MUSE Pipeline Reference Manual  2.1.1
Data Structures | Typedefs
Recipe muse_astrometry: Compute an astrometric solution.

Data Structures

struct  muse_astrometry_params_s
 Structure to hold the parameters of the muse_astrometry recipe. More...
 

Typedefs

typedef struct muse_astrometry_params_s muse_astrometry_params_t
 Structure to hold the parameters of the muse_astrometry recipe. More...
 

Detailed Description

Author
Peter Weilbacher
  Merge pixel tables from all IFUs, apply correction for differential
  atmospheric refraction, optionally apply flux calibration and telluric
  correction (if the necessary input data was given), and resample the
  data from all exposures into a datacube. Use the cube to detect objects
  which are then matched to their reference positions from which a
  two-dimensional WCS solution is computed.

  The main output is the ASTROMETRY_WCS file which is a bare FITS header
  containing the world coordinate solution.
  The secondary product is DATACUBE_ASTROMETRY, it is not needed for
  further processing but can be used for verification and debugging. It
  contains the reconstructed cube and two images created from it in
  further FITS extensions: a white-light image and the special image
  created from the central planes of the cube used to detect and centroid
  the stars (as well as its variance).

Typedef Documentation

Structure to hold the parameters of the muse_astrometry recipe.

This structure contains the parameters for the recipe that may be set on the command line, in the configuration, or through the environment.