All Tables

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.
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.
Table 3: Effective wavelength of the filters used in the photometric monitoring programme.
Table 4: Equivalent widths of the most prominent lines detected during flare #4. A comparison is done with the classical T Tauri star LkH $_{\alpha }$ 264.
Table 5: Radial velocities and H $_{\alpha }$ equivalent widths (line and residual line) measured from the high resolution spectroscopic observations.
Table 6: Parameters of the Gaussian curves used for fitting the residual H $_{\alpha }$ line. I: Gaussian maximum; V: Gaussian central velocity in km s^-1; and FWHM in km s^-1.
Table 7: List with all historically recorded flares on V410 Tau, including the ones newly detected in our campaign. Note that, in some cases, the observations presented in the literature are merely indicative of a flare, by e.g. the deviation of one or a few data points from the usual behavior of V410 Tau, rather than by providing a convincing sampling of the time evolution of the flare.