| Version 6 (modified by , 14 years ago) ( diff ) |
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IPP Progress Report for the week YYYY.MM.DD - YYYY.MM.DD
(Up to IPP Progress Reports)
Eugene Magnier
Serge Chastel
- Tuesday off
- Documentation of the "Who is the cluster?" software.
- "Who is the cluster?" given to MOPS/Denver.
Heather Flewelling
- czar for 2 days (including the day of mhpcc power outage)
- sas-subset : rsync://ipp0012.ifa.hawaii.edu/sas-subset contains all raw files all filters for skycell.1406.028 (and likely other skycells as well)
- sas9
- wait for gene for dvo changes
- built dvo for smfs (SAS_v8)
- wait for bill/gene for psphotstack
- sas-isp
- attempts at processing isp-sas stuff is located here: http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/IspSasProcessing
- lots of sciency stuff with JT (not involving sas! )
Mark Huber
Bill Sweeney
- Tested Gene's improvements to psphotStack to better model massively saturated stars. The number of false detections is greatly reduced around such objects.
- Ran staticsky and skycalibration analysis for SAS_v9 which is the new psphotStack running on the SAS_v8 pixels. Made a configuration error so had to run this twice.
- Started working on a design for software to manage "release versions" for IPP data. This is being done to support several requirements.
- users need updated calibration information in IPP data. For example zero points for a stack or exposure. These change with re-calibrations, but we have no method for tracking this information and so we can't update the headers of fits files which are requested by users through the postage stamp server
- currently there is no way to track which pixels the IPP used for to measure a given detection in the PSPS data base.
- we need to distinguish "released" data from test runs in the IPP data base.
- Iterated with Conrad on the postage stamp user interface project.
- Lot's of assistant czar work helping to manage the fallout from the MHPCC cluster power outage and various other strange problems.
Chris Waters
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