Table 4: Two-spot solutions for the annual BVI light curves.
Year $\ell_{\rm N}$ $b_{\rm N}$ $r_{\rm N}$ $A_{\rm N}$ $\ell_{\rm S}$ $b_{\rm S}$ $r_{\rm S}$ $A_{\rm S}$ $T_{\rm spot}$

1988.87
461.73 -46.51 44.07 14.07 606.43 87.81 59.41 24.56 ...
1989.88 468.21 -66.34 55.90 21.96 597.52 88.22 61.04 25.79 ...
1990.95 326.78 -59.98 52.51 19.57 471.06 67.79 59.89 24.92 ...
1992.87 394.80 -59.45 73.74 36.00 624.22 27.68 23.68 4.21 ...
1993.91 397.53 -55.56 68.74 31.87 667.14 37.77 23.35 4.09 ...
1994.95 374.49 -41.20 51.30 18.73 507.17 81.77 60.07 25.05 ...
1995.88 357.52 -39.90 49.22 17.34 495.76 81.69 65.06 28.91 ...
1996.97 344.75 -48.51 63.42 27.63 571.55 73.62 55.90 21.97 ...
1997.49 349.07 -51.62 57.91 23.44 572.45 76.36 59.17 24.37 ...
1997.93 327.28 -50.24 55.26 21.51 487.61 72.02 61.29 25.98 3905
1998.81 281.78 -67.14 53.28 20.10 446.18 78.55 59.82 24.86 3621
1999.88 216.45 -57.36 55.44 21.63 359.67 84.89 50.50 18.19 3562
2000.92 181.45 -52.35 40.46 11.95 383.74 75.26 55.89 21.96 ...
2001.90 144.98 -66.31 48.27 16.71 316.37 73.70 51.75 19.04 3700
2002.89 152.25 -51.86 31.27 7.26 281.15 72.22 62.99 27.29 3478
2003.85 171.40 -66.72 48.04 16.57 254.50 76.60 58.11 23.58 3769
2004.86 151.80 -56.38 51.20 18.67 281.85 83.96 50.71 18.33 ...
2005.87 140.83 -70.25 71.49 34.12 206.94 83.39 37.91 10.55 3899
2006.91 259.85 -85.79 67.88 31.17 266.99 87.82 40.09 11.75 ...
Note: index N indicates the north polar cap, S the south polar cap. Longitude, $\ell_{\rm N/S}$, is counted from 0 (a time of maximum positive radial velocity of the primary according to Table 2) to 360$^\circ$ in the same direction as the orbital motion. Latitude, $b_{\rm N/S}$, is counted from 0 = equator to $\pm$$90^\circ$ = poles; radius, $r_{\rm N/S}$, in degrees (circular spots); fractional area, $A_{\rm N/S}$, in per cent of the entire stellar surface and the spot temperature ( $T_{\rm spot}$) in Kelvin (for light-curves with good VI data; note that the photospheric temperature is 4500 K). Individual spot temperatures are assumed to be identical.

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