400d cluster survey

CCCP

The primary motivation of the 400d survey was to select a complete sample of high-redshift clusters, observe them with Chandra, and use for cosmological studies. Hence CCCP — the Chandra Cluster Cosmology Project.

Note 12/15/08: This section will be gradualy populated in the next few months. We plan to post complete likelihood grids derived from the cluster data, primers on the Chandra data and cluster mass estimates, etc. Currently, only likelihood grids for a restricted set of models are provided. If you need specific information missing on this page, please contact Alexey Vikhlinin.

Cluster likelihoods for a set of cosmological models with free dark energy equation of states
Parameter constraints in combination with other cosmological data (Burenin & Vikhlinin 2012) + cosmomc module for cluster likelihoods