Changeset 14620
- Timestamp:
- Aug 22, 2007, 3:09:54 PM (19 years ago)
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- 3 added
- 1 edited
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branches/eam_branch_20070817/psphot/doc/notes.txt
r10033 r14620 1 2 2007.08.17 3 4 I am working on a number of cleanup / fixes. I have made an overhaul 5 of the pmModel APIs, adding function pointers in the pmModel 6 structure to the class-specific utility functions (eg, 7 pmModel->modelFunc is the actual function which is evaluated). 8 9 TO DO: 10 11 * update pmSourceFitSet to be able to include more than one model 12 type (currently it assumes the sources are all, eg, PSFs). This is 13 now needed because the old implementation used the function lookups 14 which have been dropped. 15 16 * define a generic API set to handle 2D modelling of a scalar using 17 either polynomials (as the pmPSF code currently does) or an 18 image-based representation (as the psphot sky model currently 19 does). 20 21 The image-based representation can automatically step down from NxM 22 super pixels to a smaller number based on the density of 23 measurements. 24 25 Include ways to smooth and regularize the output result. 26 27 This mechanism can be applied to: psf parameters, aperture 28 residual, psf peak-to-flux variations, the psphot background 29 representation. 30 31 * generate and store the output radial profile for objects 32 33 * finish testing and incorportate the CR / EXT measurements 34 35 * adjustments to pixel center based on second derivatives : needed 36 for the sersic models. 37 38 * adjustments to pixel flux for extreme values (r ~ 0) : needed for 39 the sersic models. 40 41 * on psf stars : fall back on a Gaussian. 42 43 * OPTIMIZATIONS !! 44 45 * drop the model sky element : should only be in source->sky,dsky 46 47 2006.11.16 1 48 2 49 ensemble: … … 20 67 * solve for source amplitudes 21 68 * update models 22 23 2006.11.1624 69 25 70 * create psSparseBorder to solve matrix equations which have a large
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