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Changes between Version 123 and Version 124 of ppSub_testing_201201


Ignore:
Timestamp:
May 24, 2012, 9:23:52 PM (14 years ago)
Author:
Mark Huber
Comment:

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  • ppSub_testing_201201

    v123 v124  
    806806||  [[Image(1_md04s052.i.20120410_ipp_dophot_det_panel.jpg,300px)]] ||
    807807 
     808
     809= Extra IPP/Photpipe Calibration Catalogs 20120524 =
     810Ken Smith looked into the new ubercal calibration of the IPP images in terms of the diffim photometry in comparison to the photpipe photometry.
     811
     812http://ps1sc.ifa.hawaii.edu/PS1wiki/index.php/DRAVG_telecon#Post-Ubercal_Diffs
     813
     814
     815Photpipe catalogs (from Sept. 2011): basic ASCII tables, header line 1.
     816
     817http://orac.ifa.hawaii.edu/ipp_tests/md_abscat110912_120524
     818
     819IPP 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
    808825 
     826http://orac.ifa.hawaii.edu/ipp_tests/md_refcat20120503v0_120524
     827
     828
     829||  [[Image(md04_gi_photrefcat_sample120524.png,300px)]] || ||
     830
     831
    809832= Extra IPP Comparison Set 20120516 =
    810833 
     
    842865|| || || ||
    843866
     867Diffims 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.