A dataset provided by the European Space Agency

Name 030021
Title The Local Galaxy Cluster Mass Function of the Brightest Clusters in the Sky
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300210201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300210301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300210401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300210501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300210601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300210701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300211001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300211101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300211301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0300211401

DOI 10.5270/esa-r6nq1h2
Author Dr Thomas Reiprich
Description Galaxy clusters have proven to be highly competitive and complementary cosmo- logical probes. For the next major breakthrough more reliable mass estimates and, therefore, a better understanding of cluster physics are essential. We propose to complete XMM-Newton observations of a flux-limited sample of the 63 X-ray brightest clusters in the sky to (i) take full advantage of ~3Ms of XMM-Newton data already available, (ii) determine very precise gas temperature profiles, (iii) characterize merging clusters by direct comparison to simulations, (iv) update the luminosity--mass relation, (v) construct the most precise local cluster mass function, (vi) improve constraints on OmegaM and sigma8 significantly, and (vii) provide a reliable statistical baseline for comparison to high-redshift samples.
Publication A joint Chandra and XMM-Newton view of Abell 3158: a massive off-centre cool gas clump as a robust diagnostic of a merger stage . Wang, Yu, Xu, Haiguang, et all. . MNRAS . 403-1909 . 2010 . 2010MNRAS.403.1909W ,
HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion . Zhang, Y.-Y., Andernach, H., et all. . A&A . 526-105 . 2011 . 2011A&A...526A.105Z ,
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 Energy Dependence of the Relation Between Optical and X-ray Emission in Quasars . Young, M., Elvis, M., . ApJ . 708-1388 . 2010 . 2010ApJ...708.1388Y ,
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 ,
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 ,
Using the XMM-Newton Optical Monitor to Study Cluster Galaxy Evolution . Miller, Neal A., O.Steen, Richard, et all. . PASP . 124-95 . 2012 . 2012PASP..124...95M ,
Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations . Planck Collaboration,...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-06-24T13:04:39Z/2006-06-24T20:35:16Z
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 2008-01-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-01-05T00:00:00Z, 030021, 17.56_20190403_1200. https://doi.org/10.5270/esa-r6nq1h2