A dataset provided by the European Space Agency

Name: XMM-Newton observations of the brightest relaxed cluster lenses
Published: 2004-07-19T00:00:00Z

Proposal ID	014899
Title	XMM-Newton observations of the brightest relaxed cluster lenses
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148990101
DOI	https://doi.org/10.5270/esa-yq7umuc
Principal Investigator, PI	Dr Steve Allen
Abstract	We propose XMM-Newton observations of the X-ray brightest cooling-flowclusters with bright gravitational arcs, identified from the ROSAT XBACS/BCS lensing study. All of our targets have been (or wil be) observed for us with Chandra, HST and ground-based optical observatories. Our primary aim is to extend the X-ray temperature, X-ray gas mass and total mass profiles measured with Chandra out to large radii. In combination, the X-ray and optical (strongand weak lensing) data will be used to explore the nature of the dark matter in the clusters and to constrain cosmological parameters from the variation ofthe X-ray gas mass fraction. Our targets are the X-ray brightest, dynamically relaxed lensing clusters which have not yet been observed with XMM-Newton.
Publications	Star formation efficiency in galaxy clusters \|Lagana, T. F., Lima Neto, G. B., et al. \| A&A \| 485-633 \| 2008 \| 2008A&A...485..633L \| http://ui.adsabs.harvard.edu/#abs/2008A&A...485..633L 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 x-ray luminous galaxy cluster population at 0.9 < z &lsim; 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 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 LoCuSS: A Comparison of Cluster Mass Measurements from XMM-Newton and Subaru---Testing Deviation from Hydrostatic Equilibrium and Non-thermal Pressure Support \|Zhang, Yu-Ying, Okabe, Nobuhiro, et al. \| ApJ \| 711-1033 \| 2010 \| 2010ApJ...711.1033Z \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...711.1033Z 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 LoCuSS: Calibrating Mass-observable Scaling Relations for Cluster Cosmology with Subaru Weak-lensing Observations \|Okabe, N., Zhang, Y.-Y., et al. \| ApJ \| 721-875 \| 2010 \| 2010ApJ...721..875O \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...721..875O Mass profiles and c-MDM relation in X-ray luminous galaxy clusters \|Ettori, S., Gastaldello, F., et al. \| A&A \| 524-68 \| 2010 \| 2010A&A...524A..68E \| http://ui.adsabs.harvard.edu/#abs/2010A&A...524A..68E Diffuse light and building history of the galaxy cluster Abell 2667 \|Covone, G., Adami, C., et al. \| A&A \| 460-381 \| 2006 \| 2006A&A...460..381C \| http://ui.adsabs.harvard.edu/#abs/2006A&A...460..381C Scaling relations and mass calibration of the X-ray luminous galaxy clusters at redshift virgul0.2: XMM-Newton observations \|Zhang, Y.-Y., Finoguenov, A., et al. \| A&A \| 467-437 \| 2007 \| 2007A&A...467..437Z \| http://ui.adsabs.harvard.edu/#abs/2007A&A...467..437Z 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 LoCuSS: comparison of observed X-ray and lensing galaxy cluster scaling relations with simulations \|Zhang, Y.-Y., Finoguenov, A., et al. \| A&A \| 482-451 \| 2008 \| 2008A&A...482..451Z \| http://ui.adsabs.harvard.edu/#abs/2008A&A...482..451Z Radial temperature profiles for a large sample of galaxy clusters observed with XMM-Newton \|Leccardi, A., Molendi, S., \| A&A \| 486-359 \| 2008 \| 2008A&A...486..359L \| http://ui.adsabs.harvard.edu/#abs/2008A&A...486..359L Radial metallicity profiles for a large sample of galaxy clusters observed with XMM-Newton \|Leccardi, A., Molendi, S., \| A&A \| 487-461 \| 2008 \| 2008A&A...487..461L \| http://ui.adsabs.harvard.edu/#abs/2008A&A...487..461L Constraints on turbulent velocity broadening for a sample of clusters, groups and elliptical galaxies using XMM-Newton \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 410-1797 \| 2011 \| 2011MNRAS.410.1797S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.410.1797S Revealing O VII from stacked X-ray grating spectra of clusters, groups and elliptical galaxies \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 412-35 \| 2011 \| 2011MNRAS.412L..35S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.412L..35S 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 On the influence of non-thermal pressure on the mass determination of galaxy clusters \|Lagana, T. F., de Souza, R. S., \| A&A \| 510-76 \| 2010 \| 2010A&A...510A..76L \| http://ui.adsabs.harvard.edu/#abs/2010A&A...510A..76L 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 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 Statistics and implications of substructure detected in a representative sample of X-ray clusters \|Chon, G., Bohringer, H., \| A&A \| 548-59 \| 2012 \| 2012A&A...548A..59C \| http://ui.adsabs.harvard.edu/#abs/2012A&A...548A..59C 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 Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., 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 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 Probing the evolution of the substructure frequency in galaxy clusters up to z virgul 1 \|Weissmann, A., Bohringer, H., \| A&A \| 555-147 \| 2013 \| 2013A&A...555A.147W \| http://ui.adsabs.harvard.edu/#abs/2013A&A...555A.147W Spiral-like structure at the centre of nearby clusters of galaxies \|Lagana, T. F., Andrade-Santos, F., \| A&A \| 511-15 \| 2010 \| 2010A&A...511A..15L \| http://ui.adsabs.harvard.edu/#abs/2010A&A...511A..15L 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 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 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 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S On the Connection between Turbulent Motions and Particle Acceleration in Galaxy Clusters \|Eckert, D., Gaspari, M., et al. \| ApJ \| 843-29 \| 2017 \| 2017ApJ...843L..29E \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...843L..29E 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 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 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 A New Interpretation of the Mass-Temperature Relation and Mass Calibration of Galaxy Clusters Based on the Fundamental Plane \|Fujita, Yutaka, Umetsu, Keiichi, et al. \| ApJ \| 863-37 \| 2018 \| 2018ApJ...863...37F \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863...37F 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 Formation of Galaxy Clusters \|Kravtsov, Andrey V., Borgani, Stefano, \| ARA&A \| 50-353 \| 2012 \| 2012ARA&A..50..353K \| http://ui.adsabs.harvard.edu/#abs/2012ARA&A..50..353K The Massive and Distant Clusters of WISE Survey. I. Survey Overview and a Catalog of >2000 Galaxy Clusters at z virgul= 1 \|Gonzalez, Anthony H., Gettings, Daniel P., et al. \| ApJS \| 240-33 \| 2019 \| 2019ApJS..240...33G \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..240...33G 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 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., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H 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 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 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 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 Star formation and chemical enrichment in protoclusters \|Fukushima, Keita, Nagamine, Kentaro, \| MNRAS \| 525-3760 \| 2023 \| 2023MNRAS.525.3760F \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.3760F Outskirts of Abell 1795: Probing gas clumping in the intracluster medium \|Kov\\u00e1cs, 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 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	2003-06-21T13:21:32Z/2003-06-21T22:00:53Z
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	2004-07-19T00:00:00Z
Keywords	"XMM", "xray brightest", "constrain cosmological parameters", "total mass profiles", "optical observatories", "bcs lensing", "dark matter", "XMM-Newton", "weak lensing data", "rosat xbacs", "xray temperature", "bright gravitational arcs", "ROSAT", "xray gas mass", "HST", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Steve Allen, 2004, 'XMM-Newton observations of the brightest relaxed cluster lenses', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-yq7umuc