MUSE Pipeline Reference Manual  2.1.1
Data Fields
muse_scipost_make_cube_params_s Struct Reference

Structure to hold the parameters of the muse_scipost_make_cube recipe. More...

#include <muse_scipost_make_cube_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).
 
int resample
 The resampling technique to use for the final output cube.
 
const char * resample_s
 The resampling technique to use for the final output cube. (as string)
 
double dx
 Horizontal step size for resampling (in arcsec or pixel). The following defaults are taken when this value is set to 0.0: 0.2'' for WFM, 0.075'' for NFM, 1.0 if data is in pixel units.
 
double dy
 Vertical step size for resampling (in arcsec or pixel). The following defaults are taken when this value is set to 0.0: 0.2'' for WFM, 0.075'' for NFM, 1.0 if data is in pixel units.
 
double dlambda
 Wavelength step size (in Angstrom). Natural instrument sampling is used, if this is 0.0.
 
int crtype
 Type of statistics used for detection of cosmic rays during final resampling. "iraf" uses the variance information, "mean" uses standard (mean/stdev) statistics, "median" uses median and the median median of the absolute median deviation.
 
const char * crtype_s
 Type of statistics used for detection of cosmic rays during final resampling. "iraf" uses the variance information, "mean" uses standard (mean/stdev) statistics, "median" uses median and the median median of the absolute median deviation. (as string)
 
double crsigma
 Sigma rejection factor to use for cosmic ray rejection during final resampling. A zero or negative value switches cosmic ray rejection off.
 
double rc
 Critical radius for the "renka" resampling method.
 
const char * pixfrac
 Pixel down-scaling factor for the "drizzle" resampling method. Up to three, comma-separated, floating-point values can be given. If only one value is given, it applies to all dimensions, two values are interpreted as spatial and spectral direction, respectively, while three are taken as horizontal, vertical, and spectral.
 
int ld
 Number of adjacent pixels to take into account during resampling in all three directions (loop distance); this affects all resampling methods except "nearest".
 
int format
 Type of output file format, "Cube" is a standard FITS cube with NAXIS=3 and multiple extensions (for data and variance). The extended "x" formats include the reconstructed image(s) in FITS image extensions within the same file.
 
const char * format_s
 Type of output file format, "Cube" is a standard FITS cube with NAXIS=3 and multiple extensions (for data and variance). The extended "x" formats include the reconstructed image(s) in FITS image extensions within the same file. (as string)
 
int stacked
 If true, write an additional output file in form of a 2D stacked image (x direction is pseudo-spatial, y direction is wavelength).
 
const char * filter
 The filter name(s) to be used for the output field-of-view image. Each name has to correspond to an EXTNAME in an extension of the FILTER_LIST file. If an unsupported filter name is given, creation of the respective image is omitted. If multiple filter names are given, they have to be comma separated.
 

Detailed Description

Structure to hold the parameters of the muse_scipost_make_cube 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_make_cube_z.h.


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