We propose to use XMM-Newton to observe an exceptional cluster at z = 1.47discovered via the Sunyaev-Zel.dovich (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.
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
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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
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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
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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.
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
