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Table 2
Mid- and far-infrared properties of our combined sample.
| Galaxy | S 24 |
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| μJy | mJy | mJy | mJy | mJy | mJy | mJy | mJy | mJy | mJy | mJy | mJy | |
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| PEPJ123712+621753 | 153 ± 5 | <2.0 | 2.6 ± 0.3 | 3.5 ± 0.7 | 6.2 ± 2.5 | <9.0 | <12.0 | ... | <1.7 | ... | ... | ... |
| PEPJ123709+621507 | 128 ± 6 | <2.0 | 2.1 ± 0.4 | 3.0 ± 1.3 | 8.0 ± 2.5 | <9.0 | <12.0 | ... | <1.6 | ... | ... | ... |
| PEPJ123759+621732 | 217 ± 7 | <2.4 | 1.2 ± 0.4 | 5.3 ± 1.7 | 10.0 ± 2.5 | <9.0 | <12.0 | ... | <2.1 | ... | ... | ... |
| PEPJ123721+621346 | 238 ± 8 | 1.8 ± 0.6 | 3.1 ± 0.3 | 8.5 ± 0.8 | 14.5 ± 2.5 | 10.8 ± 3.0 | 8.0 ± 5.0 | ... | <1.6 | ... | ... | ... |
| PEPJ123615+621008 | 327 ± 7 | 4.5 ± 0.6 | 4.3 ± 0.4 | 9.2 ± 1.0 | 15.9 ± 3.1 | 14.3 ± 3.0 | <12.0 | ... | <1.7 | ... | ... | ... |
| PEPJ123634+620627 | 108 ± 9 | <2.0 | 7.1 ± 0.4 | 13.4 ± 1.2 | 18.1 ± 4.0 | 16.1 ± 3.0 | 15.1 ± 4.0 | ... | <2.0 | ... | ... | ... |
| PEPJ123633+621005 | 572 ± 7 | 2.7 ± 0.6 | 8.5 ± 0.3 | 16.3 ± 1.0 | 20.2 ± 2.5 | 13.0 ± 3.0 | <12.0 | ... | <1.6 | ... | ... | ... |
| PEPJ123646+621141 | 300 ± 6 | <2.0 | 2.9 ± 0.3 | 5.8 ± 0.7 | 12.7 ± 2.5 | 10.7 ± 3.0 | <12.0 | ... | <1.7 | ... | ... | ... |
| PEPJ123750+621600 | 188 ± 6 | <2.0 | 1.7 ± 0.3 | 4.8 ± 1.1 | 8.6 ± 2.5 | 8.8 ± 3.0 | <12.0 | ... | <1.8 | ... | ... | ... |
| HDF169 | 445 ± 7 | 13.2 ± 0.7 | 34.2 ± 0.6 | 63.2 ± 1.6 | 62.5 ± 3.7 | 47.1 ± 3.0 | 19.6 ± 4.0 | 2.2 ± 0.8 | <1.8 | ... | ... | ... |
| BzK-4171 | 140 ± 6 | <3.2 | 2.9 ± 0.3 | 9.0 ± 1.0 | 14.5 ± 2.5 | <9.0 | <12.0 | ... | <1.7 | ... | ... | ... |
| BzK-21000 | 382 ± 6 | 4.9 ± 0.7 | 8.1 ± 0.6 | 15.1 ± 1.4 | 24.4 ± 2.5 | 20.1 ± 4.7 | 11.6 ± 7.4 | ... | <2.2 | 0.32 ± 0.15 | 0.04 ± 0.06 | |
| BzK-16000 | 190 ± 6 | <2.0 | 1.6 ± 0.6 | 3.7 ± 0.9 | 9.2 ± 2.5 | <9.0 | <12.0 | ... | <1.7 | ... | ... | ... |
| BzK-17999 | 229 ± 8 | <2.0 | 4.1 ± 0.5 | 10.8 ± 1.4 | 14.7 ± 2.5 | 11.2 ± 3.0 | <12.0 | ... | <1.8 | ... | ... | ... |
| BzK-12591 | 377 ± 6 | <3.3 | 9.8 ± 0.4 | 18.3 ± 1.1 | 24.9 ± 2.5 | 20.5 ± 3.0 | 9.9 ± 4.0 | ... | <1.7 | ... | ... | ... |
| HDF242 | 255 ± 9 | <2.0 | 1.1 ± 0.3 | 6.4 ± 1.3 | 23.9 ± 4.6 | 28.3 ± 6.4 | 23.8 ± 4.0 | 8.0 ± 3.1 | <1.6 | ... | ... | ... |
| GN20 | 68 ± 4 | <2.0 | 0.7 ± 0.4 | 5.4 ± 1.0 | 18.6 ± 2.7 | 41.3 ± 5.2 | 39.7 ± 6.1 | 20.3 ± 2.0 | 10.5 ± 0.7 | 0.9 ± 0.15 | 0.33 ± 0.06 | 0.027 ± 0.027 |
Notes. SXX correspond to flux densities at the observed wavelength XX in microns.
(b)
These flux densities are taken from Pope et al. (2006).
(c)
These flux densities are taken from Penner et al. (2011).
(d)
These flux densities are taken from Magdis et al. (2011).
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