The Deep Ultraviolet Sky

Details The Deep Ultraviolet Sky The Deep Ultraviolet Sky

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3543l&link_type=abstract

HST Proposal ID #3543

Computer Science

Hst Proposal Id #3543

Scientific paper

It is proposed to obtain deep images of the extragalactic sky using the FOC on HST. These will reach a limiting magnitude of about 27.0 on the AB system and will complement existing ground-based data that reaches a comparable depth in the optical U, B, V and I bands and in the infrared K band. These data will thus extend our photo-metric survey to a full decade of wavelength. The data will define (a) where and at what rate star-formation is occuring in the Universe at redshifts around z = 0.5 and (b) will define the spectral energy distributions and hence constrain the redshifts of the population of very blue "flat-spectrum" galaxies. We propose to observe one more ground-based survey fields to complement our Cycle 1 program 2365 which is obtaining similar data on the first two of our survey fields.

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