| | 1 | PSNSC.wref.20170707 notes (draft) |
| | 2 | |
| | 3 | best input stack limited to 40 inputs max -- |
| | 4 | * label PSNSC.wref.20170707, data_group PSNSC.wref.20170707h##, PSNSC.wref.20170707h##q2 |
| | 5 | * q2 (2nd level quality, poorer), may also be a q3 for lower quality |
| | 6 | * data_group may also be LAP.PV3W or other included previously processed stacks |
| | 7 | |
| | 8 | transition band -- DEC -25 to -35 -- processed last to generate stacks without a mix of ubercal and synthetic photometry calibration (when possible) |
| | 9 | |
| | 10 | LAP.PV3W.20150312 -- will use by default for RA~8-16 -- will need to check/replace bad stacks and stacks with good_frac<0.9 (~15k) |
| | 11 | |
| | 12 | cleanup of warps to proceed as regions complete to basically try to swap space for space so that stacks are distributed across data nodes (however most warps live on ipp100-104,118-122) -- therefore used ipp054-097 with space as direct targets rather than nightly processing |
| | 13 | |
| | 14 | future stack updates/reprocessing -- as RA slice of 1-2hr sets, a improved stacks will be made -- criteria like good_frac<0.95, q2 check, Nin increase of some relative percent (TBD) |
| | 15 | |
| | 16 | |
| | 17 | MOPS vs QUB WSdiff with w-band stacks -- moving versus stationary transients -- priority MOPS, QUB, other |
| | 18 | * spatial coverage key for MOPS as most detections on sky pixels as long as diffs can be made well |
| | 19 | * MOPS not limited by stack updates, QUB needs updates only during set season (avoid using inputs with events and changing mean levels) |
