A dataset provided by the European Space Agency

Name: Unveiling the most massive clusters at z&gt;0.5 with Planck and XMM-Newton.
Published: 2014-02-09T00:00:00Z

Proposal ID	070018
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=0700180201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700180901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700182001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700182201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0700182401
DOI	https://doi.org/10.5270/esa-xsgt4vz
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<z<1. Using for the first time astatistically significant sample in this high-mass, high-redshift regime, wewill study the fundamental scalings between Y_SZ, Y_X and M_500, and thepressure and entropy profiles. This will provide an important probe of thephysics of cluster gravitational collapse and be of large legacy value for thecosmological exploitation of the Planck sample. Complementary VLT observationsare proposed. This proposal is submitted on behalf of the Planck collaboration.
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 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 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 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 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 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 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 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 four super-soft X-ray sources in XMM-Newton observations of the Large Magellanic Cloud \|Maitra, C., Haberl, F., \| A&A \| 657-26 \| 2022 \| 2022A&A...657A..26M \| http://ui.adsabs.harvard.edu/#abs/2022A&A...657A..26M ESASky SSOSS: Solar System Object Search Service and the case of Psyche \|Racero, E., Giordano, F., et al. \| A&A \| 659-38 \| 2022 \| 2022A&A...659A..38R \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..38R 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 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 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 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	2012-05-02T09:33:31Z/2013-01-20T17:55:43Z
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	2014-02-09T00:00:00Z
Keywords	"massive cluster", "entropy profiles", "cosmological exploitation", "complementary vlt", "solar masses cluster", "XMM", "}> 5e", "redshift range", "planck collaboration", "xmm newton ..", "cluster gravitational collapse", "XMM-Newton", "fundamental scalings", "redshift regime", "resolved spectroscopy", "massive m_"
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-xsgt4vz