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 57001 to MJD 57029.
2FGLJ2243.9+2021 (340.99765,20.356163) Data: 2FGLJ2243.9+2021 Assoc: RGB J2243+203 |
2FGLJ2219.1+1805 (334.79593,18.085037) Data: 2FGLJ2219.1+1805 Assoc: MG1 J221916+1806 |
2FGLJ0108.6+0135 (17.173542,1.5907097) Data: 2FGLJ0108.6+0135 Assoc: 4C +01.02 |
2FGLJ0403.9-3604 (60.986019,-36.069637) Data: 2FGLJ0403.9-3604 Assoc: PKS 0402-362 |
2FGLJ1444.1+2500 (221.02882,25.015192) Data: 2FGLJ1444.1+2500 Assoc: PKS 1441+25 |
2FGLJ2056.2-4715 (314.06757,-47.254925) Data: 2FGLJ2056.2-4715 Assoc: PKS 2052-47 |
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