Deep Photometry of the Globular Cluster M92

Details Deep Photometry of the Globular Cluster M92 Deep Photometry of the Globular Cluster M92

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6257k&link_type=abstract

HST Proposal ID #6257

Physics

Hst Proposal Id #6257 Stellar Populations

Scientific paper

A faint color-magnitude diagram and luminosity function will be
determined for the globular cluster M92 (NGC 6341). The FOC will
observe fields in B and V, at the center and 20'' out, while WFPC2
observes (on the same field at all times) in V and I. The WFPC2 field
will reach at least to V = 26.

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