A dataset provided by the European Space Agency

Name: PKS B1400-33 and Abell S753: A Very Bright Radio Relic in a Poor Cluster
Published: 2015-08-25T22:00:00Z

Proposal ID	074193
Title	PKS B1400-33 and Abell S753: A Very Bright Radio Relic in a Poor Cluster
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741930101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741930201
DOI	https://doi.org/10.5270/esa-4axets0
Principal Investigator, PI	Prof Craig Sarazin
Abstract	The cluster radio relic PKS B1400-33 in the poor cluster Abell S753 will beobserved with XMM/Newton and NuSTAR to detect and image the nonthermal InverseCompton emission. This is the second brightest cluster radio relic known.Remarkably, it is associated with a relatively poor, cool cluster. Although ithas many properties similar to other cluster radio relics, it is possible thatit is an old radio lobe, displaced by motions or buoyancy. These observationswill be a strong test of merger shock acceleration processes, and will give themagnetic field, nonthermal energy, and shock acceleration efficiency. Theobservations will allow the dynamical state of the cluster to be determined, andwill detect the merger shock which is expected to be associated with the relic.
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 The non-uniformity of galaxy cluster metallicity profiles \|Lovisari L. Reiprich T. H. \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L 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 Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey. IV. Superclusters in the local Universe at z u2264 0.03 \|Bu00f6hringer Hans Chon Gayoung \| A&A \| 656-144 \| 2021 \| 2021A&A...656A.144B \| http://ui.adsabs.harvard.edu/#abs/2021A&A...656A.144B 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	2014-07-25T21:32:51Z/2014-07-27T12:51:08Z
Version	PPS_NOT_AVAILABLE
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	2015-08-25T22:00:00Z
Last Update	2025-01-27
Keywords	"shock acceleration efficiency", "magnetic field", "abell s753", "bright radio relic", "nonthermal energy", "cluster radio relics", "Abell ", "cluster abell s753", "merger shock", "NuSTAR", "cool cluster", "XMM", "cluster radio relic", "radio lobe"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Craig Sarazin, 2015, 'PKS B1400-33 and Abell S753: A Very Bright Radio Relic in a Poor Cluster', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-4axets0