Changes between Version 40 and Version 41 of ippToPsps_Stack

Timestamp:

Sep 20, 2011, 12:37:17 AM (15 years ago)

Author:

Mark Huber

Comment:

--

ippToPsps_Stack

@@ -34 +34 @@
 || filterID||unknown||TINYINT||0||filter identifier|| cmf primary header || FPA.FILTER. This single character filter (grizy) is then used to get the PSPS ID from Filter table [browser:trunk/ippToPsps/config/init/tables.vot here] ||
 || stackTypeID||unknown||TINYINT||0||stack type identifier|| DVO || Currently we have either DEEP_STACK or NIGHTLY_STACK, which we know when queuing up stacks. This is then used to get the PSPS ID from !StackType table [browser:trunk/ippToPsps/config/init/tables.vot here]||
-|| magSat||unknown||REAL||-999||saturation magnitude level|| NA || empty ||
+|| magSat||unknown||REAL||-999||saturation magnitude level|| cmf primary header || FSATUR (not set?) ||
 || analVer||unknown||SMALLINT||-999||analysis version index|| NA || empty ||
 || expTime||s||REAL||-999|| exposure time|| GPC1 || SELECT SUM(exp_time) * (COUNT(warp_id) - reject_images) / COUNT(warp_id) as EXPTIME FROM staticskyRun. JOIN-ed through numerous tables using stack_id starting point ||
 || nP2Images||unknown||SMALLINT||-999||number of P2 images contributing to this cell||GPC1 ||a count of images listed in the !StackToImage table - see below ||
-|| completMag||unknown||REAL||-999||95% completion level in mag|| NA || empty  ||
+|| completMag||unknown||REAL||-999||95% completion level in mag|| cmf primary header || FLIMIT (not set?)  ||
 || astroScat||unknown||REAL||-999||astrometric scatter for chip|| NA || empty ||
 || photoScat||unknown||REAL||-999||photometric scatter for chip|| NA || empty ||