Changes between Version 13 and Version 14 of PSST_QUB
- Timestamp:
- Jan 24, 2018, 3:06:37 PM (9 years ago)
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PSST_QUB
v13 v14 1 1 PSST QUB requirements and notes (draft) -- 2 2 3 [[PageOutline]] 3 4 4 Processing products -- like for MOPS, czar needs to make sure all faults are cleared daily for OSS, MSS, ESS, ThreePi products 5 == Processing products == 6 Like for MOPS, czar needs to make sure all faults are cleared daily for OSS, MSS, ESS, ThreePi products 5 7 * chip-cam-warp -- nightly 6 8 * warp-stack diffims -- nightly … … 9 11 10 12 11 QUB targeted observations (QUB.nightlyscience, QUB.WS/SS) should only be managed by Mark Huber .13 QUB targeted observations (QUB.nightlyscience, QUB.WS/SS) should only be managed by Mark Huber -- notes on psweb.mp.qub.ac.uk/psat-lv-wiki/index.php/Pan-STARRS_pages 12 14 13 Processing timescale -- ideal and last cutoff times for diffim catalogs to be available for QUB ingestion and processing (TBD) 15 16 == Processing timescale == 17 Ideal and last cutoff times for diffim catalogs to be available for QUB ingestion and processing (TBD) -- 14 18 * chip-cam-warp -- nightly 15 19 * warp-stack diffims -- nightly 16 20 17 21 18 Cleanup -- 22 == Cleanup == 23 (not up to date 20180124) 19 24 * chip -- 2 days (same as MOPS) 20 25 * warp -- 4 days (so weekends covered) 21 26 * WSdiff -- 4 days (so weekends covered) -- if disk space issue, can reduce this to 2 days as long as warps uncleaned the update time is minimal 22 27 * datastore WSdiff catalog bundles -- 1 month (manually done) 23 * ps_ud_QUB -- manual, only Mark Huber should d o24 * QUB.nightlyscience, QUB.WS/SS -- manual, only Mark Huber should d o28 * ps_ud_QUB -- manual, only Mark Huber should deal with 29 * QUB.nightlyscience, QUB.WS/SS -- manual, only Mark Huber should deal with 25 30 26 31 27 Tasks to do -- in order of possible accomplishment 32 == Tasks to do == 33 (not up to date 20180124) 34 in order of possible accomplishment -- 28 35 * only really need image+mask (compressed so ~ok) -- like MOPS could switch off weight image for less disk use in processing 29 36 * gpc2 import of PV3 stack products -- requires new ops tag and then export/import of gpc1 stack rows to gpc2 … … 48 55 49 56 * gpc1 replication to ipp003 (tcs mysql) for QUB+ use -- will be retiring machines soon so need to work in that time frame 57 58 59 == Processing stage time summary == 60 Based on 20180122, 20180123 -- 61 * nightly rates limited by summitcopy, ch-cam-wrp ~60 exp/hr so keeps up with observations (generally can catchup to some degree ~80exp/hr possible?), WSdiff+distribution can match ~60-80 exp/hr without much modification 62 * dtime_script -- Nsources dependent generally, but on average (seconds) | sigma | min | max | 63 * ch -- 118.48012954361 | 34.706445650573 | 51.000003814697 | 668 | 64 * cam -- 448.97415129087 | 102.86848443046 | 9.9999856948853 | 1001 | 65 * wrp -- 63.084047381327 | 30.766145179551 | 12.999969482422 | 680 | 66 * WSdiff -- 102.62499931014 | 31.209872126263 | 56.000019073486 | 672 | 67 * timestamps using dateobs, diffRun.registered, distRun.time_stamp disappointing ~30-50 minutes for exposure through WSdiff to make it to datastore 68 {{{ 69 | exp_name | exp_time | dateobs | registered | time_stamp | chip_id | cam_id | warp_id | diff_id | dist_id | 70 +-------------+----------+---------------------+---------------------+---------------------+---------+---------+---------+---------+---------+ 71 | o8141g0062o | 120 | 2018-01-23 05:13:03 | 2018-01-23 05:40:40 | 2018-01-23 06:04:29 | 2048378 | 2014852 | 1991114 | 1651871 | 5171373 | 72 | o8141g0448o | 120 | 2018-01-23 16:02:14 | 2018-01-23 16:25:41 | 2018-01-23 16:34:55 | 2048727 | 2015202 | 1991463 | 1652218 | 5171558 | 73 | o8141g0249o | 45 | 2018-01-23 08:13:04 | 2018-01-23 08:40:38 | 2018-01-23 09:21:44 | 2048561 | 2015036 | 1991299 | 1652074 | 5171500 | 74 | o8141g0440o | 45 | 2018-01-23 11:11:03 | 2018-01-23 11:35:39 | 2018-01-23 11:43:22 | 2048720 | 2015195 | 1991452 | 1652210 | 5171550 | 75 | o8141g0445o | 45 | 2018-01-23 11:15:53 | 2018-01-23 11:40:39 | 2018-01-23 11:57:05 | 2048725 | 2015200 | 1991459 | 1652216 | 5171556 | 76 }}} 77 * manually crontab queuing WSdiffs still -- sped up somewhat -- need full night to see 78 * pstamp and updates can be limiting factor as well for flagging real transients -- 79 * need to adjust warp+WSdiff pixel cleanup to match QUB request window -- suspect 1 week for warp and 3 day for WSdiff would be sufficient (current 2/60hr day warp, 1 day/36hr WSdiff) 80 * splitting out QUB updates to dedicated nodes also useful -- depends on timing and nodes to be allocated 81 82 83 84 85
