Morphological and Structural Study of the Galaxies in Distant Cluster CL1322.5+3028

Details Morphological and Structural Study of the Galaxies in Distant Cluster CL1322.5+3028 Morphological and Structural Study of the Galaxies in Distant Cluster CL1322.5+3028

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003hst..prop.9949s&link_type=abstract

HST Proposal ID #9949

Mathematics

Logic

Hst Proposal Id #9949 Galaxies

Scientific paper

This archival project is to perform a full structural, morphological and color analysis of the galaxies in distant cluster CL1322.5+3028 {z=0.75}. CL1322.5+3028 is an extremely rich, high blue fraction cluster in which we have recently obtained deep KPNO 4m data through the four color Stromgren filter system {uvby}. Comparison between WFPC2 images and ground-based photometry will enable us to compare the structural and morphological classification of cluster members with narrow band color classification. CL1322.5+3028 presents a unique target in that we have deep, wide coverage, multi- filter WFPC2 data combined with new, equivalent depth ground- based narrow band photometry. This will be direct comparison between the photometric and physical properties of both the blue and red populations in a rich cluster, a key test of galaxy evolution.

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