Changes between Version 8 and Version 9 of IPP_Progress_Report_20121015
- Timestamp:
- Oct 24, 2012, 8:43:06 AM (14 years ago)
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IPP_Progress_Report_20121015
v8 v9 4 4 (Up to [wiki:IPP_Progress_Reports IPP Progress Reports]) 5 5 6 === Eugene Magnier === 6 === Eugene Magnier ===' 7 8 * investigations in to more ipp / psps concerns (PSF theta - found a bug in the I/O layer treating degrees as radians, funny kron mags noted by Ken - these were known garbage based on dvo / psps flags) 9 * some exploration of the PS and PS1SC web sites and content management systems. Make a mock-up of the PS public web site using Word Press that is not bad, but would need some cleanup. 10 * work on the IPP data distribution pages, need to make these a bit more clear 11 * readying phot ladder paper for submission. 7 12 8 13 === Serge Chastel === … … 10 15 * Spent (wasted?) more time than I wanted with Condor web services compilation/installation at mhpcc for the ippdor account; 11 16 * mops data format 3 tests preparation; 17 12 18 === Heather Flewelling === 13 19 … … 16 22 * ipptopsps work 17 23 * some science stuff 24 18 25 === Mark Huber === 19 26 * various liaison issues 20 27 * MD05 prep for full reprocessing of all exposures that were not done with the ubercal catalog 21 28 * observing at subaru 29 22 30 === Bill Sweeney === 23 31 * Continued investigation into the differences between the psphotStack aperture flux measurements for the different convolved images. It appears that we have different flux level when we build the psf matched stack. For a given radial aperture, the difference is .02 - .04 magnitudes where the image convolved to 6 pixels is higher. The offset is a function of the stack_id. The cause is still under investigation
