A Deep Survey at High Galactic Latitudes (WC06): Cycle 4

Details A Deep Survey at High Galactic Latitudes (WC06): Cycle 4 A Deep Survey at High Galactic Latitudes (WC06): Cycle 4

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5109w&link_type=abstract

HST Proposal ID #5109

Physics

Hst Proposal Id #5109 Galaxies &Amp, Clusters

Scientific paper

Very deep exposures will be taken in broadband V and I colors in each of two fields at high galactic and ecliptic latitudes, in order to observe objects as faint as possible. Twelve exposures should yield S/N of about 4 at magnitude 29.5 for neutral-colored point sources. The data will be used for counts and morphology of faint and distant galaxies and to study the distribution and luminosity function of galactic stars to very faint levels.

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