Computer Science
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6930j&link_type=abstract
HST Proposal ID #6930
Computer Science
Hst Proposal Id #6930
Scientific paper
The principle objective is to monitor the determine throughputs of the neutral density filters, especially F4ND and F6ND. Observations of the core of NGC5139 will provide a wide-range of magnitudes and a large number of stars for the analysis, along with direct comparison with previous calibrations done at different wavelengths. Images of R136A are necessary in order to obtain high enough S/N observations in the UV, and also to check the higher ND filters {ie, F6ND, and F8ND}.
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