A dataset provided by the European Space Agency

Name: XMM-Newton Observations of the Merging Cluster Abell S0592
Published: 2011-06-15T00:00:00Z

Proposal ID	065086
Title	XMM-Newton Observations of the Merging Cluster Abell S0592
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0650860101
DOI	https://doi.org/10.5270/esa-4n6vsqv
Principal Investigator, PI	Prof John P. Hughes
Abstract	We propose to obtain sensitive XMM-Newton observations of the X-ray brightcluster Abell S0592 (RXC J0638.7-5358), which we have selected based on itsrecent detection by ACT in the Sunyaev-Zel.dovich effect (SZE) at 145 GHz.Archival Chandra and HST/ACS data reveal that Abell S0592 is undergoing a majormerger. There is a significant offset between the peak of the gas distributionand the location of one of the two bright central dominant galaxies. Thetemperature determined from the Chandra data varies significantly with position.Further detailed study of the X-ray spectrum and morphology of this interactingcluster (along with weak lensing and SZE data) will shed light on thedistribution of its baryons and dark matter.
Publications	Detection of an Unidentified Emission Line in the Stacked X-Ray Spectrum of Galaxy Clusters \|Bulbul, Esra, Markevitch, Maxim, et al. \| ApJ \| 789-13 \| 2014 \| 2014ApJ...789...13B \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...789...13B 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 Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus \|Carlson, Eric, Jeltema, Tesla, \| JCAP \| 2-9 \| 2015 \| 2015JCAP...02..009C \| http://ui.adsabs.harvard.edu/#abs/2015JCAP...02..009C A novel scenario for the possible X-ray line feature at virgul3.5 keV. Charge exchange with bare sulfur ions \|Gu, L., Kaastra, J., et al. \| A&A \| 584-11 \| 2015 \| 2015A&A...584L..11G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...584L..11G 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 X-Ray Morphological Analysis of the Planck ESZ Clusters \|Lovisari, Lorenzo, Forman, William R., et al. \| ApJ \| 846-51 \| 2017 \| 2017ApJ...846...51L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...846...51L X-Ray Lines from Dark Matter Annihilation at the keV Scale \|Brdar, Vedran, Kopp, Joachim, et al. \| PhRvL \| 120-61301 \| 2018 \| 2018PhRvL.120f1301B \| http://ui.adsabs.harvard.edu/#abs/2018PhRvL.120f1301B WIMP dark matter candidates and searches---current status and future prospects \|Roszkowski, Leszek, Sessolo, Enrico Maria, \| RPPh \| 81-66201 \| 2018 \| 2018RPPh...81f6201R \| http://ui.adsabs.harvard.edu/#abs/2018RPPh...81f6201R Resonantly Produced 7A keV Sterile Neutrino Dark Matter Models and the Properties of Milky Way Satellites \|Abazajian, Kevork N., \| PhRvL \| 112-161303 \| 2014 \| 2014PhRvL.112p1303A \| http://ui.adsabs.harvard.edu/#abs/2014PhRvL.112p1303A Laboratory Measurements of X-Ray Emission from Highly Charged Argon Ions \|Bulbul, Esra, Foster, Adam, et al. \| ApJ \| 870-21 \| 2019 \| 2019ApJ...870...21B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...21B X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton \|Bulbul, Esra, Chiu, I.-Non, et al. \| ApJ \| 871-50 \| 2019 \| 2019ApJ...871...50B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...871...50B X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton \|Lovisari, Lorenzo, Schellenberger, Gerrit, et al. \| ApJ \| 892-102 \| 2020 \| 2020ApJ...892..102L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy - II. The X-ray luminosity-mass relation \|Capasso, R., Mohr, J. J., et al. \| MNRAS \| 494-2736 \| 2020 \| 2020MNRAS.494.2736C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.2736C Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z \\u223c 1 \|Gupta, N., Pannella, M., et al. \| MNRAS \| 494-1705 \| 2020 \| 2020MNRAS.494.1705G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.1705G Comparing different mass estimators for a large subsample of the Planck-ESZ clusters \|Lovisari, L., Ettori, S., et al. \| A&A \| 644-78 \| 2020 \| 2020A&A...644A..78L \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L Constraints on the variation of fine structure constant from joint SPT-SZ and XMM-Newton observations \|Bora, Kamal, Desai, Shantanu, \| JCAP \| 2-12 \| 2021 \| 2021JCAP...02..012B \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...02..012B Metastable conformal dark matter \|Brax, Philippe, Kaneta, Kunio, et al. \| PhRvD \| 103-115016 \| 2021 \| 2021PhRvD.103k5016B \| http://ui.adsabs.harvard.edu/#abs/2021PhRvD.103k5016B A Search for the 3.5 keV Line from the Milky Way.s Dark Matter Halo with HaloSat \|Silich, E. M., Jahoda, K., et al. \| ApJ \| 916-2 \| 2021 \| 2021ApJ...916....2S \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...916....2S A test of cosmic distance duality relation using SPT-SZ galaxy clusters, Type Ia supernovae, and cosmic chronometers \|Bora, Kamal, Desai, Shantanu, \| JCAP \| 6-52 \| 2021 \| 2021JCAP...06..052B \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...06..052B The thermalization of massive galaxy clusters \|Sereno, Mauro, Lovisari, Lorenzo, et al. \| MNRAS \| 507-5214 \| 2021 \| 2021MNRAS.507.5214S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5214S 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 Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters \|Wicker, R., Douspis, M., et al. \| A&A \| 674-48 \| 2023 \| 2023A&A...674A..48W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W Was There a 3.5 keV Line? \|Dessert, Christopher, Foster, Joshua W., et al. \| ApJ \| 964-185 \| 2024 \| 2024ApJ...964..185D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...964..185D 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	2010-05-22T07:33:02Z/2010-05-22T21:05:00Z
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	2011-06-15T00:00:00Z
Keywords	"J0638.7", "XMM-Newton", "xmm newton", "sze data", "archival chandra", "dark matter", "sensitive xmm newton", "major merger", "chandra data varies", "XMM", "xray spectrum", "shed light", "acs data", "145 ghz", "Abell ", "abell s0592", "interacting cluster", "weak lensing", "dovich effect sze", "sunyaev zel", "HST", "gas distribution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof John P. Hughes, 2011, 'XMM-Newton Observations of the Merging Cluster Abell S0592', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-4n6vsqv