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Table 1

Overview of the ELAIS-S1 observations.

Filter Ep/Date Exp. time (s) m lim Seeing (″)

R 0/2003-08 8640 0.65
R 1/2004-07 5760 26.83a 0.68
R 2/2004-08 8280 26.97a 0.67
R 3/2004-09 5520 26.71a 0.69
R 4/2004-10 8760 26.94a 0.89
R 5/2004-11 7560 26.80a 0.80
R 6/2004-12 7320 26.75a 0.80
R 7/2005-01 5760 26.88a 0.76
R Cb/2006-Jan. 8 760 0.72
I 0/2003-08 11 520 0.59
I 1/2004-07 11 520 26.60a 0.59
I 2/2004-08 18 240 26.41a 0.64
I 3/2004-09 9960 26.39a 0.71
I 4/2004-10 11 520 26.52a 0.68
I 5/2004-11 15 960 25.85a 0.76
I 6/2004-12 19 080 26.04a 0.64
I 7/2005-01 12 480 26.30a 0.70
I Cb/2006-Jan. 11 520 0.69

U 2003-2006 37 740 27.44c 0.73
B 2003-2006 34 940 28.53c 0.71
V 2003-2006 20 060 26.93c 0.71

Notes. The upper part of the table shows the observational properties of the RI supernova search epochs, the lower part shows the properties of the UBV observations. The entries in the table are mean values over the four VIMOS quadrants.

(a)

3σ magnitude limits estimated from the photometric scatter of simulated sources placed in faint galaxies (mI > 24.0) in the individual subtracted epoch images (see Sect. 4.1).

(b)

Control epochs, taken approximately one year after the final SN survey epoch.

(c)

3σ magnitude limits using a 4    ×    FWHM diameter aperture.

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