A dataset provided by the European Space Agency

Name: A FIRST COMPARISON OF X-RAY AND OPTICAL INTRACLUSTER LIGHT
Published: 2005-11-11T00:00:00Z

Proposal ID	020302
Title	A FIRST COMPARISON OF X-RAY AND OPTICAL INTRACLUSTER LIGHT
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203020101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203020201
DOI	https://doi.org/10.5270/esa-3v5li5f
Principal Investigator, PI	Prof ANN ZABLUDOFF
Abstract	We propose to make the first comparison of intracluster light in the X-ray andoptical bands for four clusters of galaxies. We have developed a new approachthat constrains the stellar light profile out to at least 0.5 Mpc. Thesensitivity, wide field, and spectral capabilities of XMM-Newton will allow usto derive the total mass and gas mass profiles out to a similar radius and toanswer 1 whether the observed variations in the stellar light profiles ofsimilar clusters reflect differences in the mass profiles or in the evolution ofthe stellar intracluster medium? and 2 what are the relative contributions ofgas and stars to the overall baryon fraction?
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 HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity gas mass cluster radius and velocity dispersion \|Zhang Y.-Y. Andernach H. et al. \| A&A \| 526-105 \| 2011 \| 2011A&A...526A.105Z \| http://ui.adsabs.harvard.edu/#abs/2011A&A...526A.105Z 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 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 Swift Burst Alert Telescope Perspective on Non-thermal Emission in HIFLUGCS Galaxy Clusters \|Wik Daniel R. Sarazin Craig L. et al. \| ApJ \| 748-67 \| 2012 \| 2012ApJ...748...67W \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...748...67W 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 Constraining supernova models using the hot gas in clusters of galaxies \|de Plaa J. Werner N. et al. \| A&A \| 465-345 \| 2007 \| 2007A&A...465..345D \| http://ui.adsabs.harvard.edu/#abs/2007A&A...465..345D The Enrichment of the Intracluster Medium \|Sivanandam Suresh Zabludoff Ann I. et al. \| ApJ \| 691-1787 \| 2009 \| 2009ApJ...691.1787S \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...691.1787S 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 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 A search for thermally emitting isolated neutron stars in the 2XMMp catalogue \|Pires A. M. Motch C. \| A&A \| 504-185 \| 2009 \| 2009A&A...504..185P \| http://ui.adsabs.harvard.edu/#abs/2009A&A...504..185P 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 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 Characterization of Intracluster Medium Temperature Distributions of 62 Galaxy Clusters with XMM-Newton \|Frank K. A. Peterson J. R. et al. \| ApJ \| 764-46 \| 2013 \| 2013ApJ...764...46F \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...764...46F 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 Galaxy Cluster Baryon Fractions Revisited \|Gonzalez Anthony H. Sivanandam Suresh et al. \| ApJ \| 778-14 \| 2013 \| 2013ApJ...778...14G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...778...14G A Good Mass Proxy for Galaxy Clusters with XMM-Newton \|Zhao Hai-Hui Jia Shu-Mei et al. \| ApJ \| 778-124 \| 2013 \| 2013ApJ...778..124Z \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...778..124Z 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 XMM-Newton and Chandra cross-calibration using HIFLUGCS galaxy clusters . Systematic temperature differences and cosmological impact \|Schellenberger G. Reiprich T. H. et al. \| A&A \| 575-30 \| 2015 \| 2015A&A...575A..30S \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..30S 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 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 HIFLUGCS: X-ray luminosity-dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys \|Zhang Yu-Ying Reiprich Thomas H. et al. \| A&A \| 599-138 \| 2017 \| 2017A&A...599A.138Z \| http://ui.adsabs.harvard.edu/#abs/2017A&A...599A.138Z HICOSMO - cosmology with a complete sample of galaxy clusters - I. Data analysis sample selection and luminosity-mass scaling relation \|Schellenberger G. Reiprich T. H. \| MNRAS \| 469-3738 \| 2017 \| 2017MNRAS.469.3738S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.3738S 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 HICOSMO: cosmology with a complete sample of galaxy clusters - II. Cosmological results \|Schellenberger G. Reiprich T. H. \| MNRAS \| 471-1370 \| 2017 \| 2017MNRAS.471.1370S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1370S Recovering galaxy cluster gas density profiles with XMM-Newton and Chandra \|Bartalucci I. Arnaud M. et al. \| A&A \| 608-88 \| 2017 \| 2017A&A...608A..88B \| http://ui.adsabs.harvard.edu/#abs/2017A&A...608A..88B Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V 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 Enrichment of the Hot Intracluster Medium: Observations \|Mernier F. Biffi V. et al. \| SSRv \| 214-129 \| 2018 \| 2018SSRv..214..129M \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214..129M 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 The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population \|Pratt G. W. Arnaud M. et al. \| SSRv \| 215-25 \| 2019 \| 2019SSRv..215...25P \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215...25P 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 Binary Clusters Observed with XMM-Newton X-Ray Observatory \|Beygu B. Hudaverdi M. \| POBeo \| 86-117 \| 2009 \| 2009POBeo..86..117B \| http://ui.adsabs.harvard.edu/#abs/2009POBeo..86..117B 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 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. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H 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 The Y SZ Planck - Y SZ XMM scaling relation and its difference between cool-core and non-cool-core clusters \|Zhu Yue Wang Yuan-Hao et al. \| RAA \| 19-104 \| 2019 \| 2019RAA....19..104Z \| http://ui.adsabs.harvard.edu/#abs/2019RAA....19..104Z Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. 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 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 Mass-Velocity Dispersion Relation in HIFLUGCS Galaxy Clusters \|Tian Yong Yu Po-Chieh et al. \| ApJ \| 910-56 \| 2021 \| 2021ApJ...910...56T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910...56T 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 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 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 A systematic comparison of galaxy cluster temperatures measured with NuSTAR and Chandra \|Wallbank A. N. Maughan B. J. et al. \| MNRAS \| 517-5594 \| 2022 \| 2022MNRAS.517.5594W \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.5594W 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 Studying X-ray instruments with galaxy clusters \|Nevalainen J. Molendi S. \| A&A \| 676-142 \| 2023 \| 2023A&A...676A.142N \| http://ui.adsabs.harvard.edu/#abs/2023A&A...676A.142N 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 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	2004-07-01T14:28:14Z/2004-10-06T14:17:41Z
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	2005-11-11T00:00:00Z
Last Update	2025-01-27
Keywords	"overall baryon fraction", "gas mass profiles", "mass profiles", "optical intracluster light", "optical bands", "stellar light profiles", "xmm newton", "wide field", "XMM-Newton", "relative contributions", "stellar intracluster medium", "XMM", "intracluster light", "cluster reflect", "total mass", "stellar light profile"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof ANN ZABLUDOFF, 2005, 'A FIRST COMPARISON OF X-RAY AND OPTICAL INTRACLUSTER LIGHT', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-3v5li5f