Faint Clusters of Galaxies (WC09): Cycle 5

Details Faint Clusters of Galaxies (WC09): Cycle 5 Faint Clusters of Galaxies (WC09): Cycle 5

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6278w&link_type=abstract

HST Proposal ID #6278

Mathematics

Logic

Hst Proposal Id #6278 Galaxies &Amp, Clusters

Scientific paper

A distant clusters of galaxies, with redshifts from 0.70 to 0.92, willbe imaged in two colors corresponding to rest wavelengths of about 3400 and4500 angstroms. The primary object of the study is to investigate the colorand morphological evolution of cluster galaxies. Sufficient signal-to-noisewill be obtained for all objects to see spiral structure, if present, and thisfield contains starburst galaxies, whose morphology is of special interest.In addition, the data will yield structural parameters for the bright clustergalaxies, which will aid in interpreting the classical Hubble diagram forthe determination of the deceleration parameter.

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