MUSE Pipeline Reference Manual
2.1.1
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Structure to hold the parameters of the muse_scipost_subtract_sky recipe. More...
#include <muse_scipost_subtract_sky_z.h>
Data Fields | |
double | lambdamin |
Cut off the data below this wavelength after loading the pixel table(s). | |
double | lambdamax |
Cut off the data above this wavelength after loading the pixel table(s). | |
const char * | orig |
If specified, write an additional column containing the original data to the pixel table. | |
double | flux_sky |
Reference flat field flux, obtained by sky exposure. This parameter is needed to scale the data of each pixel table if more than one pixel table was used to determine the sky. By default, it is taken from the parameter ESO DRS MUSE FLAT FLUX SKY of the first pixel table. | |
double | flux_lamp |
Reference flat field flux, obtained by lamp exposure. This parameter is needed to scale the data of each pixel table if more than one pixel table was used to determine the sky. By default, it is taken from the parameter ESO DRS MUSE FLAT FLUX LAMP of the first pixel table. | |
Structure to hold the parameters of the muse_scipost_subtract_sky recipe.
This structure contains the parameters for the recipe that may be set on the command line, in the configuration, or through the environment.
Definition at line 48 of file muse_scipost_subtract_sky_z.h.