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Table 5.

Variability statistics (Fmin, Fmax, Rmax, ⟨F⟩, σF, and Fvar) for the continuum (after correction for Galactic foreground extinction) and for the broad emission lines (after correction for the contribution of narrow-line components; see Table 3).

Cont./Line Fmin Fmax Rmax F σF Fvar
Comb. V band 3.22 6.65 2.07 4.41 0.97 0.21

Cont. 4425 (4225) 4.51 10.01 2.22 6.22 1.77 0.28
Cont. 4755 (4540) 4.04 8.87 2.20 5.67 1.52 0.27
Cont. 5420 (5180) 3.22 6.65 2.07 4.50 1.01 0.22
Cont. 5485 (5240) 3.28 6.59 2.01 4.54 0.99 0.22
Cont. 5755 (5500) 3.02 6.04 2.00 4.23 0.90 0.21
Cont. 6530 (6240) 3.00 5.34 1.78 3.85 0.68 0.17
Cont. 7255 (6930) 3.20 5.03 1.57 3.93 0.54 0.14

Hγ 122.2 184.7 1.51 154.6 17.6 0.11
Hβ 542. 754. 1.39 670. 46. 0.07
Hβblue+He IIλ4686 33.2 76.80 2.31 57.8 9.6 0.17
Hβcenter 419. 556. 1.33 502. 30. 0.06
Hβred 89.2 126.8 1.42 109.5 8.5 0.08
HeI λ5876center 63.7 129.1 2.03 92.7 13.2 0.14
Hα 2293. 2813. 1.23 2562. 118. 0.04
Hαblue 131.3 192.4 1.47 159.2 14.7 0.09
Hαcenter 2082. 2456. 1.18 2286. 93.3 0.04
Hαred 79.6 166.9 2.10 116.1 23.9 0.21

Notes. In units of 10−15 erg s−1 cm−2 Å−1 for the continuum and in units of 10−15 erg s−1 cm−2 for the broad emission lines. The fluxes in this table are observed-frame fluxes. The continuum wavelength values in brackets correspond to the rest frame of Mrk 926.

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