Other
Scientific paper
Jul 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1281k&link_type=abstract
HST Proposal ID #1281
Other
Hst Proposal Id #1281
Scientific paper
With 1500 sec in each of U, B, and V, at f/96, we will easily reach the main-sequence turnoff in the central bulge of the Milky Way, taking advantage of the low absorption in Baade's Window. FOC resolving power is adequate to separate stars down to the limited magnitude of ST. A by-product of another program will be a pair of V and I parallel WFC exposures, overlapping the same field.
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