Other
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1317d&link_type=abstract
HST Proposal ID #1317
Other
Hst Proposal Id #1317
Scientific paper
A test will be performed to determine if there is any offset in the wavelength scales between internal and external calibration sources. Any derived offsets can be applied to the polynomial fit of pixel number versus wavelength determined from the lines in the internal Pt-Ne lamp. Unresolved lines in a dMe star will be used to determine the FOS + ST Line Spread Function. This program has a low priority compared with other SV activities.
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