Table 1.
Properties of the MIR-selected sample.
| ID | RA | Dec | r | F24 | F8 | log LHα | log LFUV | log LNUV | R |
|---|---|---|---|---|---|---|---|---|---|
| ... | deg | deg | arcsec | mJy | mJy | erg s−1 | erg s−1 | erg s−1 | kpc |
| s537 | 23.6099 | 29.9906 | 1.8 | 1.29 ± 0.02 | 0.14 ± 0.02 | ... | ... | ... | 10.4 |
| s542 | 23.6651 | 30.0625 | 1.7 | 1.31 ± 0.02 | 0.48 ± 0.03 | ... | ... | ... | 10.0 |
| s555 | 23.2454 | 30.1715 | 1.8 | 1.07 ± 0.02 | 0.33 ± 0.03 | ... | ... | ... | 7.8 |
| s631 | 23.1010 | 30.4421 | 1.3 | 0.39 ± 0.02 | 0.35 ± 0.03 | ... | 36.6 | 36.3 | 7.9 |
| s672 | 23.8356 | 30.5626 | 1.6 | 0.83 ± 0.02 | 0.73 ± 0.04 | ... | ... | ... | 8.9 |
| s771 | 23.0613 | 30.7235 | 1.7 | 0.87 ± 0.02 | 0.49 ± 0.03 | ... | ... | ... | 9.2 |
| s787 | 23.8474 | 30.7463 | 2.0 | 2.62 ± 0.02 | ... ± ... | ... | ... | ... | 8.5 |
| s799 | 23.1572 | 30.7673 | 1.4 | 0.54 ± 0.01 | 0.33 ± 0.03 | 34.7 | 37.3 | 37.0 | 7.8 |
| s854 | 23.2726 | 30.9742 | 1.4 | 0.45 ± 0.01 | 0.26 ± 0.02 | ... | 36.8 | 36.9 | 7.7 |
| s892 | 23.7057 | 31.1582 | 1.4 | 0.45 ± 0.01 | 0.37 ± 0.03 | 35.7 | 37.8 | 37.5 | 8.1 |
| s905 | 23.6735 | 31.2885 | 1.9 | 2.77 ± 0.02 | 1.80 ± 0.06 | ... | ... | ... | 10.1 |
| s907 | 23.4811 | 31.3279 | 2.0 | 1.94 ± 0.02 | 0.43 ± 0.03 | ... | ... | ... | 9.8 |
Notes. The identification number of each source in the MIR-selected sample is listed in Col. 1, and the relative celestial coordinates are presented in Cols. 2 and 3. The estimated source radius is given in Col. 4 and the flux at 24 μm in Col. 5. The 8 μm flux is listed in Col. 6, and the source luminosity in the Hα line and in the near and far continuum UV are given in Cols. 7–9, respectively. In the last column we show the source galactocentric distance.
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