Builds a score map for compact structures whose photometric SEDs differ from the local surrounding galaxy light. The score combines a local-contrast term from a collapsed image with a local SED-anomaly term measured relative to a smoothed version of the cube.
Usage
compute_clump_score(
input,
support = NULL,
bands = NULL,
contrast_weight = 0.5,
sed_weight = 0.5,
small_sigma = 0.7,
large_sigma = 4
)Arguments
- input
3-D array or FITS-like list with
imDat.- support
Optional logical foreground support mask. If
NULL, all finite pixels in the collapsed image are used.- bands
Bands used to build the score.
NULLuses all bands.- contrast_weight
Weight assigned to the local-contrast term.
- sed_weight
Weight assigned to the local SED-anomaly term.
- small_sigma
Gaussian smoothing scale for the compact image term.
- large_sigma
Gaussian smoothing scale for the local-background term.