GHRS Bright Star Target Acquisition After the Side 1 Loss

Details GHRS Bright Star Target Acquisition After the Side 1 Loss GHRS Bright Star Target Acquisition After the Side 1 Loss

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ghrs.rept...37g&link_type=abstract

GHRS Instrument Science Report 037, 4 pages

Physics

Hubble Space Telescope, Hst, Space Telescope Science Institute, Goddard High Resolution Spectrograph, Ghrs

Scientific paper

With both Sides 1 and 2 available on GHRS there were no stars too bright for routine target acquisition. Furthermore, there were no stars too bright for spectroscopy with any of the several modes on GHRS. The very brightest stars would have been acquired with the attenuated mirror on Side 1 (A1) even if the spectral observations were to use only Side 2 elements. In Cycle 1 there are several GO and GTO proposals that request acquisitions of stars that are nominally too bright for the Side 2 attenuated mirror (A2).

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