A dataset provided by the European Space Agency

Name: OBSERVING THE SHOCK WAVE IN COMPACT GALAXY CLUSTERS A2065 AND A4038
Published: 2006-02-04T00:00:00Z

Proposal ID	020208
Title	OBSERVING THE SHOCK WAVE IN COMPACT GALAXY CLUSTERS A2065 AND A4038
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0202080201
DOI	https://doi.org/10.5270/esa-m82eg3w
Principal Investigator, PI	Dr JEAN-LUC SAUVAGEOT
Abstract	Numerical simulations predict the formation and development of a shock wave inthe intracluster medium at some stage of a merging cluster event. Despiteextensive efforts however, this strong feature still lack to be observed. Thisis a conspiration between the particular physics involved in exactly this stageof the merging process and the sensitivity of X-ray instrument. After applyingcareful selection criteria based on the X-ray morphology, temperature and galaxydistribution, we propose to observe the two best candidates aimed to measure forthe first time the physical conditions at the shock wave with XMM-Newton.
Publications	Metal abundances in the cool cores of galaxy clusters \|de Grandi S. Molendi S. \| A&A \| 508-565 \| 2009 \| 2009A&A...508..565D \| http://ui.adsabs.harvard.edu/#abs/2009A&A...508..565D The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy \|Levan A. J. Tanvir N. R. et al. \| Sci \| 333-199 \| 2011 \| 2011Sci...333..199L \| http://ui.adsabs.harvard.edu/#abs/2011Sci...333..199L Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M 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 The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The Axis Ratio Distribution of X-ray Clusters Observed by XMM-Newton \|Kawahara Hajime \| ApJ \| 719-1926 \| 2010 \| 2010ApJ...719.1926K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...719.1926K A catalog of galaxy clusters observed by XMM-Newton \|Snowden S. L. Mushotzky R. F. et al. \| A&A \| 478-615 \| 2008 \| 2008A&A...478..615S \| http://ui.adsabs.harvard.edu/#abs/2008A&A...478..615S Temperature structure of the intergalactic medium within seven nearby and bright clusters of galaxies observed with XMM-Newton \|Bourdin H. Mazzotta P. \| A&A \| 479-307 \| 2008 \| 2008A&A...479..307B \| http://ui.adsabs.harvard.edu/#abs/2008A&A...479..307B Characterizing the Properties of Clusters of Galaxies as a Function of Luminosity and Redshift \|Andersson K. Peterson J. R. et al. \| ApJ \| 696-1029 \| 2009 \| 2009ApJ...696.1029A \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...696.1029A Cold fronts in galaxy clusters \|Ghizzardi S. Rossetti M. \| A&A \| 516-32 \| 2010 \| 2010A&A...516A..32G \| http://ui.adsabs.harvard.edu/#abs/2010A&A...516A..32G A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 \|Georgakakis Antonis Nandra K. \| MNRAS \| 414-992 \| 2011 \| 2011MNRAS.414..992G \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.414..992G An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Luminous X-ray Active Galactic Nuclei in Clusters of Galaxies \|Koulouridis E. Plionis M. \| ApJ \| 714-181 \| 2010 \| 2010ApJ...714L.181K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...714L.181K Detection of X-ray galaxy clusters based on the Kolmogorov method \|Gurzadyan V. G. Durret F. et al. \| EL \| 95-69001 \| 2011 \| 2011EL.....9569001G \| http://ui.adsabs.harvard.edu/#abs/2011EL.....9569001G The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L 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 Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page M. J. Brindle C. et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P The cool-core bias in X-ray galaxy cluster samples. I. Method and application to HIFLUGCS \|Eckert D. Molendi S. \| A&A \| 526-79 \| 2011 \| 2011A&A...526A..79E \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A..79E Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues \|Vagnetti F. Turriziani S. \| A&A \| 536-84 \| 2011 \| 2011A&A...536A..84V \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..84V Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau F.-X. Motch C. et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi J. A. Albacete Colombo J. F. et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 \|Ballo L. Heras F. J. H. et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B Characterization of Intracluster Medium Temperature Distributions of 62 Galaxy Clusters with XMM-Newton \|Frank K. A. Peterson J. 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N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Obscuration-dependent Evolution of Active Galactic Nuclei \|Buchner Johannes Georgakakis Antonis et al. \| ApJ \| 802-89 \| 2015 \| 2015ApJ...802...89B \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...802...89B Probing the evolution of the substructure frequency in galaxy clusters up to z ~ 1 \|Weissmann A. Bohringer H. \| A&A \| 555-147 \| 2013 \| 2013A&A...555A.147W \| http://ui.adsabs.harvard.edu/#abs/2013A&A...555A.147W Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso E. Risaliti G. \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti F. Middei R. et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc N. 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H. \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L 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 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 The Fornax3D project: Tracing the assembly history of the cluster from the kinematic and line-strength maps \|Iodice E. Sarzi M. et al. \| A&A \| 627-136 \| 2019 \| 2019A&A...627A.136I \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A.136I Projected alignment of non-sphericities of stellar gas and dark matter distributions in galaxy clusters: analysis of the Horizon-AGN simulation \|Okabe Taizo Nishimichi Takahiro et al. \| MNRAS \| 478-1141 \| 2018 \| 2018MNRAS.478.1141O \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.1141O Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. 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Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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 A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman Murray Ward Charlotte et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B On the Reliability of Photometric and Spectroscopic Tracers of Halo Relaxation \|Zhoolideh Haghighi Mohammad H. Raouf Mojtaba et al. \| ApJ \| 904-36 \| 2020 \| 2020ApJ...904...36Z \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...36Z 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. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2005-01-08T23:46:04Z/2005-01-09T09:14:34Z
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	2006-02-04T00:00:00Z
Last Update	2025-01-27
Keywords	"selection criteria", "physical conditions", "merging cluster event", "xmm newton", "xray instrument", "physics involved", "XMM-Newton", "extensive efforts", "numerical simulations predict", "merging process", "galaxy distribution", "XMM", "shock wave", "candidates aimed", "xray morphology", "intracluster medium"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr JEAN-LUC SAUVAGEOT, 2006, 'OBSERVING THE SHOCK WAVE IN COMPACT GALAXY CLUSTERS A2065 AND A4038', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-m82eg3w