Table 2
Photometry in the 11 photometric bands.
| #ID | U | B | V | R | i 775 | z 850 | H 160 | m3.6 | m4.5 | m5.8 | m8.0 |
|
|
|||||||||||
| 1 | >26.8 | >27.2 | 27.00 ± 0.15 | 24.65 ± 0.06 | 23.40 ± 0.03 | 22.44 ± 0.02 | 19.25 ± 0.01 | 16.79 ± 0.02 | 16.48 ± 0.02 | 16.13 ± 0.05 | 15.84 ± 0.07 |
| 2 | >26.8 | >27.2 | 25.88 ± 0.14 | 23.92 ± 0.06 | 22.73 ± 0.02 | 21.66 ± 0.01 | 19.01 ± 0.01 | 16.52 ± 0.10 | 16.22 ± 0.10 | 16.12 ± 0.15 | 15.68 ± 0.26 |
| 3 | >26.8 | >27.2 | 26.65 ± 0.15 | 24.93 ± 0.07 | 23.10 ± 0.01 | 21.96 ± 0.02 | 19.68 ± 0.01 | 17.29 ± 0.02 | 16.97 ± 0.02 | 16.84 ± 0.08 | 16.24 ± 0.09 |
| 4 | >26.8 | >27.2 | 25.65 ± 0.09 | 23.76 ± 0.06 | 22.41 ± 0.02 | 21.23 ± 0.01 | 18.86 ± 0.01 | 16.03 ± 0.01 | 15.70 ± 0.02 | 15.70 ± 0.06 | 15.45 ± 0.06 |
| 5 | >26.8 | 28.4 ± 0.4 | 26.17 ± 0.10 | 24.74 ± 0.10 | 23.47 ± 0.01 | 22.33 ± 0.01 | 19.93 ± 0.04 | 17.35 ± 0.11 | 17.04 ± 0.15 | 17.33 ± 0.25 | 16.63 ± 0.25 |
| 606 | >26.8 | >27.2 | 27.25 ± 0.27 | 25.39 ± 0.12 | 23.62 ± 0.02 | 22.53 ± 0.01 | 20.13 ± 0.01 | 17.56 ± 0.02 | 17.20 ± 0.02 | 17.13 ± 0.11 | 16.41 ± 0.10 |
| 590 | >26.8 | >27.2 | 26.06 ± 0.15 | 24.79 ± 0.06 | 23.72 ± 0.02 | 22.67 ± 0.01 | 20.14 ± 0.01 | 17.40 ± 0.03 | 17.03 ± 0.02 | 17.16 ± 0.09 | 16.34 ± 0.10 |
| 568 | >26.8 | >27.2 | >28.10 ± 99.0 | >26.70 ± 99.0 | 24.12 ± 0.02 | 23.05 ± 0.01 | 20.51 ± 0.01 | 18.23 ± 0.02 | 17.90 ± 0.03 | 18.18 ± 0.15 | 17.96 ± 0.23 |
| 719 | >26.8 | >27.2 | >28.10 ± 99.0 | 25.26 ± 0.16 | 24.35 ± 0.03 | 23.23 ± 0.01 | 20.53 ± 0.02 | 17.68 ± 0.02 | 17.33 ± 0.03 | 17.48 ± 0.13 | 16.92 ± 0.14 |
| 1250 | >26.8 | >27.2 | 27.87 ± 0.43 | >26.70 ± 99.0 | 24.55 ± 0.04 | 23.46 ± 0.02 | 21.09 ± 0.02 | 18.61 ± 0.03 | 18.30 ± 0.04 | 17.90 ± 0.12 | 17.58 ± 0.16 |
| 1260 | >26.8 | >27.2 | >28.10 ± 99.0 | >26.70 ± 99.0 | 24.66 ± 0.04 | 23.61 ± 0.02 | 21.92 ± 0.02 | 19.44 ± 0.12 | 19.14 ± 0.13 | 19.04 ± 0.22 | 18.60 ± 0.36 |
| 173 | >26.8 | >27.2 | >28.10 ± 99.0 | 26.83 ± 0.18 | 24.96 ± 0.03 | 23.92 ± 0.02 | 21.12 ± 0.03 | 18.67 ± 0.02 | 18.39 ± 0.05 | 17.23 ± 0.15 | 17.58 ± 0.23 |
| 1160 | >26.8 | >27.2 | >28.10 ± 99.0 | >26.70 ± 99.0 | 23.97 ± 0.03 | 22.96 ± 0.02 | 20.56 ± 0.02 | 17.54 ± 0.02 | 17.33 ± 0.03 | 17.53 ± 0.13 | 16.71 ± 0.11 |
| 657 | >26.8 | 28.4 ± 0.4 | 26.17 ± 0.10 | 24.74 ± 0.10 | 23.45 ± 0.01 | 22.32 ± 0.01 | 19.93 ± 0.04 | 17.35 ± 0.14 | 17.04 ± 0.15 | 17.33 ± 0.25 | 16.63 ± 0.25 |
| 626 | >26.8 | 28.4 ± 0.4 | 26.17 ± 0.10 | 24.74 ± 0.10 | 23.49 ± 0.02 | 22.36 ± 0.01 | 19.93 ± 0.04 | 17.35 ± 0.14 | 17.04 ± 0.15 | 17.33 ± 0.25 | 16.63 ± 0.25 |
| 471 | >26.8 | >27.2 | >28.10 ± 99.0 | >26.70 ± 99.0 | 24.79 ± 0.05 | 23.78 ± 0.03 | – | 19.22 ± 0.05 | 19.01 ± 0.06 | 18.40 ± 0.22 | 99.00 ± 99.00 |
Notes. U,B,V and R magnitudes for each galaxy in the sample come from the data obtained at the Large Binocular Telescope (LBT); i775, z850, and H160 from the HST archival ACS and NICMOS-NIC3 data in the F775W,F850LP, and F160W filters respectively; m3.6, m4.5, m5.8 and m8.0 from the Spitzer archival images in the corresponding filters. Photometric errors were calculated by quadratically summing to the Sextractor statistical errors the uncertainty in the photometric calibration (0.04 mag) dominant in the ground-based data and the true sky noise variations computed within apertures across the images in space-based data to account for the smoothed noise resulting from the alignment and subpixel shifting procedures (~0.008 mag for HST; from 0.01 mag to more than 0.05 mag for Spitzer).
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