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Table 11

Possible flares in the pure AGN-continuum (blue and red) and the corresponding changes of the Hβ and Hα fluxes.

N UT-Date cnt-agn5100 Amplitude cnt-agn6200 Amplitude F(Hβ)agn Var F(Hα)agn Var
1 2 3 4 5 6 7 8 9 10

1 1989 Oct. 27 3.70 35.6% 36.09 12%
1989 Oct. 28 2.21 42.87
2 1998 Jul. 25 5.71 28% 5.98 23% 16.0 1.2% 59.33 4.7%
1998 Jul. 26 8.58 8.30 15.72 55.49
3 2000 Apr. 24 2.40 17.7% 3.07 23.8% 12.47 3.5% 45.96 5.3%
2000 Apr. 25 3.09 4.31 11.87 49.51
4 2002 Apr. 02 4.18 5.8% 12.1 1.1%
2002 Apr. 03 3.32 33.4% 41.83 4.4%
2002 Apr. 05 4.54 5.38 12.29 44.51
5 2003 Mar. 24 2.81 20% 12.15 3.0%
2003 Mar. 25 3.74 4.0 34.5% 11.65 42.01 1.3%
2003 Mar. 26 2.43 41.23
6 2004 Apr. 11 4.51 23% 4.54 7.2% 11.4 1.4% 38.88 1.0%
2004 Apr. 12 3.25 11.17
2004 Apr. 13 5.03 38.36
7 2006 Aug. 28 3.38 19.8% 5.56 25.5% 12.01 3.3% 41.38 5.2%
2006 Aug. 28 4.92 4.33 11.46
2006 Aug. 29 4.65 12.67 45.02
2006 Aug. 30 3.72 3.32 12.03 39.82
2006 Aug. 30 3.73 12.35
2006 Aug. 31 2.88 3.35 12.30 42.06
8 2009 May 17 2.83 21.4% 3.19 34% 11.22 1.6% 37.95 1.7%
2009 May 19 3.84 6.29 10.97 36.88
2009 May 20 6.29 36.86

Notes. Column (1): number of the possible flare. Column (2): date. Columns (3) and (5): pure AGN blue (at 5100Å) and red (at 6200Å) continuum flux, corrected for the host-galaxy contribution, in units of 10-16 erg cm-2 s-1 Å-1. Columns (4) and (6): flare amplitude in %. Columns (7) and (9): Hβ and Hα fluxes corrected for the host-galaxy contribution, in units of 10-14erg  cm-2   s-1. Columns (8) and (10): The change in the line flux in %.

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