A dataset provided by the European Space Agency

Name 074385
Title XMM Frontier Observation of the Pandora Cluster
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743850101

DOI 10.5270/esa-69xlwo3
Author Prof Jean-Paul Kneib
Description We propose a deep XMM 100 ksec observation of the A2744 a unique massive cluster merger: the Pandora cluster. A2744 is the first of the six Frontier Field Clusters to be observed with HST, reaching unprecedented depth. With the proposed observation we will: 1) study the thermodynamic properties and metallicity of the complex merging taking place in the cluster core; 2) compare the lensing and hydrostatic mass estimates of the cluster and the different sub clumps identified; 3) map the large-scale matter distribution out to the virial radius where current data reveal possible substructure not yet confirmed that may contribute to the growth of the cluster. This data set will be of legacy value considering the HST Frontier Field initiative, we suggest to have no data proprietary right.
Publication Probing the evolution of the substructure frequency in galaxy clusters up to z ~ 1 . Weissmann, A., Bohringer, H., . A&A . 555-147 . 2013 . 2013A&A...555A.147W ,
Warm--hot baryons comprise 5--10 per cent of filaments in the cosmic web . Eckert, Dominique, Jauzac, Mathilde, et all. . Natur . 528-105 . 2015 . 2015Natur.528..105E ,
Frontier Fields: Subaru Weak-Lensing Analysis of the Merging Galaxy Cluster A2744 . Medezinski, Elinor, Umetsu, Keiichi, et all. . ApJ . 817-24 . 2016 . 2016ApJ...817...24M ,
A shock front at the radio relic of Abell 2744 . Eckert, D., Jauzac, M., et all. . MNRAS . 461-1302 . 2016 . 2016MNRAS.461.1302E ,
The extraordinary amount of substructure in the Hubble Frontier Fields cluster Abell 2744 . Jauzac, M., Eckert, D., et all. . MNRAS . 463-3876 . 2016 . 2016MNRAS.463.3876J ,
A study of halo and relic radio emission in merging clusters using the Murchison Widefield Array . George, L. T., Dwarakanath, K. S., et all. . MNRAS . 467-936 . 2017 . 2017MNRAS.467..936G ,
X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L ,
Search for the warm-hot intergalactic medium around A 2744 using Suzaku . Hattori, Shiho, Ota, Naomi, et all. . PASJ . 69-39 . 2017 . 2017PASJ...69...39H ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-12-18T19:09:13Z/2014-12-20T02:14:13Z
Version 17.56_20190403_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 2016-01-13T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016-01-13T23:00:00Z, 074385, 17.56_20190403_1200. https://doi.org/10.5270/esa-69xlwo3