A dataset provided by the European Space Agency

Name: X-ray Observations of a SZ Discovered Cluster at z = 1.47
Published: 2014-10-19T00:00:00Z

Proposal ID	072329
Title	X-ray Observations of a SZ Discovered Cluster at z = 1.47
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723290101
DOI	https://doi.org/10.5270/esa-f30x65k
Principal Investigator, PI	Dr Bradford Benson
Abstract	We propose to use XMM-Newton to observe an exceptional cluster at z = 1.47discovered via the Sunyaev-Zeldovich (SZ) effect by the South Pole Telescope(SPT). The cluster, SPT-CL J2040-4451, is the highest redshift cluster yetdiscovered by SPT, with a spectroscopic redshift of z=1.47. We predict thatSPT-CL J2040-4451 has a mass of 5.6e14 Msun, an X-ray temperature of 6.0 keV,and an X-ray luminosity of 11e44 ergs/s. These properties would place SPT-CLJ2040-4451 amongst the most massive known clusters at z > 1.4, and an importantsystem to study the earliest forming massive clusters. We are requesting a 75ksec observation with XMM-Newton; enough to obtain 2000 X-ray photons, andmeasure an X-ray luminosity and temperature of this young massive cluster.
Publications	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 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 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 Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8 \|Ghirardini Vittorio Bulbul Esra et al. \| ApJ \| 910-14 \| 2021 \| 2021ApJ...910...14G \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910...14G 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 Thermodynamic evolution of the z = 1.75 galaxy cluster IDCS J1426.5+3508 \|Andreon S. Romero C. et al. \| MNRAS \| 505-5896 \| 2021 \| 2021MNRAS.505.5896A \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.505.5896A 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 history of metal enrichment traced by X-ray observations of high-redshift galaxy clusters \|Flores Anthony M. Mantz Adam B. et al. \| MNRAS \| 507-5195 \| 2021 \| 2021MNRAS.507.5195F \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5195F 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	2013-10-04T09:30:31Z/2013-10-05T08:35:31Z
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	2014-10-19T00:00:00Z
Last Update	2025-01-27
Keywords	"dovich sz effect", "spectroscopic redshift", "xmm newton", "XMM-Newton", "x ray", "2000 xray photons", "xray temperature", "11e44 ergs", "XMM", "redshift cluster", "xray luminosity", "sunyaev zel", "6e14 msun"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Bradford Benson, 2014, 'X-ray Observations of a SZ Discovered Cluster at z = 1.47', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-f30x65k