Towards Precision Cosmology With Optically Selected Cluster Catalogs

Mathematics – Logic

Scientific paper

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Scientific paper

Precision cosmology with galaxy clusters requires that: a- the cluster selection function be well undestood. b- the relation between cluster mass and the cluster observable used to trace mass be completely characterized. Indeed, all current cluster cosmological constraints are systematics limited by one or both of these requirements. Given the unparalled statistical precision that near future cluster catalogs can achieve, succesfully resolving these difficulties is now more urgent than ever. In this talk, we review ongoing work aimed at addressing these problems within the context of optical cluster cosmology, focusing particularly on where we are now and what remains to be done.

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