Fos-Ov 110/111 Aperture Locations - Phase Iiib Fine Positions

Details Fos-Ov 110/111 Aperture Locations - Phase Iiib Fine Positions Fos-Ov 110/111 Aperture Locations - Phase Iiib Fine Positions

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1444h&link_type=abstract

HST Proposal ID #1444

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Hst Proposal Id #1444

Scientific paper

Phase IIIb The goal is to measure the aperture locations and sizes in 4 phases as described in detail in "Aperture Locations and Sizes for the Space Telescope Science Instruments" by O. Lupie, R. Bohlin, and A. Holm. Another goal is obtaining the first spectra of an external object for each FOS detector system. This program has the highest priority. Phases I to III must be completed before attempting observations of any other stellar targets. This program will result in a data base change to the table of aperture location matrices: YXFMTRIX-A and -B.

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