Morphology of Distant Galaxies - Cycle 4 Carry-Over

Details Morphology of Distant Galaxies - Cycle 4 Carry-Over Morphology of Distant Galaxies - Cycle 4 Carry-Over

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5706k&link_type=abstract

HST Proposal ID #5706

Physics

Hst Proposal Id #5706 Galaxies &Amp, Clusters Faint Galaxies

Scientific paper

This is a Cycle 4 carryover from GTO 3685 to study the morphology of distant galaxies, a field that has lagged far behind what has been learned from spectroscopic work. The targeted galaxies all have been extensively observed from the ground. Nearly all are in the redshift range 0.24-0.65. Ground-based data include broad-baseline 4-color photometry and, in nearly all cases, redshifts. The target fields each have numerous galaxies that have been richly observed from the ground. Each field will be observed with the WFPC-2, with orientation optimized to include as many galaxies as possible while avoiding bright stars. These observations will continue our ongoing investigation into the morphology of the rich sample of medium-redshift galaxies in the Koo-Kron redshift surveys.

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