Changes between Version 163 and Version 164 of MD.GR0

Timestamp:

Oct 9, 2011, 1:58:04 PM (15 years ago)

Author:

Mark Huber

Comment:

--

MD.GR0

@@ -103 +103 @@
 Compared to the cumulative metrics at http://ipp0022.ifa.hawaii.edu/ps1sc/metrics/range_2010-05-13_current/
 
-Histograms of the FWHM major and minor from camera stage for reprocessed g-band exposures (red) and refstack.20110722 (top blue), psfrefstack.20110814 (middle blue) and refstack.20100721 V2 (bottom blue). The unmatched blue/red overlap for refstack.20110722 FWHM major<6.5 pixels for exposures in the refstack is from using also low zeropoint and bright background cuts. Psfrefstack used <5.1 pixels.
-[[Image(MD10.g.00000.expfwhm_stkrefpsfv2.png,300px)]]
-
-The same refstacks with the selected exposures over time
-[[Image(MD10.g.00000.expfwhmzptbgmjd_stkrefpsfv2.png,300px)]]
+|| Histograms of the FWHM major and minor from camera stage for reprocessed g-band exposures (red) and refstack.20110722 (top blue), psfrefstack.20110814 (middle blue) and refstack.20100721 V2 (bottom blue). The unmatched blue/red overlap for refstack.20110722 FWHM major<6.5 pixels for exposures in the refstack is from using also low zeropoint and bright background cuts. Psfrefstack used <5.1 pixels.
+|| [[Image(MD10.g.00000.expfwhm_stkrefpsfv2.png,300px)]] ||
+
+|| The same refstacks with the selected exposures over time || [[Image(MD10.g.00000.expfwhmzptbgmjd_stkrefpsfv2.png,300px)]] ||
 
 Sample skycell coverage map by good_frac with N input warps, N rejected warps, dtime_script for making stack, and if quality error that rejects entire skycell. The ~130 input warps provided enough of a sample for the outer edge skycells from earlier exposures.