24 #ifndef MUSE_CREATE_SKY_Z_H
25 #define MUSE_CREATE_SKY_Z_H
31 #include <muse_instrument.h>
75 #define MUSE_CREATE_SKY_PARAM_CR_NONE 1
76 #define MUSE_CREATE_SKY_PARAM_CR_CUBE 2
77 #define MUSE_CREATE_SKY_PARAM_CR_SPECTRUM 3
78 #define MUSE_CREATE_SKY_PARAM_CR_INVALID_VALUE -1
struct muse_create_sky_params_s muse_create_sky_params_t
Structure to hold the parameters of the muse_create_sky recipe.
double csampling
Spectral sampling of the continuum spectrum [Angstrom].
int cr
Type of cosmic ray cleaning to use. "Cube" is the standard CR cleaning which works on a datacube...
double lambdamin
Cut off the data below this wavelength after loading the pixel table(s).
double sampling
Spectral sampling of the sky spectrum [Angstrom].
double fraction
Fraction of the image to be considered as sky. If an input sky mask is provided, the fraction is appl...
double lambdamax
Cut off the data above this wavelength after loading the pixel table(s).
double lambdaref
Reference wavelength used for correction of differential atmospheric refraction. The R-band (peak wav...
const char * cr_s
Type of cosmic ray cleaning to use. "Cube" is the standard CR cleaning which works on a datacube...
Structure to hold the parameters of the muse_create_sky recipe.