All Tables

Table 1: Observational parameters and AO performances for NACO observations of SWAN fields. See the text for a full description of the entries. ^a CONICA was fitted with a new detector in June 2004. ^b The noise is that measured in the resulting co-added image, scaled to a 1 sec integration. Its statistical properties closely follow a Gaussian distribution with additional weak wings. ^c " $\theta _0$ '' refers to the isoplanatic angle in $K_{\rm s}$ band as measured fitting the variation of the Strehl ratio of the point sources in the fields as described in the text.
Table 2: Differential number counts in the SWAN fields. The raw number of detected galaxies is reported in (2). In (3) the corrected number counts ( $\textrm {N}\ \textrm {mag}^{-1}\ \textrm {deg}^{-2}$ ) for the whole sample are shown, while (4) and (5) separate late-type and early-type counts, respectively.