All Tables

• Table 1: Open clusters observed at ESO and UTSO in 1995 (upper panel) as well as CASLEO in 1998 and 2001 (lower panel). The ages (log t) and distance moduli (V₀-M_V) were taken from the literature. The limit of apparent variability (Limit) is according to Sect. 3. The errors in the final digits of the corresponding quantity are given in parentheses.
• Table 2: Photometric data for the Johnson UBV system taken from WEBDA for the identified variable stars; the mean reddening values for the open clusters are according to the literature. The lower panel includes the four variable objects which are most probably not members of the corresponding cluster. The objects are numbered according to WEBDA or to our internal numbering system (marked with asterisks).