MUSE Pipeline Reference Manual
1.0.2
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Structure to hold the parameters of the muse_create_sky recipe. More...
#include <muse_create_sky_z.h>
Data Fields | |
double | fraction |
Fraction of the image to be considered as sky. If an input sky mask is provided, the fraction is applied to the regions within the mask. If the whole sky mask should be used, set this parameter to 1. | |
double | sampling |
Spectral sampling of the sky spectrum [Angstrom]. | |
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, "spectrum" uses sigma clipping on the spectrum. | |
const char * | cr_s |
Type of cosmic ray cleaning to use. "Cube" is the standard CR cleaning which works on a datacube, "spectrum" uses sigma clipping on the spectrum. (as string) | |
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). | |
double | lambdaref |
Reference wavelength used for correction of differential atmospheric refraction. The R-band (peak wavelength ~7000 Angstrom) that is usually used for guiding, is close to the central wavelength of MUSE, so a value of 7000.0 Angstrom should be used if nothing else is known. A value less than zero switches DAR correction off. | |
Structure to hold the parameters of the muse_create_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_create_sky_z.h.