A dataset provided by the European Space Agency

Name: Cluster and galaxy interactions in dense environment: Shapley supercluster core
Published: 2010-08-18T00:00:00Z

Proposal ID	060198
Title	Cluster and galaxy interactions in dense environment: Shapley supercluster core
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601980101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601980201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0601980301
DOI	https://doi.org/10.5270/esa-6pdszt7
Principal Investigator, PI	Dr Herve Bourdin
Abstract	The Shapley Supercluster core hosts a remarkably dense structure showing threegalaxy clusters --A3562 A3558, A3556-- and two galaxy groups --SC1327-312,SC1329-313-- connected to each other by a filament of hot gas and galaxies. Thisproposal aims at completing archive data in order to cover continously thisfilamentary structure. A combined analysis of X-ray data and optical surveyswill enable us to investigate thermodynamics of the ICM overcoming group andcluster interactions in the area, and constrain the influence of galaxy-ICMinteractions in the global budget of the environmental effects affecting galaxyevolution. We will further search for X-ray emission from the hottest anddensest phase of the WHIM, by separating ICM and filament emissions.
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Shapley Supercluster Survey: ram-pressure stripping versus tidal interactions in the Shapley supercluster \|Merluzzi, P., Busarello, G., et al. \| MNRAS \| 460-3345 \| 2016 \| 2016MNRAS.460.3345M \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.460.3345M The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Radio footprints of a minor merger in the Shapley Supercluster: From supercluster down to galactic scales \|Venturi, T., Giacintucci, S., et al. \| A&A \| 660-81 \| 2022 \| 2022A&A...660A..81V \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..81V Two large-scale sloshing cold fronts in the outskirts of the galaxy cluster Abell 3558 \|Mirakhor, M. S., Walker, S. A., et al. \| MNRAS \| 526-124 \| 2023 \| 2023MNRAS.526L.124M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526L.124M From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 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	2010-08-18T00:00:00Z
Keywords	"sc1327 312", "sc1329 313 connected", "xray data", "filamentary structure", "combined analysis", "separating icm", "densest phase", "galaxy icm interactions", "dense structure", "global budget", "filament emissions", "icm overcoming", "cluster interactions", "cover continously", "shapley supercluster core", "completing archive data", "hot gas", "galaxy interactions", "xray emission", "optical surveys"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Herve Bourdin, 2010, 'Cluster and galaxy interactions in dense environment: Shapley supercluster core', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6pdszt7