Changes between Version 29 and Version 30 of PSNSC_NCU
- Timestamp:
- Oct 26, 2016, 12:15:00 AM (10 years ago)
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PSNSC_NCU
v29 v30 108 108 * WSdiff runs in ~ippmops/stdscience_ws with modified ipp-20141024 ops tag to make uncompressed WSdiffs (like FSS, PSNSC_MOPS) 109 109 * larger volume, may need more nodes -- must be uncompressed for MOPS stamps since large data volume 110 * default detection @5-sigma while WWdiff is <5-sigma and may need to be adjusted -- default plan will be at normal 5-sigma level unless tuning agreed upon to a lower level (test chunk to be evaluated for this still) -- MD not a great equal comparison since exptimes were longer (but was also 5-sigma) 111 112 * [[html(<span style="color:red">[sc] Not sure if the catalog size is not going to explode if threshold too small. WWdiff is at 2.5-sigma(not sure?). What was the value for WSdiffs e.g. MDs? We could use the values (in each rgiz) unless something has changed. Not sure about what's used for w-band.</span>)]] 110 * default detection @5-sigma while WWdiff is <5-sigma (3.5) and may need to be adjusted -- default plan will be at normal 5-sigma level unless tuning agreed upon to a lower level 111 * test chunk should be evaluated in more detail -- see below 112 * MD not a great equal comparison since exptimes were longer (but was also 5-sigma) 113 * [[html(<span style="color:red">[sc] Not sure if the catalog size is not going to explode if threshold too small. WWdiff is at 2.5-sigma(not sure?). What was the value for WSdiffs e.g. MDs? We could use the values (in each rgiz) unless something has changed. Not sure about what's used for w-band.</span>)]] 113 114 114 115 * WSdiff published to IPP-MOPS-WS -- WWdiff possibly later to regular datastore IPP-MOPS-TEST 115 116 * normal OSS warp-warp diffims will go to IPP-MOPS-TEST during the night 116 117 117 * [[html(<span style="color:red">[sc] We will likely request WWdiff to be published to the regular datastore (IPP-MOPS-TEST) later (manual queuing/processing at the IPP level OK for MOPS)</span>)]] 118 118 … … 138 138 139 139 Tasks to do -- priority order now 140 * verify w-band stacks okay along ecliptic for opposition end October -- new reference stacks to be made for the expected area (mix of reprocessing+updates to minimize data load) 141 * WSdiff detection threshold -- 5-sigma default but may need to lower -- preliminary tests shows default 5-sigma should recover WWdiff threshold ~3.5 in MOPS test chunk 140 * verify w-band stacks okay along ecliptic for opposition end October -- 141 * new reference stacks to be made for the expected area (mix of reprocessing+updates to minimize data load) -- NCU.ref.20161026 -- (add more details) 142 * WSdiff detection threshold -- 5-sigma default but may need to lower 143 * preliminary check of known sources shows default 5-sigma should recover ones with WWdiff threshold ~3.5 in MOPS test chunk -- 142 144 * MOPS interested in SSdiff -- published where? 143 * check processing rate/nodes for WSdiffs -- during the night of observations -- likely the normal 3x c2 group is sufficient but will have some nodes available to boost as needed (more c2 and/or m0+1, x3?) 145 * check processing rate/nodes for WSdiffs -- during the night of observations -- likely the normal 3x c2 group is sufficient but will have some nodes available to boost as needed (more c2 and/or m0+1, x3?) -- only x2+3 available 144 146 145 147
