Table 3.
VLA observations: sky-plane HCN and HCO+ luminosities, and the rest-frame 88 GHz continuum.
| Galaxy |  |
 |
 |
 |
 |
 |
S88 GHz |
|---|---|---|---|---|---|---|---|
| [L⊙] | [K km s−1 pc2] | [L⊙] | [K km s−1 pc2] | [L⊙] | [K km s−1 pc2] | [μJy] | |
| SDP.81 | ≤8.2 × 105 | ≤3.7 × 1010 | ≤7.2 × 105 | ≤4.2 × 1010 | ≤4.3 × 105 | ≤2.4 × 1010 | 170 ± 2 |
| SDP.130 | ≤3.1 × 105 | ≤1.4 × 1010 | ≤2.2 × 105 | ≤1.3 × 1010 | ≤3.0 × 105 | ≤1.6 × 1010 | 21 ± 1.4 |
| HXMM.02 | ≤8.6 × 105 | ≤5.1 × 1010 | ≤9.8 × 105 | ≤5.7 × 1010 | ≤15 × 105 | ≤8.3 × 1010 | 31 ± 3 |
| J0209 | ≤23 × 105 | ≤10 × 1010 | ≤29 × 105 | ≤13 × 1010 | ≤19 × 105 | ≤1.1 × 1010 | 266 ± 28 |
| J1202 | (18 ± 9) × 105 | (8 ± 4) × 1010 | ≤9.5 × 105 | ≤4.2 × 1010 | ≤10 × 105 | ≤5.7 × 1010 | 177 ± 16 |
| J1609 | ≤10 × 105 | ≤11.4 × 1010 | (12 ± 7) × 105 | (7 ± 4) × 1010 | ≤20 × 105 | ≤5.8 × 1010 | 293 ± 10 |
Notes. Upper limits are set at 3σ level. The HCN(1–0) detection in J1202 and the tentative HCO+(1–0) detection in J1609 are marked in bold; the quoted uncertainties are for the D = 10″ circular aperture. Upper limits on additional emission lines are listed in Appendix A.
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