A dataset provided by the European Space Agency

Name 005774
Title The Physical Properties of the Intra-Cluster Gas at z > 1
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057740301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057740401

DOI 10.5270/esa-0bz3i16
Author Dr Piero Rosati
Description We propose deep EPIC observations of two X-ray selected spectroscopically confirmed, clusters at z=1.10 and z=1.23. High S-N X-ray imaging and spectroscopy will allow us to measure, for the first time, both the temperature and the metallicity of the intra-cluster gas in two bona-fide clusters at z>1, with unprecented insight in their physical properties. Given the large look-back time, these measurements: 1. will yield an estimate of the cluster masses with direct implications on cosmological models; 2. will permit to study evolutionary effects on the cluster Lx-T relation; 3. will also constrain the mode and epoch of metal enrichment of the gas.
Publication Chandra and XMM-Newton Observations of RDCS 1252.9-2927, A Massive Cluster at z=1.24 . Rosati, P., Tozzi, P., et all. . AJ . 127-230 . 2004 . 2004AJ....127..230R ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project . Fassbender, R., Bohringer, H., et all. . NJPh . 13-125014 . 2011 . 2011NJPh...13l5014F ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters . Baldi, A., Ettori, S., et all. . A&A . 537-142 . 2012 . 2012A&A...537A.142B ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
A deficit of faint red galaxies in the possible large-scale structures around the RDCS J1252.9-2927 cluster at z = 1.24 . Tanaka, Masayuki, Kodama, Tadayuki, et all. . MNRAS . 377-1206 . 2007 . 2007MNRAS.377.1206T ,
Redshift Evolution in the Iron Abundance of the Intracluster Medium . Anderson, Michael E.,...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-01-03T01:54:11Z/2003-01-11T19:49:30Z
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 2004-05-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-05-20T00:00:00Z, 005774, 17.56_20190403_1200. https://doi.org/10.5270/esa-0bz3i16