MUSE Pipeline Reference Manual  1.0.2
Data Fields
muse_sky_master Struct Reference

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.
 

Detailed Description

Structure to hold the MASTER SKY result.

This structure contains the resulting MASTER SKY parameters.

Definition at line 57 of file muse_sky.h.

Field Documentation

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().


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