A dataset provided by the European Space Agency

Name: High-resolution X-ray spectroscopy of the cluster of galaxies 2A 0335+096
Published: 2002-08-07T00:00:00Z

Proposal ID	010987
Title	High-resolution X-ray spectroscopy of the cluster of galaxies 2A 0335+096
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109870101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109870201
DOI	https://doi.org/10.5270/esa-82prywh
Principal Investigator, PI	Dr Albert Brinkman
Abstract	We propose to observe the cluster of galaxies 2A 0335+096 in order to performspatially resolved spectroscopy with the RGS. 2A 0335+096 is an ideal target forthis since it has a FWHM of only 1.4 arcmin, allowing a high spectralresolution with the RGS and also an almost complete coverage of the cooling flowregion of the cluster within the cross-dispersion width of the detector. Inparticular we will study the temperature and abundance distribution within thecentral region using the RGS. The EPIC observations will supplement this forthe outer regions of the cluster, where we will study the abundance andtemperature gradients as well as investigate the existence of non-thermalcomponents.
Publications	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 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 XMM-Newton confirmation of soft X-ray excess emission in clusters of galaxies - The discovery of O VII emission from an extended warm baryonic component \|Kaastra, J. S., Lieu, R., et al. \| A&A \| 397-445 \| 2003 \| 2003A&A...397..445K \| http://ui.adsabs.harvard.edu/#abs/2003A&A...397..445K Spatially resolved X-ray spectroscopy of cooling clusters of galaxies \|Kaastra, J. S., Tamura, T., et al. \| A&A \| 413-415 \| 2004 \| 2004A&A...413..415K \| http://ui.adsabs.harvard.edu/#abs/2004A&A...413..415K Elemental abundances in the intracluster medium as observed with XMM-Newton \|Tamura, T., Kaastra, J. S., et al. \| A&A \| 420-135 \| 2004 \| 2004A&A...420..135T \| http://ui.adsabs.harvard.edu/#abs/2004A&A...420..135T Temperature and entropy profiles of nearby cooling flow clusters observed with XMM-Newton \|Piffaretti, R., Jetzer, Ph., et al. \| A&A \| 433-101 \| 2005 \| 2005A&A...433..101P \| http://ui.adsabs.harvard.edu/#abs/2005A&A...433..101P Effervescent heating: constraints from nearby cooling flow clusters observed with XMM-Newton \|Piffaretti, R., Kaastra, J. S., \| A&A \| 453-423 \| 2006 \| 2006A&A...453..423P \| http://ui.adsabs.harvard.edu/#abs/2006A&A...453..423P 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 High-Resolution X-Ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies \|Peterson, J. R., Kahn, S. M., et al. \| ApJ \| 590-207 \| 2003 \| 2003ApJ...590..207P \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...590..207P 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 XMM-Newton study of soft excess X-ray emission in clusters of galaxies \|Kaastra, J. S., Lieu, R., et al. \| AdSpR \| 34-2504 \| 2004 \| 2004AdSpR..34.2504K \| http://ui.adsabs.harvard.edu/#abs/2004AdSpR..34.2504K 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 Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog \|Georgakakis, A. E., Chavushyan, V., et al. \| MNRAS \| 367-1017 \| 2006 \| 2006MNRAS.367.1017G \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G Thermo-dynamic and chemical properties of the intra-cluster medium \|Leccardi, A., Rossetti, M., \| A&A \| 510-82 \| 2010 \| 2010A&A...510A..82L \| http://ui.adsabs.harvard.edu/#abs/2010A&A...510A..82L 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 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 XMM-Newton serendipitous source catalogue \|Watson, M. G., Pye, J. P., et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W 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 Chemical Enrichment RGS cluster Sample (CHEERS): Constraints on turbulence \|Pinto, Ciro, Sanders, Jeremy S., et al. \| A&A \| 575-38 \| 2015 \| 2015A&A...575A..38P \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..38P Sunyaev-Zel.dovich 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 Origin of central abundances in the hot intra-cluster medium. I. Individual and average abundance ratios from XMM-Newton EPIC \|Mernier, F., de Plaa, J., et al. \| A&A \| 592-157 \| 2016 \| 2016A&A...592A.157M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...592A.157M 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 Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models \|Mernier, F., de Plaa, J., et al. \| A&A \| 595-126 \| 2016 \| 2016A&A...595A.126M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A.126M Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>virgul1 and their Galaxy Populations \|Fassbender, Rene, \| PhDT \| 0-116 \| 2008 \| 2008PhDT.......116F \| http://ui.adsabs.harvard.edu/#abs/2008PhDT.......116F CHEERS: The chemical evolution RGS sample \|de Plaa, J., Kaastra, J. S., et al. \| A&A \| 607-98 \| 2017 \| 2017A&A...607A..98D \| http://ui.adsabs.harvard.edu/#abs/2017A&A...607A..98D Solar abundance ratios of the iron-peak elements in the Perseus cluster \|Hitomi Collaboration, Aharonian, Felix, et al. \| Natur \| 551-478 \| 2017 \| 2017Natur.551..478H \| http://ui.adsabs.harvard.edu/#abs/2017Natur.551..478H Charge exchange in galaxy clusters \|Gu, Liyi, Mao, Junjie, et al. \| A&A \| 611-26 \| 2018 \| 2018A&A...611A..26G \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..26G 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 Mass-invariance of the iron enrichment in the hot haloes of massive ellipticals, groups, and clusters of galaxies \|Mernier, F., de Plaa, J., et al. \| MNRAS \| 478-116 \| 2018 \| 2018MNRAS.478L.116M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478L.116M 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 Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies \|Mernier, F., Werner, N., et al. \| MNRAS \| 480-95 \| 2018 \| 2018MNRAS.480L..95M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480L..95M 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 Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within 104 yr \|Ichikawa, Kohei, Ueda, Junko, et al. \| ApJ \| 870-65 \| 2019 \| 2019ApJ...870...65I \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...65I Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups \|Liu, Haonan, Pinto, Ciro, et al. \| MNRAS \| 485-1757 \| 2019 \| 2019MNRAS.485.1757L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.1757L 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 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 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 The inner gas mass-temperature profile in the core of nearby galaxy clusters \|Liu, Haonan, Fabian, Andrew C., \| MNRAS \| 497-1256 \| 2020 \| 2020MNRAS.497.1256L \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.1256L 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 The Metal Content of the Hot Atmospheres of Galaxy Groups \|Gastaldello, Fabio, Simionescu, Aurora, et al. \| Univ \| 7-208 \| 2021 \| 2021Univ....7..208G \| http://ui.adsabs.harvard.edu/#abs/2021Univ....7..208G 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 High-resolution X-ray spectroscopy of astrophysical plasmas with X-ray microcalorimeters \|Ezoe, Yuichiro, Ohashi, Takaya, \| RvMPP \| 5-4 \| 2021 \| 2021RvMPP...5....4E \| http://ui.adsabs.harvard.edu/#abs/2021RvMPP...5....4E Hidden cooling flows in clusters of galaxies - III. Accretion on to the central black hole \|Fabian, A. C., Sanders, J. S., et al. \| MNRAS \| 524-716 \| 2023 \| 2023MNRAS.524..716F \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524..716F 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	2001-02-09T11:15:37Z/2001-02-09T22:48:49Z
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	2002-08-07T00:00:00Z
Keywords	"cooling flow region", "resolution xray spectroscopy", "temperature gradients", "nonthermal components", "abundance distribution", "2a 0335", "complete coverage", "central region", "cross dispersion width", "EPIC", "spectral resolution", "resolved spectroscopy", "outer region", "ideal target", "galaxy 2a 0335"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Albert Brinkman, 2002, 'High-resolution X-ray spectroscopy of the cluster of galaxies 2A 0335+096', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-82prywh