Disentangling the Influence of Cosmological Parameters and Structure Formation in the Universe with Distant Clusters of

Details Disentangling the Influence of Cosmological Parameters and Structure Formation in the Universe with Distant Clusters of Disentangling the Influence of Cosmological Parameters and Structure Formation in the Universe with Distant Clusters of

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1303u&link_type=abstract

Chandra Proposal ID #04800149

Mathematics

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Chandra Proposal Id #04800149

Scientific paper

The detection and study of distant clusters with redshifts beyond unity is very important to study cluster evolution, which is strongly linked to structure formation and cosmological parameters. In a search for distant clusters in ROSAT PSPC pointings we recently found two very promising high redshift cluster candidates with estimated redshifts between z = 1.2--1.7 and corresponding bolometric X-ray luminosities of about 1E45 erg/sec. We propose to observe these two candidates with Chandra and XMM-Newton to determine their form, temperature and redshift, which will allow us to disentangle the interplay between cosmological parameters and structure formation.

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