Completing multi-wavelength studies of the REFLEX-DXL sample

Details Completing multi-wavelength studies of the REFLEX-DXL sample Completing multi-wavelength studies of the REFLEX-DXL sample

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...86z&link_type=abstract

XMM-Newton Proposal ID #04022201

Mathematics

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Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxcj2011.3-5725, Xmm-Newton Proposal 04022201

Scientific paper

To use massive clusters as the most sensitive probes to study the evolution of cosmic structure and to test cosmological models, it is important to control the systematics of the mass--observable relations. To meet this requirements, we constructed a morphology-unbiased and volume-limited sample with a well defined flux limit, consisting of 14 distant X-ray luminous clusters in the REFLEX survey (the REFLEX-DXL sample). The sample was observed in AO1 and AO3. We published detailed studies of 13 clusters. However, the observations of RXCJ2011.3-5725 were seriously spoiled by flares. To complete the REFLEX-DXL sample to finish the multi-wavelength studies, we request a re-observation of 36 ks for RXCJ2011.3-5725.

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