All Tables

• Table 1: Details concerning the pointings for the U deep field. Filter central wavelengths and FWHM are given before and after (in italics) the convolution with the telescope, CCD and atmosphere transmissions. The area includes only the region where sources have been included in the catalog: it does not include border regions with vignetting or a low signal to noise ratio.
• Table 2: Zero points, color terms and airmasses for the different pointings and filters. Date and airmass (X) refer to the image taken as reference when the relative photometry was computed. The last column gives the values to be added to the Vega-system magnitudes to obtain AB magnitudes.
• Table 3: Completeness and limiting magnitudes and surface brightnesses (mag arcsec^-2) derived from simulated point-like and extended sources respectively. All values are in the AB system.