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Table A.4.

Results relative to the temporal and spectral optical analysis.

name N (×100 mJy) a b tb/104s χ2/dof log10(Lopt(erg/s))
Sample 1

050824 4.2 ± 0.1 0.66 ± 0.01 - - 58.9/27 -

050319 0.9 ± 0.1 0.53 ± 0.02 2.85 ± 0.30 41.57 ± 3.40 39.9/37

050416A 11.9 ± 2.1 −0.31 ± 0.32 0.92 ± 0.07 0.05 ± 0.02 40.1/28

051109A 17.2 ± 0.3 0.81 ± 0.02 - - 25.0/21 -

060526 2.5 ± 0.2 0.60 ± 0.01 2.64 ± 0.10 15.78 ± 0.85 199.0/43

060605 12.0 ± 1.6 0.80 ± 0.03 3.00 ± 0.17 2.45 ± 0.18 165.5/29

060729 31.0 ± 2.1 0.02 ± 0.03 1.60 ± 0.03 8.16 ± 0.72 305.0/41

061121 4.9 ± 4.2 0.53 ± 0.08 1.26 ± 0.14 4.09 ± 3.93 58.2/30

080413B 1.5 ± 0.1 0.43 ± 0.01 3.00 ± 0.27 40.12 ± 2.46 213.7/25

080605 8.0 ± 0.1 0.64 ± 0.01 - - 172.4/39 -

090618 44.3 ± 10.9 0.51 ± 0.05 1.45 ± 0.04 1.72 ± 0.43 43.2/43

091018 1.2 ± 0.1 0.91 ± 0.01 2.84 ± 0.32 12.51 ± 0.88 42.5/36

091029 3.8 ± 0.8 0.39 ± 0.03 1.63 ± 0.13 5.87 ± 1.43 48.6/37

100621A 32.2 ± 2.7 0.22 ± 0.02 2.41 ± 0.18 4.00 ± 0.40 2560.6/29

110213A 290.4 ± 5.6 0.20 ± 0.01 2.01 ± 0.02 1.52 ± 0.04 2645.9/41

111228A 29.4 ± 2.6 0.25 ± 0.03 1.54 ± 0.04 1.91 ± 0.20 72.5/39

130702A 320.1 ± 24.6 1.31 ± 0.02 - - 41.8/40 -

140419A 15.1 ± 0.2 1.06 ± 0.01 - - 119.6/34 -

180728A 123.7 ± 1.7 1.08 ± 0.01 - - 92.5/39 -

Sample 2

050730 74.9 ± 13.0 −0.22 ± 0.28 1.58 ± 0.08 0.74 ± 0.19 236.9/18

060614 8.6 ± 0.6 0.03 ± 0.06 2.47 ± 0.08 7.55 ± 0.46 48.4/22

080310 175.7 ± 5.0 −0.60 ± 0.10 1.16 ± 0.01 0.18 ± 0.01 795.5/43

081007 8.9 ± 0.1 0.73 ± 0.01 - - 272.4/38 -

081029 197.6 ± 3.0 −1.31 ± 0.06 1.90 ± 0.02 0.86 ± 0.02 316.7/30

100219A 6.9 ± 0.2 0.99 ± 0.02 - - 73.1/21 -

100418A 21.6 ± 0.8 −0.32 ± 0.03 1.66 ± 0.04 5.72 ± 0.33 200.0/31

100814A 8.2 ± 0.2 0.09 ± 0.01 3.90 ± 0.15 39.14 ± 0.70 3100.6/47

110715A 9.6 ± 1.3 0.52 ± 0.01 2.87 ± 0.30 37.49 ± 3.19 123.4/30

120404A 147.0 ± 3.0 −1.65 ± 0.11 1.60 ± 0.04 0.26 ± 0.01 22.3/38

150910A 315.1 ± 11.6 −4.00 ± 0.34 1.26 ± 0.01 0.11 ± 0.00 75.3/36

Notes. The first four columns show the best-fit parameters. The break time tb is in the observer frame. The fifth column is the reduced χ2, and Lopt is the average optical luminosity during the plateau, if present. The reported parameters are specified in the text. Errors are given at one sigma level of confidence. When the fit with a broken power law does not converge, we performed the fit with a single power law, and therefore only the value of the slope a is reported.

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