MUSE Pipeline Reference Manual  2.1.1
Data Fields
muse_scipost_subtract_sky_params_s Struct Reference

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.
 

Detailed Description

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.


The documentation for this struct was generated from the following file: