Mathematics – Logic
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..103b&link_type=abstract
XMM-Newton Proposal ID #02019032
Mathematics
Logic
Rxcj0003.8+0203, Rxcj0006.0-3443, Rxcj0020.7-2542, Rxcj0049.4-2931, Rxcj0145.0-5300, Rxcj0211.4-4017, Rxcj0225.1-2928, Rxcj0345.7-4112, Rxcj0547.6-3152, Rxcj0605.8-3518, Rxcj0616.8-4748, Rxcj0645.4-5413, Rxcj0821.8+0112, Rxcj0958.3-1103, Rxcj1044.5-0704, Rxcj1141.4-1216, Rxcj1236.7-3354, Rxcj1302.8-0230, Rxcj1350.7-3343, Rxcj1516.3+0005, Rxcj1516.5-0056, Rxcj2014.8-2430, Rxcj2023.0-2056, Rxcj2048.1-1750, Rxcj2129.8-5048, Rxcj2149.1-3041, Rxcj2152.2-1942, Rxcj2157.4-0747, Rxcj2217.7-3543, Rxcj2218.6-3853, Rx
Scientific paper
Galaxy clusters are important tools for probing the cosmic large-scale structure evolution and for performing precision tests of cosmological models. The limiting factor for the application of clusters in such cosmological studies is currently the uncertainty in the relation between the observed X-ray luminosity (or temperature) and the cluster mass needed for the theoretical modeling. In view of the large efforts currently undertaken in X-ray cluster surveys and evolutionary studies (also using XMM extensively) it is crucial to pin down the cluster scaling relations at low z in a first step. Therefore we propose a comprehensive, detailed study of a representative cluster sample as an open, Legacy-type project to provide the community with the necessary data.
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