FOC F/48 Long Slit - Calibration

Physics

Scientific paper

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Hst Proposal Id #1513

Scientific paper

The aim of this SV task is to determine the wavelength calibration of the spectrograph using an external source, namely a planetary nebula. There is no internal wavelength calibration for the spectrograph. Although there is only time in SV to do this task once, it must be repeated during cycle 2 and later. Both echelle and filter modes will be studied. The resulting data will be used to update the SOGS RSDP files for routine processing of FOC images.

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