A dataset provided by the European Space Agency

Name: Unveiling the most massive Planck clusters at z>0.5 (XMM LP re-observations).
Published: 2014-12-20T23:00:00Z

Proposal ID	072378
Title	Unveiling the most massive Planck clusters at z>0.5 (XMM LP re-observations).
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723780101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723780201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723780301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723780401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723780501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723780601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723780701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723780801
DOI	https://doi.org/10.5270/esa-jiu2l8y
Principal Investigator, PI	Dr Monique ARNAUD
Abstract	We have been awarded a Large Program in AO11 to gather spatially resolved X rayspectroscopy on a sample of 32 massive (M_500 > 5e+14Msun) clusters detectedblindly by Planck in the redshift range 0.5
Publications	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 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 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 Gravitational lensing detection of an extremely dense environment around a galaxy cluster \|Sereno Mauro Giocoli Carlo et al. \| NatAs \| 2-744 \| 2018 \| 2018NatAs...2..744S \| http://ui.adsabs.harvard.edu/#abs/2018NatAs...2..744S 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 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 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 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 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 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 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 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 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 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 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	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-05-19T19:46:46Z/2013-11-30T22:19:43Z
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	2014-12-20T23:00:00Z
Last Update	2025-01-27
Keywords	"massive planck cluster", "redshift regime", "planck sample", "M500", "fundamental scalings", "massive m_500", "xmm lp re", "cosmological exploitation", "resolved xray spectroscopy", "entropy profiles", "redshift range", "XMM", "cluster gravitational collapse", "14msun cluster"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Monique ARNAUD, 2014, 'Unveiling the most massive Planck clusters at z>0.5 (XMM LP re-observations).', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jiu2l8y