Table 1: The fields observed and their coordinates, the exposure times, the magnitude at which the narrow band data are 50% complete and the image quality of the stacked images. All magnitudes are in Vega and have been corrected to 4 $^{\prime \prime }$ diameter apertures. The 90% completeness limit is approximately 0.5 mag brighter. The field names correspond to those used at http://www.eso.org/science/goods/.
Field RA Dec Exp. Lim. IQ
  (2000) (2000) time mag. FWHM
      (s) (Vega) ( $^{\prime \prime }$)
F09 03:32:33.2 -27:44:55 10 800 23.4 0.55
F11 03:32:10.6 -27:44:55 18 000 23.2 0.46
F14 03:32:38.8 -27:47:25 21 600 23.2 0.55
F15 03:32:27.5 -27:47:25 6000 22.4 0.69
F16 03:32:16.2 -27:47:25 26 400 23.2 0.53
F20 03:32:33.2 -27:49:55 18 000 23.3 0.59
F21 03:32:21.9 -27:49:55 20 400 23.3 0.58

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