MUSE Pipeline Reference Manual
1.0.2
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Structure to hold the MASTER SKY result. More...
#include <muse_sky.h>
Data Fields | |
cpl_table * | lines |
Table of Atmospheric emission lines and their intensities. More... | |
cpl_table * | continuum |
Continuum flux table | |
muse_lsf_params ** | lsf |
LSF parameter for the resampled spectrum. | |
Structure to hold the MASTER SKY result.
This structure contains the resulting MASTER SKY parameters.
Definition at line 57 of file muse_sky.h.
cpl_table* muse_sky_master::lines |
Table of Atmospheric emission lines and their intensities.
This type of file contains one or more binary tables with the relative fluxes on the sky emission lines. If both tables are present, they are merged, so that lines should not appear in both tables.
Columns:
name
': Line name [string]group
': Line group id [int]lambda
': Air wavelength [double]flux
': Line flux [double]dq
': Quality of the entry (>0: dont use) [int] Definition at line 61 of file muse_sky.h.
Referenced by muse_postproc_process_exposure(), muse_sky_master_delete(), muse_sky_master_fit(), muse_sky_master_load(), and muse_sky_subtract_pixtable().