Table 1: Characteristic parameters for three of the four largest photometric flares observed on V410 Tau in November 2001. They were detected with the Johnson UBV filters. The flare amplitudes, luminosities and energies refer to the maximum emission. The quiescent luminosity refers to the average luminosity just before the flare and was very similar for all three flares.

	Flare amplitude (mag)			Flare lum. (erg s-1) [ ]			Flare energy (erg) [ ]			Decay time* (h)
	U	B	V	U	B	V	U	B	V	U	B	V
Flare #1	0.51	0.15	0.08	1.17	1.32	1.24	4.21	2.97	2.38	1.5	1.1	0.9
Flare #2	0.19	0.03	0.02	0.38	0.14	0.07	1.4	0.4:	0.2:	1.6	1.1	-
Flare #3	0.77	0.17	0.08	2.18	1.51	1.25	1.71	1.33	1.35	0.9	0.8	0.7
Quiescent lum.				2.0	9.3	18.3

^* Decay time back to 10% of the peak magnitude.