Faint Clusters of Galaxies (WC09)

Details Faint Clusters of Galaxies (WC09) Faint Clusters of Galaxies (WC09)

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5102w&link_type=abstract

HST Proposal ID #5102

Mathematics

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Hst Proposal Id #5102

Scientific paper

Three distant clusters of galaxies, with redshifts from 0.70 to 0.92, will be imaged in two colors corresponding to rest wavelengths of about 3400 and 4500 angstroms. The primary object of the study is to investigate the color and morphological evolution of cluster galaxies. Sufficient signal-to-noise will be obtained for all objects to see spiral structure, if present, and all fields contain starburst galaxies, whose morphology is of special interest. In addition, the data will yield structural parameters for the bright cluster galaxiess, which will aid in interpreting the classical Hubble diagram for the determination of the deceleration parameter.

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