Changes between Version 10 and Version 11 of IPP_Progress_Report_20120903
- Timestamp:
- Sep 11, 2012, 1:20:08 PM (14 years ago)
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IPP_Progress_Report_20120903
v10 v11 6 6 === Eugene Magnier === 7 7 8 * finished up the psphot saturated star radial profile analysis, and it really helps a lot (see Bill's report). Also fixed some issues with duplicate detections (using a mask to block re-detection of the cores) and negative fluxes in linear fits (at least in psphot; psphotStack was fixed earlier). 9 * update the dvo schema and pushed changes into the trunk. 10 8 11 === Serge Chastel === 9 12 * Tuesday off 10 13 * Documentation of the "Who is the cluster?" software. 11 14 * "Who is the cluster?" given to MOPS/Denver. 15 12 16 === Heather Flewelling === 13 17 … … 21 25 * attempts at processing isp-sas stuff is located here: http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/IspSasProcessing 22 26 * lots of sciency stuff with JT (not involving sas! ) 27 23 28 === Mark Huber === 24 29 * vacation 30 25 31 === Bill Sweeney === 26 32 * Tested Gene's improvements to psphotStack to better model massively saturated stars. The number of false detections is greatly reduced around such objects. … … 34 40 * Lot's of assistant czar work helping to manage the fallout from the MHPCC cluster power outage and various other strange problems. 35 41 36 37 42 === Chris Waters === 38 43 * Investigated the possibility of minimizing row-to-row variations by constructing 8 per-OTA correction images. http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/GPC1_Bias_Pattern_Study This looks somewhat promising, although it will require some level of development.
