| 7 | | * various changes to psphotstack (Gene/Bill know more) |
| 8 | | * various changes to dvo related stuff (Gene knows more, here's what heather remembers of the top of her head) |
| 9 | | * best qf_perfect, best sg_sep for dvo averages |
| 10 | | * does the right thing for nx=0 - mags are null |
| 11 | | * nframes has been fixed, now reports the correct value |
| 12 | | * nigel's "goofy mags" due to dvo having duplicates - should be fixed both in dvo and in ipptopsps |
| 13 | | |
| | 7 | * best qf_perfect, best sg_sep reported for dvo averages |
| | 8 | * does the right thing for nx=0 - mags are null |
| | 9 | * nigel's "goofy mags" due to dvo having duplicates - should be fixed both in dvo and in ipptopsps |
| | 10 | * Better modeling and subtraction of flux from very bright stars (subtract a smoothed radial profile) -- reduces number of false detections |
| | 11 | * do not allow negative fluxes for real detected objects in linear flux fit - improves measurements of nearby sources |
| | 12 | * use a mask to prevent detections on 2nd pass within 1" of detections from 1st pass |
| | 13 | * Changes to psphotStack object matching- reduces spurious sources |
| | 14 | * Require object be detected in 2 bands before creating sources for forced photometry (matched sources)... |
| | 15 | * ... Except if only detection is in y band perform forced photometry in |
| | 16 | all bands. |
| | 17 | * Drop matched sources for which aperture flux is not finite (This usually |
| | 18 | happens when the pixels in the matched band are totally masked) |
| | 19 | * Insure that NAN pixels in image and variance images are masked. This avoids several crashes that prevented some static sky analysis from completing for some skycells. |
| | 20 | * Better error handling in Kron radius measurements. This reduces spurious large values. |
| | 21 | * When psf matching fails for an input continue with the psphotStack analysis skipping the radial aperture measurements for the matched images in that band. |
| | 22 | * Perform psphotStack even if stacks are available for less than five filters in a given skycell. |
| | 23 | * Fix N_FRAMES measurement which was getting lost in the skycell calibration process. |
| | 24 | * In DVO correct an error in zero point application to the object level flux measurments |
