GHRS Far UV Throughput with COSTAR Mirrors -- Cycle 6 Closeout

Details GHRS Far UV Throughput with COSTAR Mirrors -- Cycle 6 Closeout GHRS Far UV Throughput with COSTAR Mirrors -- Cycle 6 Closeout

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6896s&link_type=abstract

HST Proposal ID #6896

Physics

Optics

Hst Proposal Id #6896

Scientific paper

In order to determine if COSTAR is the sole cause of the loss
ofthroughput at the short-wavelength end of GHRS, we intend to makea
series of measurements of 2 stars just before and just afterthe removal
of the GHRS COSTAR mirrors. There may also beimplications for the
primary optics of HST.

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