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Table 1:

Observational material for the construction of the light curve.

Telescope
$N_{\rm t}$ $N_{\rm e}$ Years Source

(a) Digitized photographic plates:
Asiago Schmidt 24 8 1968.8-1993.1 (1)
Calar Alto Schmidt 43 15 1983.0-2000.7 (1)
Calar Alto 1.2 m 8 5 1976.7-1982.6 (1)
Palomar Schmidt 4 4 1948.7-1989.7 (1), (3)
Sonneberg 40 cm 9 1 1992.2-1992.6 (1)
Tautenburg Schmidt 362 77 1961.5-1997.0 (1)
         
(b) CCD observations:
Calar Alto 2.2 m 3 2 2008.7-2009.3 (1)
CFHT 3.6 m 1 1 1993.8 (1)
INT (WFS) 5 1 1998.8 (1)
INT 522 6 1999.7-2003.7 (2)
Kitt Peak 4 m 10 2 2000.8,2001.7 (4)
Skinakas 60 cm 5 1 2007.6 (1)
Tautenburg Schmidt 30 14 2006.1-2009.7 (1)
         
(c) Original data from Sharov et al. (1998):
four other telescopes $\sim $150 84 1969.0-1997.7 (5)


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