A dataset provided by the European Space Agency

Name: The dark matter distribution in high redshift clusters: probing evolution.
Published: 2010-04-02T00:00:00Z

Proposal ID	055185
Title	The dark matter distribution in high redshift clusters: probing evolution.
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551850101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551850201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551850401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551850601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551850901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551851201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551851301
DOI	https://doi.org/10.5270/esa-fqtt7h1
Principal Investigator, PI	Dr Monique ARNAUD
Abstract	We propose to measure the mass profiles of a complete sample of massive, relaxedgalaxy clusters at z greater than 0.5, with a precision equal to that currentlyobtained for local objects. We will assess the evolution of the dark matterconcentration at cluster scales, a critical test of theoretical scenario ofstructure formation. This data set will also strongly constrain the evolution offundamental mass-proxy relations and the evolution of the gas entropy profilesin the high mass regime, a critical test of gravitational gas heating.
Publications	An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters \|Baldi A. Ettori S. et al. \| A&A \| 537-142 \| 2012 \| 2012A&A...537A.142B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...537A.142B 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 Self-similarity of temperature profiles in distant galaxy clusters: the quest for a universal law \|Baldi A. Ettori S. et al. \| A&A \| 545-41 \| 2012 \| 2012A&A...545A..41B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..41B An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H Structure and substructure analysis of DAFT/FADA galaxy clusters in the 0.4-0.9 redshift range \|Guennou L. Adami C. et al. \| A&A \| 561-112 \| 2014 \| 2014A&A...561A.112G \| http://ui.adsabs.harvard.edu/#abs/2014A&A...561A.112G Scaling Relations and X-Ray Properties of Moderate-luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton \|Connor Thomas Donahue Megan et al. \| ApJ \| 794-48 \| 2014 \| 2014ApJ...794...48C \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...794...48C 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 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 Weak lensing study of 16 DAFT/FADA clusters: Substructures and filaments \|Martinet Nicolas Clowe Douglas et al. \| A&A \| 590-69 \| 2016 \| 2016A&A...590A..69M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...590A..69M 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 The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 Gas mass fractions from XMM-Newton \|Della Monica Ferreira Desiree \| PhDT \| 0-186 \| 2011 \| 2011PhDT.......186D \| http://ui.adsabs.harvard.edu/#abs/2011PhDT.......186D Pressure Profiles of Distant Galaxy Clusters in the Planck Catalogue \|Bourdin H. Mazzotta P. et al. \| ApJ \| 843-72 \| 2017 \| 2017ApJ...843...72B \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...843...72B 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 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 First Sunyaev-Zeldovich mapping with the NIKA2 camera: Implication of cluster substructures for the pressure profile and mass estimate \|Ruppin F. Mayet F. et al. \| A&A \| 615-112 \| 2018 \| 2018A&A...615A.112R \| http://ui.adsabs.harvard.edu/#abs/2018A&A...615A.112R The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching \|van der Burg Remco F. J. McGee Sean et al. \| A&A \| 618-140 \| 2018 \| 2018A&A...618A.140V \| http://ui.adsabs.harvard.edu/#abs/2018A&A...618A.140V 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 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 An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 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 Comparison of hydrostatic and lensing cluster mass estimates: A pilot study in MACS J0647.7+7015 \|Ferragamo A. Macu00edas-Pu00e9rez J. F. et al. \| A&A \| 661-65 \| 2022 \| 2022A&A...661A..65F \| http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..65F The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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 X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf J. Nandra K. et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W Xu2011HESS: A large sample of highly accreting serendipitous AGN under the XMMu2011Newton microscope \|Laurenti M. Tombesi F. et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L 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	2008-07-13T08:03:58Z/2009-03-23T01:10:19Z
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	2010-04-02T00:00:00Z
Last Update	2025-01-27
Keywords	"gravitational gas heating", "mass profiles", "complete sample", "probing evolution ..", "relaxed galaxy cluster", "local objects", "dark matter distribution", "structure formation", "redshift clusters", "mass regime", "cluster scales", "dark matter concentration", "data set", "precision equal", "gas entropy profiles"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Monique ARNAUD, 2010, 'The dark matter distribution in high redshift clusters: probing evolution.', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fqtt7h1