Changes between Version 27 and Version 28 of PSNSC_NCU

Timestamp:

Oct 17, 2016, 1:48:47 PM (10 years ago)

Author:

Mark Huber

Comment:

--

PSNSC_NCU

@@ -110 +110 @@
 [[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>)]]
 
- * WSdiff published to IPP-MOPS-WS -- normal MOPS datastore location for WWdiff possibly later
+ * WSdiff published to IPP-MOPS-WS -- WWdiff possibly later to regular datastore IPP-MOPS-TEST
 
 [[html(<span style="color:red">[sc] Please publish WSdiff to IPP-MOPS-WS</span>)]]
@@ -135 +135 @@
 
 Tasks to do -- priority order now
- * verify w-band stacks okay along ecliptic for opposition end October -- new reference stacks to be made for the expected area
- * detection threshold -- 5-sigma default but may need to lower?
+ * 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)
+ * WSdiff detection threshold -- 5-sigma default but may need to lower?
  * MOPS interested in SSdiff -- published where?
  * 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?)