This section describes the eclipse recipes that are used in the ISAAC pipeline. The recipes have a variety of purposes, from recipes that take quality control data to recipes that produce reduced data. Not all recipes will be of direct interest to people wishing to reduce ISAAC data.
The principle purpose of these recipes is to produce and use calibration products that can be used to reduce ISAAC data. These recipes produce products such as flat fields, fits to slit curvature, wavelength calibration, etc.
|Recipes to produce calibrations and to do quality control|
|isaacp sw_spflat||Creates spectroscopic flat fields|
|isaacp sw_arc||Models the slit curvature|
|isaacp slitpos||Measures slit positions|
|isaacp sw_startrace||Models the trace of a star as a function of y|
|isaacp sw_respfunc||Measures the spectroscopic throughput|
|Recipes to reduce the data|
|isaacp sw_spjitter||Reduces ISAAC spectroscopic data|