Changes between Version 240 and Version 241 of Processing
- Timestamp:
- Apr 19, 2019, 1:01:39 PM (7 years ago)
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Processing
v240 v241 22 22 MOPS -- [wiki:PSNSC_MOPS] -- OSS,ESS,MSS processed through publishing, processed throughout the night and finished by early morning 23 23 * summary for czaring -- 24 * OSS, ESS, MSS , EU chip->warp, WWdiff, publishing -- time critical, problems and requested alternative diffims must be addressed ASAP (early morning)25 * targeted FSS.* chip->warp, WSdiff, publishing -- time critical, faults must be cleared ASAP (early morning)26 27 QUB -- [wiki:PSST_QUB] (should have been labeled PSNSC_PSST_QUB) 24 * OSS, ESS, MSS and EU, XSS, Bright.nightlyscience: chip->warp, WWdiff, publishing -- time critical, problems and requested alternative diffims must be addressed ASAP (must be fully finished early morning) 25 * FSS.* targeted chip->warp, WSdiff, publishing -- time critical, faults must be cleared ASAP (must be finished early morning) 26 27 QUB -- [wiki:PSST_QUB] (should have been labeled PSNSC_PSST_QUB) -- MEH taking care of until further notice (201904xx) 28 28 * summary for czaring -- 29 29 * xSS WSdiff catalog products for PSST -- moderately time critical, faults must be cleared by end of day (WS queuing done by MEH) … … 31 31 * QUB.* stack, WSdiff, SSdiff manually dealt with by Mark Huber 32 32 33 SNIaF -- [wiki:PSST_SNIaF] -- (should have been labeled PSNSC_SNIaF) 33 SNIaF -- [wiki:PSST_SNIaF] -- (should have been labeled PSNSC_SNIaF) -- MEH taking care of until further notice (201904xx) 34 34 * summary for czaring -- processing chip->warp, WSdiff, but only warp images distributed -- time critical, faults must be cleared before noon (ended 201808xx) 35 35 36 CFA -- [wiki:CFA_MD07] -- (should have been labeled PSNSC_CFA_MD07) 36 CFA -- [wiki:CFA_MD07] -- (should have been labeled PSNSC_CFA_MD07) -- MEH taking care of until further notice (201904xx) 37 37 * summary for czaring -- processing chip->warp, nightly stack, WS+SSdiff but not distributed yet -- not time critical, but faults should be cleared before cleanup.. 38 38 39 NCU -- [wiki:PSNSC_NCU] -- NCU 39 NCU -- [wiki:PSNSC_NCU] -- NCU -- none planned currently, MEH taking care of until further notice (201904xx) 40 40 * summary for czaring (Mark Huber responsible for currently 20161026) -- NCU.nightlyscience chip->warp, WSdiffs, publishing for MOPS -- time critical, faults must be cleared ASAP (early morning) for MOPS 41 41 * nightly stack, SSdiffs -- TBD 42 42 43 K2 -- similar to SNIaF and 3PI (3PI needs to be documented still) -- setup still in progress by MEH43 K2 -- similar to SNIaF and 3PI (3PI needs to be documented still) -- none planned currenently -- MEH taking care of until further notice (201904xx) 44 44 * summary for czaring -- processing chip->warp, WSdiff with only diff cmf distributed to QUB -- fairly time critical like SNIaF, faults must be cleared before noon (WS queuing done by MEH) 45 45 46 46 Bright -- observations done in twilight and bright full moon time (fully replaces ThreePi observations now except for occasional filler fields) -- setup ongoing progress by MEH 47 * summary for czaring -- processing chip->warp, WWdiff for MOPS, WSdiff with only diff cmf distributed to QUB -- time critical, faults must be cleared ASAP (early morning) for MOPS, QUB (WW, WS queuing done by MEH) 47 * summary for czaring -- processing chip->warp, WWdiff for MOPS 48 * WSdiff with only diff cmf distributed to QUB -- time critical, faults must be cleared ASAP (early morning) QUB 49 * BrightTwi and Bright3Pi only WSdiffs to QUB, split to avoid messing up WWdiff sets during full moon 48 50 * details on https://ps1wiki.ifa.hawaii.edu/trac/wiki/EuclidObservations 49 51
