Table 2: Characteristic parameters for the largest photometric flare observed on V410 Tau in November 2001 with the uvby Strömgren filters. The flare amplitudes, luminosities and energies refer to the maximum emission, while the quiescent luminosity refers to the average luminosity just before the flare.
Flare amplitude (mag) Flare lum. (erg s^-1)[ $\times10^{32}$ ] Flare energy (erg)[ $\times10^{35}$ ] Decay time^* (h)

u v b y u v b y u v b y u v b y

Flare #4 3.01 2.02 1.32 0.96 31.0 32.2 33.3 29.4 93.7 78.0 71.3 69.6 3.5 2.4 1.8 1.7

Quiescent lum. (erg s^-1) 2.06 5.91 14.0 20.5

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

**Table 2:** Characteristic parameters for the largest photometric flare observed on V410 Tau in November 2001 with the *uvby* Strömgren filters. The flare amplitudes, luminosities and energies refer to the maximum emission, while the quiescent luminosity refers to the average luminosity just before the flare.
	Flare amplitude (mag)	Flare lum. (erg s^-1)[ $\times10^{32}$ ]	Flare energy (erg)[ $\times10^{35}$ ]	Decay time^* (h)
	u	v	b	y	u	v	b	y	u	v	b	y	u	v	b	y
Flare #4	3.01	2.02	1.32	0.96	31.0	32.2	33.3	29.4	93.7	78.0	71.3	69.6	3.5	2.4	1.8	1.7
Quiescent lum. (erg s^-1)					2.06	5.91	14.0	20.5

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