- Timestamp:
- Mar 24, 2010, 4:56:11 PM (16 years ago)
- File:
-
- 1 edited
Legend:
- Unmodified
- Added
- Removed
-
branches/eam_branches/20100225/psphot/doc/notes.20100131.txt
r26894 r27440 1 2 2010.03.24 3 4 I have finished another iteration on source size analysis. I feel 5 fairly confident of the extended source and CR identifications. They 6 are not perfect, but they are in pretty good shape. The CR IDs use 7 the moments to find things smaller in one dimension than a PSF, while 8 the EXT is set for things larger than a PSF in one dimention. 9 10 There still seems to be some trouble with SATSTARS : these are being 11 set for sources which are fainter than the SAT limit -- I'm not sure 12 if this is due to the quality of the PSF fit or if they really are 13 SAT, but have integrated fluxes lower than expected (underfitted in 14 PSF). 1 15 2 16 20100131
Note:
See TracChangeset
for help on using the changeset viewer.
