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Changes between Version 29 and Version 30 of PSNSC_NCU


Ignore:
Timestamp:
Oct 26, 2016, 12:15:00 AM (10 years ago)
Author:
Mark Huber
Comment:

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  • PSNSC_NCU

    v29 v30  
    108108 * WSdiff runs in ~ippmops/stdscience_ws with modified ipp-20141024 ops tag to make uncompressed WSdiffs (like FSS, PSNSC_MOPS)
    109109  * 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>)]]
    113114
    114115 * WSdiff published to IPP-MOPS-WS -- WWdiff possibly later to regular datastore IPP-MOPS-TEST
    115116  * normal OSS warp-warp diffims will go to IPP-MOPS-TEST during the night
    116 
    117117  * [[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>)]]
    118118
     
    138138
    139139Tasks 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 --
    142144 * 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
    144146
    145147