Table 2: Statistics for the triple comparisons process. The 8 columns give respectively the code of the observing period, the filter, the number of comparisons  $N_{\rm tri}$, the sky area involved in the comparisons  $S_{\rm tri}$, the limiting magnitude of the comparisons  $M_{\rm lim}$, the number of asteroids found in the comparisons  $N_{\rm ast}$, the number of variable sources found in the comparisons  $N_{\rm var}$, and the number of variable candidates per 106 astrophysical objects found by the program N6.
Run Flt $N_{\rm tri}$ $S_{\rm tri}$ $M_{\rm lim}$ $N_{\rm ast}$ $N_{\rm var}$ N6
      [deg2]        
05AQ01 g' 24 20.83 23.1 1072 242 744
05AQ03 i' 31 27.55 22.0 912 362 585
05AQ04 g' 16 14.36 22.9 618 398 537
05AQ04 r' 50 44.94 22.5 2543 842 657
05AQ05 g' 16 14.31 22.6 488 302 599
05AQ05 i' 10 9.02 22.0 288 88 387
05BQ11 g' 7 6.32 23.4 274 91 624
05BQ13 r' 20 17.95 22.6 1129 270 746
05BQ13 i' 13 11.73 22.1 507 220 505
06AQ01 r' 18 16.19 22.1 749 152 638
06AQ01 i' 13 11.73 22.7 800 542 762
All - 218 194.94 22.5 9380 3509 628

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