Changes between Version 1 and Version 2 of NightlyScienceV2

Timestamp:

Dec 21, 2010, 3:24:38 PM (16 years ago)

Author:

watersc1

Comment:

--

NightlyScienceV2

@@ -48 +48 @@
 === UNRECOVERABLE_QUALITY ===
 
+This lists {{{quality}}} values that are acceptable for a warp stage exposure to have with respect to stack queuing.  If a warp has one of these values, then it is counted as full, even if not.
 
+=== MACRO_DEFINITIONS ===
 
+These define a macro to be executed by pantasks upon successful completion of a task.  The {{{PROC_MODE}}} describes the stage of {{{nightly_science.pl}}} the macro defined in {{{MACRO}}} should be executed.  This is not well tested and is not used at the moment.
+
+=== TARGETS ===
+
+These rules define the properties of exposures for each survey target.  Each target must have a {{{NAME}}}.  Exposures that comprise this target are defined by one or more of the the {{{OBSMODE,OBJECT,COMMENT}}} fields, which accept SQL-like % wildcards.  The {{{DISTRIBUTION,TESS,REDUCTION}}} fields allow the {{{dist_group,tess_id,reduction}}} to be set for the science processing.  The two booleans {{{STACKABLE,DIFFABLE}}} define whether this target should be examined for stacks and diffs.  The {{{MIN_STACK}}} sets the minimum number of warps needed to make a stack while observing is still happening.  Finally, any of the {{{CLEAN_MODES}}} listed above may be set here to change the retention time for this data.
+
+=== DETRENDS ===
+
+These rules define how the detrend verify runs are queued.  Each has a {{{NAME}}} and use {{{DETTYPE,EXPTYPE}}} to determine the type of verify run to generate.  The reference detrend is set using the {{{REF_ID,REF_ITER}}} values.  If a {{{FILTER}}} value is set, then only exposures in that filter are used for the verification.  The number of exposures to use in the verification process is set by {{{MAX_EXP}}}.
 
 == Faults ==