A dataset provided by the European Space Agency

Name: Cluster and galaxy interactions in dense environment: Shapley supercluster core
Published: 2011-07-29T00:00:00Z

Proposal ID	065159
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=0651590101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651590201
DOI	https://doi.org/10.5270/esa-pqex4bp
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. Acombined analysis of X-ray and optical data will enable us to investigatethermodynamics of the ICM overcoming group and cluster interactions, andconstrain the influence of galaxy-ICM interactions in the global budget of theenvironmental effects affecting galaxy evolution. We will further search forX-ray emission from the hottest phase of the WHIM, by separating ICM andfilament emissions. Following an AO8 proposal, this proposal aims atre-observing a region where pointings are contaminated by soft protons and extending the observed area.
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 The non-uniformity of galaxy cluster metallicity profiles \|Lovisari L. Reiprich T. H. \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters \|Lagana T. F. Durret F. \| MNRAS \| 484-2807 \| 2019 \| 2019MNRAS.484.2807L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484.2807L 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 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	2010-07-05T12:58:21Z/2010-07-06T04:33:38Z
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	2011-07-29T00:00:00Z
Last Update	2025-01-27
Keywords	"combined analysis", "separating icm", "optical data", "sc1329 313 connected", "filament emissions", "icm overcoming", "hottest phase", "sc1327 312", "xray emission", "soft protons", "global budget", "dense structure", "galaxy icm interactions", "hot gas", "shapley supercluster core", "galaxy interactions", "cluster interactions"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Herve Bourdin, 2011, 'Cluster and galaxy interactions in dense environment: Shapley supercluster core', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pqex4bp