MUSE Pipeline Reference Manual
2.1.1
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Structure to hold the parameters of the muse_scipost_correct_dar recipe. More...
#include <muse_scipost_correct_dar_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). | |
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. | |
int | darcheck |
Carry out a check of the theoretical DAR correction using source centroiding. If "correct" it will also apply an empirical correction. | |
const char * | darcheck_s |
Carry out a check of the theoretical DAR correction using source centroiding. If "correct" it will also apply an empirical correction. (as string) | |
Structure to hold the parameters of the muse_scipost_correct_dar 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_correct_dar_z.h.