All Tables

Table 1: Summary of observations for the seven analyzed fields. The mean seeing is estimated when faint stars were detected.
Table 2: Error estimates of the C-A classification. Fraction of misclassified objects for several magnitude ranges.
Table 3: GIM2D output for some objects. Left: original images, middle: GIM2D models, right: residuals. The small thumbnails show the real and the model galaxy. The image size is $1.7\hbox {$^\prime $ }\times 1.7\hbox {$^\prime $ }$
Table 4: Error analysis of the bulge fraction B/T for different recovered magnitude ranges and different bins in recovered galaxy size. The galaxy size is represented by the half-light radius and is distributed into 4 bins in $\log~(r_{\rm hl})$ . In the top left corner bright and small objects are found whereas faint and large objects are placed in the bottom right corner. $\overline {\Delta B/T}$ is the average difference between introduced and recovered values of B/T, while $\sigma \Delta B/T$ is the dispersion (see text for details). N is the number of simulations used for each bin.
Table 5: Morphological k correction: morphological differences when observing in the K and I-bands. The same objects observed in the K and I bands present different morphologies. The images size is $1.7\hbox {$^\prime $ }\times 1.7\hbox {$^\prime $ }$ .
Table 6: Summary of the morphological classifications for the 79 detected objects. For each object we show the I and K band magnitudes and the estimated morphological type from AO imaging in the K-band (with GIM2D and C-A) and from HST-ACS in the I-band. BD stands for bulge-dominated, DD for disk-dominated and I for irregular.