Changes between Version 123 and Version 124 of ppSub_testing_201201
- Timestamp:
- May 24, 2012, 9:23:52 PM (14 years ago)
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ppSub_testing_201201
v123 v124 806 806 || [[Image(1_md04s052.i.20120410_ipp_dophot_det_panel.jpg,300px)]] || 807 807 808 809 = Extra IPP/Photpipe Calibration Catalogs 20120524 = 810 Ken Smith looked into the new ubercal calibration of the IPP images in terms of the diffim photometry in comparison to the photpipe photometry. 811 812 http://ps1sc.ifa.hawaii.edu/PS1wiki/index.php/DRAVG_telecon#Post-Ubercal_Diffs 813 814 815 Photpipe catalogs (from Sept. 2011): basic ASCII tables, header line 1. 816 817 http://orac.ifa.hawaii.edu/ipp_tests/md_abscat110912_120524 818 819 IPP refcat/ubercal from May 2012: dump of the current refcat.20120503 for the MD field region using getstar into FITS tables. The MAG_C1,MAG_C2 columns are for each filter 820 * g: g,i 821 * r: r,i 822 * i: r,i 823 * z: i,z 824 * y: z,y 808 825 826 http://orac.ifa.hawaii.edu/ipp_tests/md_refcat20120503v0_120524 827 828 829 || [[Image(md04_gi_photrefcat_sample120524.png,300px)]] || || 830 831 809 832 = Extra IPP Comparison Set 20120516 = 810 833 … … 842 865 || || || || 843 866 867 Diffims are not necessarily better for convolving the other direction. More often than not seems the psphot detections of the source of interest is dropped from the inverting of the core flux, but not for all detections.
