A dataset provided by the European Space Agency

Name: X-ray Observations of a SZ Discovered Cluster at z=1.45
Published: 2014-04-18T00:00:00Z

Proposal ID	069438
Title	X-ray Observations of a SZ Discovered Cluster at z=1.45
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694380101
DOI	https://doi.org/10.5270/esa-7m0e65p
Principal Investigator, PI	Dr Bradford Benson
Abstract	We propose to use XMM-Newton to observe an exceptional cluster at z=1.45discovered via the Sunyaev-Zeldovich (SZ) effect by the South Pole Telescope(SPT). The cluster, SPT-CLJ2109-4626, is the highest redshift cluster yetdiscovered by SPT, with a Spitzer-optical red-sequence redshift of z=1.45. Wepredict that SPT-CL J2109-4626 has a mass of 4.0e14 M_sun, an X-ray temperatureof 5.9 keV, and an X-ray luminosity of 9.8e44 ergs/s. These properties wouldplace SPT-CL J2109-4626 amongst the most massive known clusters at z > 1.4, andan important system to study the earliest forming massive clusters. We arerequesting a 60 ksec observation, enough to obtain 1500 X-ray photons, measurean X-ray luminosity and temperature, and to assess the dynamical state of this exceptional young 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 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 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	2013-04-05T06:35:04Z/2013-04-06T01:57:38Z
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	2014-04-18T00:00:00Z
Last Update	2025-01-27
Keywords	"spt clj2109 4626", "8e44 ergs", "1500 xray photons", "xmm newton", "XMM-Newton", "x ray", "xray temperature", "redshift cluster", "XMM", "xray luminosity", "0e14 m_sun"
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=1.45', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7m0e65p