A dataset provided by the European Space Agency

Name: Unveiling the most massive clusters at z>0.5 with Planck and XMM-Newton.
Published: 2014-02-05T00:00:00Z

Proposal ID	069366
Title	Unveiling the most massive clusters at z>0.5 with Planck and XMM-Newton.
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693660101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693660301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693660401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693660501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693660601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693660701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693660801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661301 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693661901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693662101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693662301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693662501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693662701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693662801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693662901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693663001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693663101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693663201
DOI	https://doi.org/10.5270/esa-ngf0ztw
Principal Investigator, PI	Dr monique arnaud
Abstract	We propose to gather spatially resolved spectroscopy of a sample of 33 massive(M_{500}>5e+14 solar masses) clusters detected blindly by Planck and confirmedto-day to be in the redshift range 0.5
Publications	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 Discovery of radio haloes and double relics in distant MACS galaxy clusters: clues to the efficiency of particle acceleration \|Bonafede A. Bruggen M. et al. \| MNRAS \| 426-40 \| 2012 \| 2012MNRAS.426...40B \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426...40B Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMO \|Mroczkowski T. Kovacs A. et al. \| ApJ \| 808-6 \| 2015 \| 2015ApJ...808L...6M \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...808L...6M New XMM-Newton observation of the Phoenix cluster: properties of the cool core \|Tozzi P. Gastaldello F. et al. \| A&A \| 580-6 \| 2015 \| 2015A&A...580A...6T \| http://ui.adsabs.harvard.edu/#abs/2015A&A...580A...6T 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 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 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 Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71 \|Ruppin F. Adam R. et al. \| A&A \| 597-110 \| 2017 \| 2017A&A...597A.110R \| http://ui.adsabs.harvard.edu/#abs/2017A&A...597A.110R 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 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 The close environments of accreting massive black holes are shaped by radiative feedback \|Ricci Claudio Trakhtenbrot Benny et al. \| Natur \| 549-488 \| 2017 \| 2017Natur.549..488R \| http://ui.adsabs.harvard.edu/#abs/2017Natur.549..488R BAT AGN Spectroscopic Survey (BASS) - VI. The GammaX-L/LEdd relation \|Trakhtenbrot Benny Ricci Claudio et al. \| MNRAS \| 470-800 \| 2017 \| 2017MNRAS.470..800T \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..800T BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog \|Ricci C. Trakhtenbrot B. et al. \| ApJS \| 233-17 \| 2017 \| 2017ApJS..233...17R \| http://ui.adsabs.harvard.edu/#abs/2017ApJS..233...17R The Swift/BAT AGN Spectroscopic Survey. IX. The Clustering Environments of an Unbiased Sample of Local AGNs \|Powell M. C. Cappelluti N. et al. \| ApJ \| 858-110 \| 2018 \| 2018ApJ...858..110P \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...858..110P Substructure and merger detection in resolved NIKA Sunyaev-Zeldovich images of distant clusters \|Adam R. Hahn O. et al. \| A&A \| 614-118 \| 2018 \| 2018A&A...614A.118A \| http://ui.adsabs.harvard.edu/#abs/2018A&A...614A.118A AGN feedback in the Phoenix cluster \|Pinto C. Bambic C. J. et al. \| MNRAS \| 480-4113 \| 2018 \| 2018MNRAS.480.4113P \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480.4113P 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 X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton \|Bulbul Esra Chiu I.-Non et al. \| ApJ \| 871-50 \| 2019 \| 2019ApJ...871...50B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...871...50B The XMM-Newton serendipitous survey. VIII. The first XMM-Newton serendipitous source catalogue from overlapping observations \|Traulsen I. Schwope A. D. et al. \| A&A \| 624-77 \| 2019 \| 2019A&A...624A..77T \| http://ui.adsabs.harvard.edu/#abs/2019A&A...624A..77T Hot corona properties of Swift/BAT-detected AGNs \|Wang Chan Yu Li-Ming et al. \| MNRAS \| 487-2463 \| 2019 \| 2019MNRAS.487.2463W \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.2463W LOFAR Discovery of a Radio Halo in the High-redshift Galaxy Cluster PSZ2 G099.86+58.45 \|Cassano R. Botteon A. et al. \| ApJ \| 881-18 \| 2019 \| 2019ApJ...881L..18C \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...881L..18C 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 Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster \|McDonald M. McNamara B. R. et al. \| ApJ \| 885-63 \| 2019 \| 2019ApJ...885...63M \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...885...63M Mass variance from archival X-ray properties of Dark Energy Survey Year-1 galaxy clusters \|Farahi A. Chen X. et al. \| MNRAS \| 490-3341 \| 2019 \| 2019MNRAS.490.3341F \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.490.3341F 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 The BUFFALO HST Survey \|Steinhardt Charles L. Jauzac Mathilde et al. \| ApJS \| 247-64 \| 2020 \| 2020ApJS..247...64S \| http://ui.adsabs.harvard.edu/#abs/2020ApJS..247...64S Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy - II. The X-ray luminosity-mass relation \|Capasso R. Mohr J. J. et al. \| MNRAS \| 494-2736 \| 2020 \| 2020MNRAS.494.2736C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.2736C Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z u223c 1 \|Gupta N. Pannella M. et al. \| MNRAS \| 494-1705 \| 2020 \| 2020MNRAS.494.1705G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.1705G A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava S. Giles P. A. et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B A new multiwavelength census of blazars \|Paggi A. Bonato M. et al. \| A&A \| 641-62 \| 2020 \| 2020A&A...641A..62P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A..62P 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 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 The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou Min-Hua Gu Min-Feng \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z Fast magnetic field amplification in distant galaxy clusters \|Di Gennaro Gabriella van Weeren Reinout J. et al. \| NatAs \| 5-268 \| 2021 \| 2021NatAs...5..268D \| http://ui.adsabs.harvard.edu/#abs/2021NatAs...5..268D Constraints on the variation of fine structure constant from joint SPT-SZ and XMM-Newton observations \|Bora Kamal Desai Shantanu \| JCAP \| 2-12 \| 2021 \| 2021JCAP...02..012B \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...02..012B A test of cosmic distance duality relation using SPT-SZ galaxy clusters Type Ia supernovae and cosmic chronometers \|Bora Kamal Desai Shantanu \| JCAP \| 6-52 \| 2021 \| 2021JCAP...06..052B \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...06..052B 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 The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview \|CHEX-MATE Collaboration Arnaud M. et al. \| A&A \| 650-104 \| 2021 \| 2021A&A...650A.104C \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.104C Discovery of Three Candidate Magnetar-powered Fast X-Ray Transients from Chandra Archival Data \|Lin Dacheng Irwin Jimmy A. et al. \| ApJ \| 927-211 \| 2022 \| 2022ApJ...927..211L \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...927..211L The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview \|Botteon A. Shimwell T. W. et al. \| A&A \| 660-78 \| 2022 \| 2022A&A...660A..78B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B A highly magnified star at redshift 6.2 \|Welch Brian Coe Dan et al. \| Natur \| 603-815 \| 2022 \| 2022Natur.603..815W \| http://ui.adsabs.harvard.edu/#abs/2022Natur.603..815W CHEX-MATE: Morphological analysis of the sample \|Campitiello M. G. Ettori S. et al. \| A&A \| 665-117 \| 2022 \| 2022A&A...665A.117C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A.117C 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 Hidden Cooling Flows in clusters of Galaxies II: a wider sample \|Fabian A. C. Sanders J. S. et al. \| MNRAS \| 521-1794 \| 2023 \| 2023MNRAS.521.1794F \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.521.1794F The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium \|Zhang X. Simionescu A. et al. \| A&A \| 672-42 \| 2023 \| 2023A&A...672A..42Z \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models \|Cassano R. Cuciti V. et al. \| A&A \| 672-43 \| 2023 \| 2023A&A...672A..43C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C CHEX-MATE: Pressure profiles of six galaxy clusters as seen by SPT and Planck \|Oppizzi F. De Luca F. et al. \| A&A \| 672-156 \| 2023 \| 2023A&A...672A.156O \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A.156O 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 CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles \|Bartalucci I. Molendi S. et al. \| A&A \| 674-179 \| 2023 \| 2023A&A...674A.179B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A.179B CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters \|Bourdin H. De Luca F. et al. \| A&A \| 678-181 \| 2023 \| 2023A&A...678A.181B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.181B Characterizing the bulk and turbulent gas motions in galaxy clusters \|Dupourquu00e9 Simon Pointecouteau Etienne et al. \| EPJWC \| 257-00015 \| 2022 \| 2022EPJWC.25700015D \| http://ui.adsabs.harvard.edu/#abs/2022EPJWC.25700015D Pressure profiles of distant Galaxy clusters with Planck-SPT data \|Oppizzi Filippo De Luca Federico et al. \| EPJWC \| 257-00035 \| 2022 \| 2022EPJWC.25700035O \| http://ui.adsabs.harvard.edu/#abs/2022EPJWC.25700035O Exploring X-Ray Properties of Low-metallicity Dwarf Galaxies \|Cann Jenna M. Weaver Kimberly A. et al. \| ApJ \| 961-178 \| 2024 \| 2024ApJ...961..178C \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..178C 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 A New Dissociative Galaxy Cluster Merger: RM J150822.0+575515.2 \|Stancioli Rodrigo Wittman David et al. \| ApJ \| 966-49 \| 2024 \| 2024ApJ...966...49S \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...966...49S 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	RGS1, EPN, RGS2, EMOS1, OM, EMOS2
Temporal Coverage	2012-05-19T04:12:10Z/2013-01-13T18:44:14Z
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	2014-02-05T00:00:00Z
Last Update	2025-01-27
Keywords	"redshift regime", "XMM", "resolved spectroscopy", "fundamental scalings", "massive cluster", "cosmological exploitation", "complementary vlt", "XMM-Newton", "massive m_", "redshift range", "entropy profiles", "planck collaboration", "solar masses cluster", "xmm newton ..", "}> 5e", "cluster gravitational collapse"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr monique arnaud, 2014, 'Unveiling the most massive clusters at z>0.5 with Planck and XMM-Newton.', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ngf0ztw