A dataset provided by the European Space Agency

Name: High-resolution X-ray spectroscopy of the cluster of galaxies A 478
Published: 2003-03-07T00:00:00Z

Proposal ID	010988
Title	High-resolution X-ray spectroscopy of the cluster of galaxies A 478
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109880101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109880301
DOI	https://doi.org/10.5270/esa-wk6pqwp
Principal Investigator, PI	Dr Albert Brinkman
Abstract	We propose to observe the cluster of galaxies A 478 in order to perform spatial-ly resolved spectroscopy with the RGS. A 478 is an ideal target for this sinceit has a FWHM of only 1.6 arcmin, allowing a high spectral resolution with theRGS and an almost complete coverage of the cooling flow region. In particular wewill study the temperature and abundance distribution within the central regionusing the RGS. A478 has a very strong cooling flow and shows a considerableradially decreasing absorbing column density. The EPIC observations willsupplement this for the outer regions of the cluster, where we will study theabundance and temperature gradients as well as investigate the existence ofnon-thermal components.
Publications	XMM-Newton observation of the relaxed cluster A478: Gas and dark matter distribution from 0.01R200 to 0.5R200 \|Pointecouteau E. Arnaud M. et al. \| A&A \| 423-33 \| 2004 \| 2004A&A...423...33P \| http://ui.adsabs.harvard.edu/#abs/2004A&A...423...33P X-ray spectroscopy on Abell 478 with XMM-Newton \|de Plaa J. Kaastra J. S. et al. \| A&A \| 423-49 \| 2004 \| 2004A&A...423...49D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...423...49D 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 The structural and scaling properties of nearby galaxy clusters. II. The M-T relation \|Arnaud M. Pointecouteau E. \| A&A \| 441-893 \| 2005 \| 2005A&A...441..893A \| http://ui.adsabs.harvard.edu/#abs/2005A&A...441..893A The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project \|Fassbender R. Bohringer H. et al. \| NJPh \| 13-125014 \| 2011 \| 2011NJPh...13l5014F \| http://ui.adsabs.harvard.edu/#abs/2011NJPh...13l5014F 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 Cool core remnants in galaxy clusters \|Rossetti M. Molendi S. \| A&A \| 510-83 \| 2010 \| 2010A&A...510A..83R \| http://ui.adsabs.harvard.edu/#abs/2010A&A...510A..83R 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 The structural and scaling properties of nearby galaxy clusters. I. The universal mass profile \|Pointecouteau E. Arnaud M. \| A&A \| 435-1 \| 2005 \| 2005A&A...435....1P \| http://ui.adsabs.harvard.edu/#abs/2005A&A...435....1P Structure and scaling of the entropy in nearby galaxy clusters \|Pratt G. W. Arnaud M. \| A&A \| 446-429 \| 2006 \| 2006A&A...446..429P \| http://ui.adsabs.harvard.edu/#abs/2006A&A...446..429P An improved deprojection and PSF-deconvolution technique for galaxy-cluster X-ray surface-brightness profiles \|Croston J. H. Arnaud M. et al. \| A&A \| 459-1007 \| 2006 \| 2006A&A...459.1007C \| http://ui.adsabs.harvard.edu/#abs/2006A&A...459.1007C Calibration of the galaxy cluster M{500}-Y{X} relation with XMM-Newton \|Arnaud M. Pointecouteau E. \| A&A \| 474-37 \| 2007 \| 2007A&A...474L..37A \| http://ui.adsabs.harvard.edu/#abs/2007A&A...474L..37A 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 Possible AGN Shock Heating in the Cool-Core Galaxy Cluster Abell 478 \|Sanderson Alastair J. R. Finoguenov Alexis \| ApJ \| 630-191 \| 2005 \| 2005ApJ...630..191S \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...630..191S Oxygen Abundances in the Milky Way Using X-Ray Absorption Measurements toward Galaxy Clusters \|Baumgartner W. H. Mushotzky R. F. \| ApJ \| 639-929 \| 2006 \| 2006ApJ...639..929B \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...639..929B The X-Ray Concentration-Virial Mass Relation \|Buote David A. Gastaldello Fabio et al. \| ApJ \| 664-123 \| 2007 \| 2007ApJ...664..123B \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...664..123B Joint Analysis of Cluster Observations. I. Mass Profile of Abell 478 from Combined X-Ray Sunyaev-Zeldovich and Weak-Lensing Data \|Mahdavi Andisheh Hoekstra Henk et al. \| ApJ \| 664-162 \| 2007 \| 2007ApJ...664..162M \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...664..162M 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 Probing the dark matter profile of hot clusters and the M- T relation with XMM- Newton \|Pointecouteau E. Arnaud M. \| AdSpR \| 36-659 \| 2005 \| 2005AdSpR..36..659P \| http://ui.adsabs.harvard.edu/#abs/2005AdSpR..36..659P 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 Collisional interaction limits between dark matter particles and baryons in cooling flow clusters \|Hu Jian Lou Yu-Qing \| MNRAS \| 384-814 \| 2008 \| 2008MNRAS.384..814H \| http://ui.adsabs.harvard.edu/#abs/2008MNRAS.384..814H New constraints on modified Newtonian dynamics from galaxy clusters \|Pointecouteau Etienne Silk Joseph \| MNRAS \| 364-654 \| 2005 \| 2005MNRAS.364..654P \| http://ui.adsabs.harvard.edu/#abs/2005MNRAS.364..654P On the Origin of the Extended Halpha Filaments in Cooling Flow Clusters \|McDonald Michael Veilleux Sylvain et al. \| ApJ \| 721-1262 \| 2010 \| 2010ApJ...721.1262M \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...721.1262M 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 The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca A. Molendi S. \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D 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. 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Farrell Sean et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L 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 The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 Galaxy cluster masses without non-baryonic dark matter \|Brownstein J. R. Moffat J. W. \| MNRAS \| 367-527 \| 2006 \| 2006MNRAS.367..527B \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367..527B Chandra Temperature Profiles for a Sample of Nearby Relaxed Galaxy Clusters \|Vikhlinin A. Markevitch M. et al. \| ApJ \| 628-655 \| 2005 \| 2005ApJ...628..655V \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...628..655V 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 Where do the 3.5 keV photons come from? 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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 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 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 Ways Dark Matter Halo with HaloSat \|Silich E. M. 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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 Atmospheric Pressure and Molecular Cloud Formation in Early-type Galaxies \|Babyk Iu. V. McNamara B. R. et al. \| ApJ \| 944-69 \| 2023 \| 2023ApJ...944...69B \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...944...69B 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 Hydrostatic Mass of A478: Discrepant Results from Chandra NuSTAR and XMM-Newton \|Potter Cicely Tu00fcmer Ayu015fegu00fcl et al. \| ApJ \| 958-112 \| 2023 \| 2023ApJ...958..112P \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...958..112P Outskirts of Abell 1795: Probing gas clumping in the intracluster medium \|Kovu00e1cs Orsolya Eszter Zhu Zhenlin et al. \| A&A \| 678-91 \| 2023 \| 2023A&A...678A..91K \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A..91K 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	2002-02-15T14:52:08Z/2002-02-17T02:58:40Z
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	2003-03-07T00:00:00Z
Last Update	2025-01-27
Keywords	"resolution xray spectroscopy", "EPIC", "cooling flow region", "cooling flow", "nonthermal components", "spectral resolution", "complete coverage", "absorbing column density", "outer region", "temperature gradients", "central region", "ideal target", "abundance distribution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Albert Brinkman, 2003, 'High-resolution X-ray spectroscopy of the cluster of galaxies A 478', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wk6pqwp