A dataset provided by the European Space Agency

Name: The merging cluster RXCJ0548-2154 with a Radio Relic
Published: 2017-04-12T22:00:00Z

Proposal ID	076097
Title	The merging cluster RXCJ0548-2154 with a Radio Relic
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760970101
DOI	https://doi.org/10.5270/esa-84fmd59
Principal Investigator, PI	Prof Hans Boehringer
Abstract	The cluster RXCJ0548-2154 (A3365) is a merging system with a pronouncedperipheralradio relic. Similar to the prototype system A3667 the relic is almostaligned with the merger axis and the cluster shows a simple head-on mergergeometry. This clear morphology and the fact that the cluster has a low redshiftof z=0.0928 makes it a very attractive object for the study of the mergingprocess in connection with cosmic ray acceleration. To detect a shock near therelic position, to get a postshock temperature, and to unravel the mergerdynamics we propose a deeper XMM-Newton observation of 120 ks.
Publications	Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers \|Golovich N. Dawson W. A. et al. \| ApJ \| 882-69 \| 2019 \| 2019ApJ...882...69G \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...882...69G X-ray study of Abell 3365 with XMM-Newton \|Urdampilleta I. Simionescu A. et al. \| A&A \| 646-95 \| 2021 \| 2021A&A...646A..95U \| http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..95U 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 Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan Z. S. Han J. L. \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y 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 X-ray spectroscopy of merging galaxy clusters \|Urdampilleta Igone \| PhDT \| 0-14 \| 2019 \| 2019PhDT........14U \| http://ui.adsabs.harvard.edu/#abs/2019PhDT........14U New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-03-29T05:40:36Z/2016-03-30T18:10:36Z
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	2017-04-12T22:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "low redshift", "merging process", "XMM-Newton", "merger dynamics", "cosmic ray acceleration", "merger axis", "attractive object", "simple head", "deeper xmm newton", "0928 makes", "merger geometry", "pronounced peripheralradio relic", "merging system", "radio relic", "prototype system a3667", "postshock temperature", "relic position"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Hans Boehringer, 2017, 'The merging cluster RXCJ0548-2154 with a Radio Relic', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-84fmd59