| 211 | | * check if refcat oddities in field is a problem -- Eddie and Doug catalogs to compare to |
| 212 | | * new refcat astrometry and zeropoint verification tests -- the new refcat demonstrated large astrometry and zeropoint variations when previous config used |
| 213 | | * CNP tessellation check and exposure filling factor |
| 214 | | * MD as a targeted survey and utilized throughout the different processing needs to have a summary of exposures changed/lost in PV3 -- PV3 vs PV2 and original processing comparison in quality faults and astrometry/zeropoint variations is critical so events published in transients work is reproduced |
| 215 | | * background restore M31 and masking for M31/STS -- test samples to be run and verified for final version |
| | 213 | * check if refcat oddities in field is a problem -- Eddie and Doug catalogs to compare to (TBD) |
| | 214 | * new refcat astrometry and zeropoint verification tests -- the new refcat demonstrated large astrometry and zeropoint variations when previous config used -- final verification needed with full fields finished |
| | 215 | * CNP tessellation check and exposure filling factor -- done, need plots for notes wiki |
| | 216 | * MD as a targeted survey and utilized throughout the different processing needs to have a summary of exposures changed/lost in PV3 -- PV3 vs PV2 and original processing comparison in quality faults and astrometry/zeropoint variations is critical so events published in transients work is reproduced -- TBD before final night+ref stack and diffs done |
| | 217 | * background restore M31 and masking for M31/STS -- test samples to be run and verified for final version, on hold for now 1/2015 |
| 219 | | * night stack config, refstack edge loss -- see diffim for as well -- comparison to PV2 and earlier datasets |
| 220 | | * reference, deep stack input cuts -- need feedback on if 2009 and or early 2010 data is okay to use -- 2009 is not great data so not to be used, Jan/June 2010 is still under consideration if the baffle is critical or not. |
| | 221 | * night stack config, refstack edge loss -- see diffim for as well -- comparison to PV2 and earlier datasets -- TBD w/ final night+ref stacks |
| | 222 | * reference, deep stack input cuts -- need feedback on if 2009 and or early 2010 data is okay to use -- 2009 is not great data so not to be used, Jan/June 2010 seems okay (level of impact unknown) and has been used in deep stack |
| 223 | | * stack photometry sky oddities -- |
| 224 | | * check refcat oddities in the MD fields for skycal re-zeropointing |
| 225 | | * zeropt recalibration in skycal improvement and characterization (y-band at least may need own config) -- |
| 226 | | * evaluate test samples for CNP (M31,STS) -- equivalent stacks in available filters vs deeper in primary filter, single filter only for STS/M31 so no extended source fits? |
| | 225 | * stack photometry sky oddities -- |
| | 226 | * check refcat oddities in the MD fields for skycal re-zeropointing -- TBD |
| | 227 | * zeropt recalibration in skycal improvement and characterization (y-band at least may need own config) -- TBD |
| | 228 | * evaluate test samples for CNP (M31,STS) -- equivalent stacks in available filters vs deeper in primary filter, single filter only for STS/M31 so no extended source fits? -- TBD |
| 228 | | * verify similar photometry to previous reductions -- |
| 229 | | * verify similar detections/coverage (no sig loss on edges) -- a key point for reference stack creation above |
| 230 | | * evaluate test samples for CNP (M31,STS) -- |
| 231 | | * full-forced photometry -- unknown, untested still for any MD type field |
| | 230 | * verify similar photometry to previous reductions -- TBD |
| | 231 | * verify similar detections/coverage (no sig loss on edges) -- a key point for reference stack creation above -- TBD |
| | 232 | * evaluate test samples for CNP (M31,STS) -- TBD |
| | 233 | * full-forced photometry -- unknown, untested still for any MD type field -- TBD |
