A dataset provided by the European Space Agency

Name 014021
Title XMM-VLT Study of Cosmic Evolution with Groups and Clusters of Galaxies
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0140210101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0140210201

DOI 10.5270/esa-wurtbbx
Author Dr Hans Boehringer
Description We propose to use the combined observational power of XMM-Newton and VLT to study important aspects of cosmic evolution with massive clusters and groups of galaxies. Using a small sample of well defined, X-ray selected very massive clusters and groups of galaxies from the REFLEX Survey as cosmic laboratories we aim for a simultaneous study of the cluster masses and mass-to-light ratios, the dynamical ages, the mass fractions of various matter components, the galaxy populations, the heavy element abundances, the supernova rates, the entropy structure of the intracluster medium, and the large scale structure environments of these systems. Most importantly we will study the interconnections and correlations of these phenomena.
Publication 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 ,
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 ,
2XMM ultraluminous X-ray source candidates in nearby galaxies . Walton, D. J., Roberts, T. P., et all. . MNRAS . 416-1844 . 2011 . 2011MNRAS.416.1844W ,
The X-Ray Concentration-Virial Mass Relation . Buote, David A., Gastaldello, Fabio, et all. . ApJ . 664-123 . 2007 . 2007ApJ...664..123B ,
Probing the Dark Matter and Gas Fraction in Relaxed Galaxy Groups with X-Ray Observations from Chandra and XMM-Newton . Gastaldello, Fabio, Buote, David A., et all. . ApJ . 669-158 . 2007 . 2007ApJ...669..158G ,
A large catalogue of ultraluminous X-ray source candidates in nearby galaxies . Walton, D. J., Gladstone, J. C., et all. . AN . 332-354 ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-12-20T11:20:10Z/2003-03-26T07:27:44Z
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 2004-04-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-04-16T00:00:00Z, 014021, 17.56_20190403_1200. https://doi.org/10.5270/esa-wurtbbx