A dataset provided by the European Space Agency

Name 076207
Title Origin of the SZ and Radio Structures in the Massive CLASH Cluster MACS J1206
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762070101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762070201

DOI 10.5270/esa-zm9lgzc
Author Prof Craig Sarazin
Description MACSJ1206 is a very massive hot cluster which is part of the CLASH sample. Our high resolution MUSTANG SZ image shows an excess NE of the cluster core which is coincident with a large group of galaxies seen optically and in weak lensing. We will detect the X-rays from this group, and determine if it is foreground or infalling (perhaps with a shock) into MACSJ1206. GMRT radio data show an extended feature to the W of the cluster center. We will determine if this is a radio relic or displaced radio lobe. MACSJ1206 has very extensive galaxy velocity and lensing data, and the masses agree well. We will determine the X-ray hydrostatic mass out of 1.5 Mpc; comparison to the lensing and dynamical masses will give the strongest constraints on hydrostatic bias in X-ray masses.
Publication X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L ,
Thermodynamic profiles of galaxy clusters from a joint X-ray-SZ analysis . Shitanishi, Jennifer A., Pierpaoli, Elena, et all. . MNRAS . 481-749 . 2018 . 2018MNRAS.481..749S ,
X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton . Lovisari, Lorenzo, Schellenberger, Gerrit, et all. . ApJ . 892-102 . 2020 . 2020ApJ...892..102L ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-07-11T21:31:03Z/2015-07-13T11:46:33Z
Version PPS_NOT_AVAILABLE
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 2016-07-23T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016-07-23T22:00:00Z, 076207, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-zm9lgzc