Computer Science
Scientific paper
Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6292b&link_type=abstract
HST Proposal ID #6292
Computer Science
Hst Proposal Id #6292 Cool Stars
Scientific paper
As part of the SV program of HSP HD 60435 was observed with the HSP as a test of the photometric stability of the HSP. This program was successful in identifying many of the photometric stability problems which had to be dealt with in later HSP observations. However, it also yielded some interesting scientfic results which will followed up. The primary results of the HSP data were the detection of both known and previously unknown pulsations in the star. In addition significant low frequency features are evident in the power spectrum of the star which have not been accounted for as either noise or instrument effects. Further observations of this star will be accomplished with the FOS in RAPID mode for an observation duration of about 6 hours while the target is in the CVZ of the HST.
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