LBDS 53W091: a Cluster of Old, Red Galaxies

Details LBDS 53W091: a Cluster of Old, Red Galaxies LBDS 53W091: a Cluster of Old, Red Galaxies

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7174s&link_type=abstract

HST Proposal ID #7174

Mathematics

Logic

Hst Proposal Id #7174

Scientific paper

This distant cluster or group of red E {z=1.55} are representative of the oldest stellar systems we can glimpse at their "middle age"; we are interested in their morphologies. One prospect with NICMOS observations is to simultaneously measure the passive evolutionary brightening and the cosmological Tolman {1+z}^-4 surface brightness changes compared to relatively nearby E clusters. In addition to the NICMOS IDT members, the collaborators on this investigation are Arjun Dey {KPNO}, Andrew Bunker, Daniel Stern {UC Berkeley}, James Dunlop, John Peacock, Raul Jimenez {Edinburgh}, Mark Dickinson {STScI} and Rogier Windhorst {Arizona State University}.

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