HST Imaging of Ground-Based Ultra-Deep Survey Fields

Details HST Imaging of Ground-Based Ultra-Deep Survey Fields HST Imaging of Ground-Based Ultra-Deep Survey Fields

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.2365l&link_type=abstract

HST Proposal ID #2365

Computer Science

Hst Proposal Id #2365

Scientific paper

A deep ground based multi-color survey of several small areas of sky is being used to search for young galaxies in order to study galaxy formation and early evolution. Extremely deep images in five colors spread between the ultraviolet atmospheric cut-off at 3200 A and the thermal infrared at 2.4 micron have been obtained, and spectroscopic redshifts obtained for almost all of the galaxies with B < 24 and I < 22.5. The aim of this proposal is to use the FOC to obtain complementary deep images at a wavelength of 2200 A. This will enable us to degine the spectral energy distributions of these galaxies over a full decade of wavelength. This project representa a fundamental attempt to study the Universe at faint ultraviolet wavelengths.

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