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Changes between Version 3 and Version 4 of PSNSC_NCU


Ignore:
Timestamp:
Oct 13, 2016, 10:46:22 PM (10 years ago)
Author:
Mark Huber
Comment:

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  • PSNSC_NCU

    v3 v4  
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    4 NCU observations -- processing needs to be finished by early morning for MOPS to use
    5  * obs_mode NCU (new end Oct 2016 possibly) -- 8 fields/targets (chunks?), 8 dithers for 6 hrs (64 exposures per field?), 45s exptime over 4 nights? (not sure right yet)
    6   * offset only dither (no rotation like MD)
    7   * WSdiff and published to normal MOPS datastore location
    8  * chip->warp normal stdscience pantasks as with xSS products
    9  * WSdiff runs in ~ippmops/stdscience_ws with modified ipp-20141024 ops tag to make uncompressed WSdiffs (like FSS) -- larger volume, may need more nodes -- must be uncompressed for MOPS stamps since large data volume
    10  * comment string -- needs to be worked on
     4NCU observations -- processing needs to be finished by early morning for MOPS to use for NEO
     5 * obs_mode NCU -- new, possibly start end Oct 2016
     6  * 4 chunks (visits?) -- NCU1B...NCU4B -- B=color set, sequence wgwrwiwz per chunk; A=w-band only (8 returns, dither?)
     7  * 8 targets (fields?) --   NCU1.1...NCU1.8; NCU2.1...NCU2.8; NCU3.1...NCU3.8 ; NCU4.1...NCU4.8
     8  * offset only dither (no rotation like MD) -- is the offset in the queue files yet? is the dither added to each visit?
     9  * exposures per field --
     10   * griz -- 1/chunk * 4 chunks = 4
     11   * w -- B: 4/chunk * 4 chunks = 16; A: 8/chunk * 4 chunk = 32
     12  * 4 sequential nights, ~6 hr/night?
     13  * exptimes wgriz: 60,120,120,120,180s
     14  * comment string -- needs to be descriptive and easily parsed
     15   * B: NCU1B w4 NCU1.1 -- (chunk) (filter)(set number for w) (target) --
     16    * need to replace set number with (visit number) at end of all comments? is this tricky for generating/running queue?
     17   * A: NCU1A NCU1.1 --
     18    * add w for filter even though default?
     19    * add (visit number) at end of all? is this tricky for generating/running queue?
     20 * chip->warp normal stdscience pantasks as with xSS products (ipp-20141024 tag)
     21 * WSdiff runs in ~ippmops/stdscience_ws with modified ipp-20141024 ops tag to make uncompressed WSdiffs (like FSS)
     22  * larger volume, may need more nodes -- must be uncompressed for MOPS stamps since large data volume
     23 * WSdiff published to normal MOPS datastore location?
    1124
    1225
     
    1528 * warp-stack diffims -- NCU.WS.nightlyscience -- nightly
    1629 * publishing of WSdiffs -- (need datastore location to use from MOPS) -- nightly
    17  * nightly stack -- NCU.nightlyscience -- nightly, manually done to avoid any poor images
    18  * stack-stack diffims -- NCU.SS.nightlyscience -- nightly, likely automatic possible once manual stacks made
     30 * manually done -- not czar responsibility
     31  * nightly stack -- NCU.nightlyscience -- nightly, manually done to avoid any poor images
     32  * stack-stack diffims -- NCU.SS.nightlyscience -- nightly, likely automatic possible once manual stacks made
    1933 * stamps -- TBD
    2034