A dataset provided by the European Space Agency

Name: XMM observation of AS1063 comma one of the most luminous clusters known
Published: 2009-06-07T00:00:00Z

Proposal ID	050463
Title	XMM observation of AS1063, one of the most luminous clusters known
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504630101
DOI	https://doi.org/10.5270/esa-rget3te
Principal Investigator, PI	Mr Karl Andersson
Abstract	We propose a 45 ksec observation of Abell S1063 (z=0.3475), the second mostX-ray luminous cluster in the ROSAT-ESO Flux Limited X-ray (REFLEX) galaxycluster survey and maybe one of the most massive clusters known. Chandra dataimply strong centroid variation with the core being clearly offset. The veryhigh luminosity L_44=30 and high temperaure T=11 keV imply that this cluster isboosted by merger effects. If this is true for AS1063 we should see a starktemperature structure perhaps similar to that of the bullet. clusterRXJ0658-55. It is necessary to produce highly resolved temperature maps tocategorize these clusters and to understand their formation and this is notpossible with the existing Chandra data.
Publications	Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 536-11 \| 2011 \| 2011A&A...536A..11P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..11P Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 550-131 \| 2013 \| 2013A&A...550A.131P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A.131P An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission \|Henley, David B., Shelton, Robin L., \| ApJ \| 773-92 \| 2013 \| 2013ApJ...773...92H \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...773...92H 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 Scaling Relations and X-Ray Properties of Moderate-luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton \|Connor, Thomas, Donahue, Megan, et al. \| ApJ \| 794-48 \| 2014 \| 2014ApJ...794...48C \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...794...48C 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 The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models. X-Ray Emission \|Henley, David B., Shelton, Robin L., et al. \| ApJ \| 800-102 \| 2015 \| 2015ApJ...800..102H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...800..102H 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 Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters \|Kozmanyan, Arpine, Bourdin, Herve, et al. \| A&A \| 621-34 \| 2019 \| 2019A&A...621A..34K \| http://ui.adsabs.harvard.edu/#abs/2019A&A...621A..34K 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 The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state \|Bartalucci, I., Arnaud, M., et al. \| A&A \| 628-86 \| 2019 \| 2019A&A...628A..86B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..86B Mass variance from archival X-ray properties of Dark Energy Survey Year-1 galaxy clusters \|Farahi, A., Chen, X., et al. \| MNRAS \| 490-3341 \| 2019 \| 2019MNRAS.490.3341F \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.490.3341F 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 X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M The BUFFALO HST Survey \|Steinhardt, Charles L., Jauzac, Mathilde, et al. \| ApJS \| 247-64 \| 2020 \| 2020ApJS..247...64S \| http://ui.adsabs.harvard.edu/#abs/2020ApJS..247...64S 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 The discovery of radio halos in the frontier fields clusters Abell S1063 and Abell 370 \|Xie, C., van Weeren, R. J., et al. \| A&A \| 636-3 \| 2020 \| 2020A&A...636A...3X \| http://ui.adsabs.harvard.edu/#abs/2020A&A...636A...3X Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C 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 Constraining the Milky Way Mass with Its Hot Gaseous Halo \|Guo, Fulai, Zhang, Ruiyu, \| ApJ \| 904-14 \| 2020 \| 2020ApJ...904L..14G \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904L..14G An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q Diffuse galaxy cluster emission at 168 MHz within the Murchison Widefield Array Epoch of Reionization 0-h field \|Duchesne, S. W., Johnston-Hollitt, M., et al. \| PASA \| 38-10 \| 2021 \| 2021PASA...38...10D \| http://ui.adsabs.harvard.edu/#abs/2021PASA...38...10D 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 The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview \|CHEX-MATE Collaboration, Arnaud, M., et al. \| A&A \| 650-104 \| 2021 \| 2021A&A...650A.104C \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.104C PACT. II. Pressure profiles of galaxy clusters using Planck and ACT \|Pointecouteau, E., Santiago-Bautista, I., et al. \| A&A \| 651-73 \| 2021 \| 2021A&A...651A..73P \| http://ui.adsabs.harvard.edu/#abs/2021A&A...651A..73P The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q CHEX-MATE: Morphological analysis of the sample \|Campitiello, M. G., Ettori, S., et al. \| A&A \| 665-117 \| 2022 \| 2022A&A...665A.117C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A.117C Linking a universal gas density profile to the core-excised X-ray luminosity in galaxy clusters up to z \\u223c 1.1 \|Pratt, G. W., Arnaud, M., et al. \| A&A \| 665-24 \| 2022 \| 2022A&A...665A..24P \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A..24P Heating of the intracluster medium by buoyant bubbles and sound waves \|Iqbal, Asif, Majumdar, Subhabrata, et al. \| MNRAS \| 518-2735 \| 2023 \| 2023MNRAS.518.2735I \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.518.2735I 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 CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles \|Bartalucci, I., Molendi, S., et al. \| A&A \| 674-179 \| 2023 \| 2023A&A...674A.179B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A.179B CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters \|Bourdin, H., De Luca, F., et al. \| A&A \| 678-181 \| 2023 \| 2023A&A...678A.181B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.181B CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles \|Iqbal, A., Pratt, G. W., et al. \| A&A \| 679-51 \| 2023 \| 2023A&A...679A..51I \| http://ui.adsabs.harvard.edu/#abs/2023A&A...679A..51I Pressure profiles of distant Galaxy clusters with Planck-SPT data \|Oppizzi, Filippo, De Luca, Federico, et al. \| EPJWC \| 257-00035 \| 2022 \| 2022EPJWC.25700035O \| http://ui.adsabs.harvard.edu/#abs/2022EPJWC.25700035O CHEX-MATE: Characterization of the intra-cluster medium temperature distribution \|Lovisari, L., Ettori, S., et al. \| A&A \| 682-A45 \| 2024 \| 2024A&A...682A..45L \| http://ui.adsabs.harvard.edu/#abs/2024A&A...682A..45L 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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 CHEX-MATE: Robust reconstruction of temperature profiles in galaxy clusters with XMM-Newton \|Rossetti, M., Eckert, D., et al. \| A&A \| 686-A68 \| 2024 \| 2024A&A...686A..68R \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A..68R 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	2008-04-30T11:14:46Z/2008-05-01T01:53:40Z
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	2009-06-07T00:00:00Z
Keywords	"xray luminous cluster", "massive cluster", "abell s1063 z", "XMM", "cluster rxj0658", "stark temperature structure", "chandra data", "luminosity l_44", "centroid variation", "resolved temperature maps", "existing chandra data", "merger effects", "Abell ", "ROSAT", "luminous cluster"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Karl Andersson, 2009, 'XMM observation of AS1063 comma one of the most luminous clusters known', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rget3te