A dataset provided by the European Space Agency

Name 010846
Title The Mass and Abundance Profiles of Clusters Out to the Virial Radius
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108460101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108460201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0108460301

DOI 10.5270/esa-j5kva5m
Author Dr Richard Mushotzky
Description GT- We propose to observe three luminous clusters at redshift approximately one-tenth with XMM in order to measure temperature and abundance profiles out to the virial radius -- the largest radius at which the cluster is expected to be in dynamical equilibrium. The temperature profile will be of sufficient extent and precision to constrain the shape of the dark matter spatial distribution, as well as the total mass. The total and relative abundance profiles are a powerful probe of the star formation and mass loss history of cluster galaxies. .
Publication The XMM-Newton Needles in the Haystack Survey: the local X-ray luminosity function of 'normal. galaxies . Georgantopoulos, I., Georgakakis, A., . MNRAS . 360-782 . 2005 . 2005MNRAS.360..782G ,
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 structural and scaling properties of nearby galaxy clusters. II. The M-T relation . Arnaud, M., Pointecouteau, E., . A&A . 441-893 . 2005 . 2005A&A...441..893A ,
The Needles in the Haystack Survey: searching for X-ray-selected normal galaxies . Georgakakis, A. E., Georgantopoulos, I., et all. . MNRAS . 354-123 . 2004 . 2004MNRAS.354..123G ,
Normal galaxies in the XMM-Newton fields. X-rays as a star formation indicator . Rovilos, E., Georgantopoulos, I., et all. . A&A . 502-85 . 2009 . 2009A&A...502...85R ,
An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
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., ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-11-30T03:29:02Z/2003-01-10T09:42:45Z
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 2004-02-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-02-21T00:00:00Z, 010846, 17.56_20190403_1200. https://doi.org/10.5270/esa-j5kva5m