double pixfrac
Pixel down-scaling factor for the "drizzle" resampling method.
const char * filter
The filter name(s) to be used for the output field-of-view image. Each name has to correspond to an E...
const char * resample_s
The resampling technique to use for the final output cube. (as string)
double crsigma
Sigma rejection factor to use for cosmic ray rejection during final resampling. A zero or negative va...
int ld
Number of adjacent pixels to take into account during resampling in all three directions (loop distan...
int format
Type of output file format, "Cube" is a standard FITS cube with NAXIS=3 and multiple extensions (for ...
double lambdamax
Cut off the data above this wavelength after loading the pixel table(s).
int stacked
If true, write an additional output file in form of a 2D stacked image (x direction is pseudo-spatial...
int resample
The resampling technique to use for the final output cube.
double dx
Horizontal step size for resampling (in arcsec or pixel). The following defaults are taken when this ...
double rc
Critical radius for the "renka" resampling method.
Structure to hold the parameters of the muse_scipost_make_cube recipe.
const char * crtype_s
Type of statistics used for detection of cosmic rays during final resampling. "iraf" uses the varianc...
double lambdamin
Cut off the data below this wavelength after loading the pixel table(s).
double dy
Vertical step size for resampling (in arcsec or pixel). The following defaults are taken when this va...
int crtype
Type of statistics used for detection of cosmic rays during final resampling. "iraf" uses the varianc...
double dlambda
Wavelength step size (in Angstrom). Natural instrument sampling is used, if this is 0...
struct muse_scipost_make_cube_params_s muse_scipost_make_cube_params_t
Structure to hold the parameters of the muse_scipost_make_cube recipe.
const char * format_s
Type of output file format, "Cube" is a standard FITS cube with NAXIS=3 and multiple extensions (for ...