A dataset provided by the European Space Agency

Name 060198
Title Cluster and galaxy interactions in dense environment: Shapley supercluster core
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601980101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601980201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601980301

DOI 10.5270/esa-6pdszt7
Author Dr Herve Bourdin
Description The Shapley Supercluster core hosts a remarkably dense structure showing three galaxy clusters --A3562 A3558, A3556-- and two galaxy groups --SC1327-312, SC1329-313-- connected to each other by a filament of hot gas and galaxies. This proposal aims at completing archive data in order to cover continously this filamentary structure. A combined analysis of X-ray data and optical surveys will enable us to investigate thermodynamics of the ICM overcoming group and cluster interactions in the area, and constrain the influence of galaxy-ICM interactions in the global budget of the environmental effects affecting galaxy evolution. We will further search for X-ray emission from the hottest and densest phase of the WHIM, by separating ICM and filament emissions.
Publication Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Shapley Supercluster Survey: ram-pressure stripping versus tidal interactions in the Shapley supercluster . Merluzzi, P., Busarello, G., et all. . MNRAS . 460-3345 . 2016 . 2016MNRAS.460.3345M ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-07-03T15:33:41Z/2009-07-04T18:36:16Z
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 2010-08-18T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-08-18T00:00:00Z, 060198, 17.56_20190403_1200. https://doi.org/10.5270/esa-6pdszt7