A Coordinated XMM, SZE and Optical Survey for Galaxy Cluster Cosmology

Details A Coordinated XMM, SZE and Optical Survey for Galaxy Cluster Cosmology A Coordinated XMM, SZE and Optical Survey for Galaxy Cluster Cosmology

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..137b&link_type=abstract

XMM-Newton Proposal ID #05545607

Mathematics

Logic

Cosmology, Extragalactic Deep Fields And Area Surveys, Sze Survey Fiel, Sze Survey Fiel, Sze Survey Fiel, Sze Survey Fiel, Sze Survey Fiel, Sze Survey Fiel, Sze Survey Fiel, Xmm-Newton Proposal Id #05545607

Scientific paper

We are currently witnessing the opening of a new survey window to the Universe through the first surveys for galaxy clusters using the Sunyaev-Zeldovich effect (SZE) contributing to the understanding of the nature of Dark Energy. In AO6 we have been granted observing time for a 6.3 sqdeg. survey to help in the understanding and calibration of these surveys in a region where the three major survey experiments have joint forces for an intercomparison of this new type of cosmological surveys. The first seven pointings have been conducted and analysed and found to be mostly unuseful due to large contamination by soft proton flares, for reasons explained in detail in the proposal. Here we request the reobservations of the fields lost to enable a timely analysis of the survey data.

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