The ultimate XMM extragalactic survey [b]

Physics

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Cosmology, Extragalactic Deep Fields And Area Surveys, Cfhtls-W1

Scientific paper

We propose a 10-40ks/field XMM survey over 50 deg2, designed to constrain the dark energy equation of state using the 600 - 1,400 clusters of galaxies that we will detect. The constraints that we will achieve on w_0 and w_a, of 0.7 and 2.4 (10ks coverage) and 0.4 and 1.2 (40ks coverage) are at the level of the ultimate Stage-IV DETF accuracy estimates achievable by cluster studies. This survey will also have lasting legacy value for cluster scaling laws and studies of AGN and XRB.

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