Due to a glitch in the analysis pipeline there are apparent increases in flux around MJD 56810 for many sources. These increases are *not* real and should be disregarded. The problem is now believed to be fixed, and the most recent flux measurements are expected to be correct. At a later date the light curves will be reprocessed to remove these incorrect data points.
Please pay attention to all of the caveats on the Aperture Photometry Lightcurve Page. All of the warnings detailed there pertain to this analysis as well.
The following lightcurves were found to have extraordinary flaring events in the last 28 days. This page is updated whenever the Aperture Photometry Lightcurves are updated. These events were determined in the following fashion:
Each panel shows:
Looking for flares from MJD 56924 to MJD 56952.
Assoc: PMN J1911-1908
Assoc: MG1 J050533+0415
Assoc: 4C +71.07
Assoc: PKS 0502+049
Assoc: PKS 1352-104
Assoc: PKS B1908-201
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