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Table A.1
Properties of the PACS-detected LBGs at z ~ 3 studied in the present work.
| ID | RA [deg] | Dec [deg] | z phot | log (LIR/L⊙) | A1200 [mag] | SFRtotal [M⊙ yr-1] | log (M∗/M⊙) | UV slope |
|
|
||||||||
| GOODS-MUSIC 15985 | 53.15745 | –27.70906 | 2.71 | 12.7 | 5.3 | 894.6 | 8.5 | –1.50 |
| GOODS-MUSIC 2989 | 53.21566 | –27.88574 | 2.63 | 12.4 | 6.7 | 436.4 | 10.6 | –0.52 |
| GOODS-MUSIC 4742 | 53.22782 | –27.86125 | 2.69 | 12.7 | 5.9 | 970.4 | 11.6 | –0.74 |
| GOODS-MUSIC 7180 | 53.18829 | –27.82934 | 2.63 | 12.4 | 3.8 | 518.0 | 10.5 | –1.44 |
| GOODS-MUSIC 12229 | 53.09410 | –27.76094 | 3.05 | 12.7 | 7.7 | 987.3 | 10.4 | 0.17 |
| GOODS-MUSIC 14620 | 53.12506 | –27.72682 | 3.21 | 12.5 | 5.8 | 594.9 | 10.4 | –0.27 |
| GOODS-MUSIC 17602 | 53.16990 | –27.68388 | 2.77 | 12.5 | 5.3 | 567.2 | 11.4 | –1.14 |
| GOODS-MUSIC 17746 | 53.11330 | –27.68094 | 3.35 | 13.0 | 6.3 | 1732.1 | 10.8 | –0.08 |
| GOODS-MUSIC 70202 | 53.11884 | –27.78282 | 2.63 | 13.1 | 8.3 | 2022.2 | 11.3 | 0.121 |
| HDFN-1113 | 189.42146 | 62.20577 | 3.11 | 12.9 | 5.4 | 1197.1 | 10.5 | –0.66 |
| HDFN-1871 | 189.24800 | 62.37027 | 2.63 | 12.7 | 4.4 | 884.1 | 10.6 | –0.95 |
| HDFN-2128 | 189.43324 | 62.30835 | 2.54 | 12.6 | 5.8 | 689.9 | 11.3 | –0.99 |
| HDFN-923 | 189.39473 | 62.25430 | 4.00 | 12.7 | 5.4 | 970.2 | 11.7 | –1.06 |
| HDFN-1108 | 189.42360 | 62.20658 | 3.44 | 13.0 | 5.6 | 1910.9 | 11.6 | –1.39 |
| HDFN-1520 | 189.18370 | 62.21974 | 3.11 | 12.5 | 3.6 | 624.9 | 10.4 | –1.32 |
| HDFN-1700 | 188.91438 | 62.21230 | 3.11 | 12.6 | 5.4 | 720.5 | 10.6 | –0.33 |
Notes.We show the galaxy ID, sky position, photometric redshift, total IR luminosity, dust attenuation derived from the LIR/LUV ratio (Buat et al. 2005), UV+IR-derived SFR (Kennicutt 1998), stellar mass, and UV continuum slope.
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