planck, we will recover the thermo-dynamic properties of the gas out to R200 and study the accretion processes in cluster outskirts. We will disentangle for the first time the effects of gas clumping and non-thermal pressure support. In addition, since it will allow us to map the entire volume of several well-known systems, our program will have an important legacy value.
Publication XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Suzaku observations of the merging galaxy cluster Abell 2255: The northeast radio relic . Akamatsu, H., Mizuno, M., et all. . A&A . 600-100 . 2017 . 2017A&A...600A.100A ,
The XMM cluster outskirts project (X-COP) . Eckert, D., Ettori, S., et all. . AN . 338-293 . 2017 . 2017AN....338..293E ,
Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity . Ettori, S., Ghirardini, V., et all. . MNRAS . 470-29 . 2017 . 2017MNRAS.470L..29E ,
X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L ,
PSZ2LenS. Weak lensing analysis of the Planck clusters in the CFHTLenS and in the RCSLenS . Sereno, Mauro, Covone, Giovanni, et all. . MNRAS . 472-1946 . 2017 . 2017MNRAS.472.1946S ,
The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the intracluster medium out to R200 in Abell 2319 . Ghirardini, V., Ettori, S., et all. . A&A . 614-7 . 2018 . 2018A&A...614A...7G ,
Thermodynamic profiles of galaxy clusters from a joint X-ra...
Instrument EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage 2014-03-14T06:30:32Z/2015-12-17T11:00:38Z
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 2016-03-02T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016-03-02T23:00:00Z, 074441, 17.56_20190403_1200. https://doi.org/10.5270/esa-ukqsqpj