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Table 3.

Light curve properties and results from the variability analysis.

Filter λeff N Δt F σ Fvar Rmax FAGN Fgal
(Å) (days) (mJy) (mJy) (mJy) (mJy)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
u 3468 ± 145 236 0.25 8.478 ± 0.046 1.3085 0.1542 ± 0.0004 1.556 7.91 ± 0.10 0.571 ± 0.026
v 4120 ± 92 240 0.23 8.141 ± 0.057 1.1378 0.1396 ± 0.0004 1.504 6.96 ± 0.13 1.179 ± 0.061
b 4668 ± 75 239 0.24 8.980 ± 0.062 1.1454 0.1273 ± 0.0004 1.452 7.00 ± 0.17 1.977 ± 0.102
y 5460 ± 90 241 0.23 9.412 ± 0.067 0.9976 0.1057 ± 0.0005 1.357 6.13 ± 0.31 3.285 ± 0.248
I 8105 ± 465 164 0.77 11.082 ± 0.086 0.9660 0.0868 ± 0.0006 1.262 6.75 ± 0.22 4.331 ± 0.214

Notes. Columns are as follows: (1) name of filter, (2) effective wavelength of the filter with the rms width of the transmission curve representing the filter’s wavelength uncertainty, (3) number of data points in the light curve, (4) median cadence value of the light curve, (5) mean flux value, (6) standard deviation of light curve, (7) normalized excess variance, (8) maximum to minimum flux ratio, (9) median AGN flux, and (10) median host-galaxy flux. The AGN and host-galaxy fluxes are measured from the FVG method.

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