Spectroscopy: Data Reduction Recipes

The following tables describe the UIST spectroscopy ORACDR recipes; click on the recipe name for more information. The Requirements listed below are frames that should be obtained prior to use of the recipe, although data can always be re-reduced when the appropriate frames have been taken. Flats and standard stars must be obtained through the same grism and slit.

There are versions of these recipes which reduce a standard star sequence; these data are then filed for use with the target observations (see e.g. STANDARD_STAR)