FOC Neutral Density Filter Calibrations

Computer Science

Scientific paper

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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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