This article has an erratum: [https://doi.org/10.1051/0004-6361/201016348e]
Characteristics of the MPG-ESO/WFI, CFHT/Megaprime and INT/WFC data.
|Instrument||Filter||texp [s]||Seeing [′′]||Mlim [AB]|
|WFC/INT||g||1800||1.′′50 ± 0.21||24.2 ± 0.2|
|WFC/INT||r||1800||1.′′33 ± 0.14||23.5 ± 0.1|
|WFC/INT||i||1800||1.′′30 ± 0.13||22.8 ± 0.1|
Notes. The limiting AB magnitudes represent the 5σ completeness limit for non-stellar sources. The scattering in seeing and depth for the INT/WFC pointings is given as well (excluding pointings 1−3 for gi which are significantly worse, see Sect. 2.3).
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