Changes between Version 8 and Version 9 of fullforce_SAStest2
- Timestamp:
- Mar 31, 2014, 2:14:07 PM (12 years ago)
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fullforce_SAStest2
v8 v9 5 5 6 6 There we presented plots that send to indicate that the full force results provided a much 7 better match to SDSS model fits than the psphotStack results for de Vaucouleurs models (dev model) There was some scepticism that7 better match to SDSS model fits than the psphotStack results for de Vaucouleurs models (dev model). There was some scepticism that 8 8 the difference was so great. In particular the validity of the [http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/attachment/wiki/fullforce_SAStest1/ddevrad_hist_comparison.jpg plot] 9 9 was doubted. 10 10 11 It turns out that this scepticism was justified. The ddevrad values for the stack photometry were incorrect (the difference in units between the sdss value (arcseconds) and the IPP values (pixels) was not accounted for. Upon further review wediscovered that the wrong stacks (label SAS.20130620) were used for that investigation rather than the SAS 32 stacks (label SAS.20130703).11 It turns out that this scepticism was justified. The ddevrad values for the stack photometry were incorrect. The difference in units between the sdss value (arcseconds) and the IPP values (0.25 arcsecond pixels) was not accounted for. Upon further review we also discovered that the wrong stacks (label SAS.20130620) were used for that investigation rather than the SAS 32 stacks (label SAS.20130703). 12 12 13 13 In order to examine the dev model results in more detail we re-ran the full force pipeline on a subset of the SAS skycells. To improve statistics we changed 14 the system to select ing only dev models for forced photometry rather than the usual method of choosing the best model. The skycells processed were near the center14 the system to select only dev models for forced photometry rather than the usual method of choosing the best of the 3 model fits. The skycells processed were near the center 15 15 of the SAS field: 332 < ra < 336, -3 < dec < 3. 16 16
