All Tables

Table 1: Statistics of the catalog creation process. The 9 columns give respectively the code of the observing period or run (see footnote 6), the filter f, the galactic latitude b, the number of images $N_{\rm obs}$ , the number of square degrees observed $S_{\rm obs}$ , the median precision of the astrometric calibration $\delta _{\rm pos}$ , the limiting magnitude $M_{\rm lim}$ (see text), and the number of astrophysical objects found par square degree $N_{\rm obj}/{\rm deg}^{2}$ .
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.
Table 3: Statistics for the double comparisons process. The columns are identical to those of Table 2, except for $N_{\rm sin}$ which is the number of new or vanished objects. This number is higher for the g' filter images of 05AQ04 and 05AQ05 because halos of bright stars generate more fake objects in this filter.
Table 4: Characterization of variable objects of 05AQ01.
Table 5: Comparison of 4 programs dedicated to the search of GRB optical afterglows, $\beta$ have been chosen according to Totani & Panaitescu (2002).