A dataset provided by the European Space Agency

Name 086297
Title A spectacular LOFAR-selected merging galaxy cluster
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862970101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0862970201

DOI https://doi.org/10.5270/esa-[xxxxxxx]
Author Dr Andra Stroe
Description Relics are diffuse radio sources thought to trace shocks at the periphery of merging clusters. LOFAR, with its unique resolution and sensitivity, is revolutionizing the field by opening a new window of discovery. The LOFAR survey recently discovered a rare example of double relics in a low-mass cluster, confirmed as a 3:1 merger by our Cy21 Chandra observations. The bright relics are located exceptionally far away from the cluster core -- at about R500 (1.3 Mpc). The properties of the radio sources are hard to reconcile with current relic formation models, given the low cluster mass. We propose XMM-Newton observations to study the luminosity and temperature substructure, understand the cluster merger history and place tight constraints on relic formation models.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2020-05-05T02:14:25Z/2020-05-07T18:26:10Z
Version 18.02_20200221_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2021-05-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2021-05-21T00:00:00Z, 086297, 18.02_20200221_1200. https://doi.org/10.5270/esa-[xxxxxxx]