Table 2.
PAH, CO, and IR luminosities of the main-sequence (ASPECS) sample.
| ID_3 mm | RA | Dec | z | log(L(PAH7.7)/L⊙) |  |
log(L(IR)/L⊙) | AGN |
|---|---|---|---|---|---|---|---|
| 1 | 03:32:38.54 | −27:46:34.62 | 2.543 | 10.69 ± 0.03 | 10.51 ± 0.09 | 12.65 ± 0.03 | X-ray/IR |
| 2 | 03:32:42.38 | −27:47:07.92 | 1.317 | 9.82 ± 0.16 | 10.15 ± 0.07 | 11.50 ± 0.04 | − |
| 3 | 03:32:41.02 | −27:46:31.56 | 2.454 | 10.30 ± 0.17 | 10.21 ± 0.09 | 12.01 ± -0.04 | − |
| 4 | 03:32:34.44 | −27:46:59.82 | 1.414 | 10.41 ± 0.06 | 10.49 ± 0.07 | 11.99 ± 0.02 | − |
| 5 | 03:32:39.76 | −27:46:11.58 | 1.551 | 10.49 ± 0.10 | 10.44 ± 0.07 | 12.01 ± 0.04 | X-ray |
| 6 | 03:32:39.90 | −27:47:15.12 | 1.095 | 10.10 ± 0.04 | 10.01 ± 0.08 | 11.46 ± -0.01 | − |
| 7 | 03:32:43.53 | −27:46:39.47 | 2.696 | 10.70 ± 0.09 | 10.48 ± 0.15 | 12.44 ± -0.01 | − |
| 9 | 03:32:44.03 | −27:46:36.05 | 2.698 | 10.60 ± 0.15 | 10.11 ± 0.09 | 12.57 ± 0.07 | X-ray/IR |
| 10 | 03:32:42.98 | −27:46:50.45 | 1.037 | 10.11 ± 0.06 | 10.05 ± 0.08 | 11.69 ± 0.03 | − |
| 11 | 03:32:39.80 | −27:46:53.70 | 1.096 | 9.44 ± 0.32 | 9.53 ± 0.10 | 10.91 ± 0.10 | − |
| 12 | 03:32:36.21 | −27:46:27.78 | 2.574 | 10.16 ± 0.13 | 9.77 ± 0.10 | 11.54 ± -0.04 | X-ray |
| 14 | 03:32:34.84 | −27:46:40.74 | 1.098 | 9.97 ± 0.04 | 9.87 ± 0.09 | 11.46 ± -0.03 | − |
| 15 | 03:32:36.48 | −27:46:31.92 | 1.096 | 9.81 ± 0.05 | 9.65 ± 0.09 | 11.57 ± 0.01 | X-ray |
| 16 | 03:32:39.92 | −27:46:07.44 | 1.294 | 9.75 ± 0.19 | 9.37 ± 0.08 | 11.19 ± -0.05 | − |
Notes. Columns are, from left to right: ASPECS 3 mm ID, right ascension, declination, spectroscopic redshift, PAH 7.7 μm luminosity, CO(1–0) luminosity, total IR luminosity, and the AGN flag (X-ray, IR, or no AGN). Note that 3 mm.8 and 3 mm.13 are not included, the former because it is largely behind a foreground galaxy and the latter because it is at z > 3 and thus lacks the PAH coverage from MIRI.
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