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Reinhold
This algorithm was developed by Kim Reinhold whilst working at the Joint
Astronomy Centre in Hilo, Hawaii. Its overall strategy is first to
identify pixels within the data array which mark the edges of clumps of
emission. This typically produces a set of rings (in 2D), or shells (in 3D),
outlining the clumps. However, these structures can be badly affected by
noise in the data and so need to be cleaned up. This is done using a
sequence of cellular automata which first dilate the rings or shells, and
the erodes them. After cleaning, all pixels within each ring or shell
are assumed to belong to a single clump.
Subsections
Next: Identifying the Clump Edges
Up: Clump Identification Algorithms
Previous: Comparing CUPID ClumpFind with other Implementations
CUPID
Starlink User Note 255
D.S. Berry
19th March 2008
E-mail:ussc@star.rl.ac.uk
Copyright © 2008 Science and Technology Facilities Council