Table B.1.
Detected lines.
| Source | νObs | Line | νRest | Flux |
|---|---|---|---|---|
| (GHz) | (GHz) | (Jy km s−1) | ||
| III Zw 035 | 112.21 | CO(1-0) | 115.27 | 70.6 |
| III Zw 035 | 110.45 | CN N=1-0 | 113.49 m | 5.8 |
| III Zw 035 | 110.15 | CN N=1-0 | 113.19 m | 2.7 |
| IRAS F05189−2524 | 110.54 | CO(1-0) | 115.27 | 25.7 |
| IRAS F05189−2524 | 108.83 | CN N=1-0 | 113.49 m | 4.4 |
| IRAS F05189−2524 | 108.52 | CN N=1-0 | 113.19 m | 2.3 |
| IRAS F05189−2524 | 95.96 | HC3N 11−10 | 100.08 | 0.5 |
| NGC 2623 | 113.18 | CO(1-0) | 115.27 | 161.0 |
| NGC 2623 | 111.44 | CN N=1-0 | 113.49 m | 8.5 |
| NGC 2623 | 111.13 | CN N=1-0 | 113.19 m | 4.9 |
| IRAS F09111−1007 W | 109.33 | CO(1-0) | 115.27 | 51.0 |
| IRAS F09111−1007 W | 107.64 | CN N=1-0 | 113.49 m | 4.0 |
| IRAS F09111−1007 W | 107.33 | CN N=1-0 | 113.19 m | 2.6 |
| IRAS F09111−1107 W | 94.92 | HC3N 11−10 | 100.08 | 0.3 |
| IRAS F09111−1007 E | 109.28 | CO(1-0) | 115.27 | 19.7 |
| IRAS F10173+0828 | 109.89 | CO(1-0) | 115.27 | 24.2 |
| IRAS F10173+0828 | 108.19 | CN N=1-0 | 113.49 m | 1.4 |
| IRAS F10173+0828 | 107.89 | CN N=1-0 | 113.19 m | 0.7 |
| IRAS F10173+0828 | 95.41 | HC3N 11−10 | 100.08 | 0.7 |
| IRAS F12224−0624 | 112.30 | CO(1-0) | 115.27 | 22.6 |
| IRAS F12224−0624 | 110.56 | CN N=1-0 | 113.49 m | 2.0 |
| IRAS F12224−0624 | 110.25 | CN N=1-0 | 113.19 m | 1.1 |
| IRAS F12224−0624 | 98.02 | ? | 100.62 m | 0.4 |
| IRAS F12224−0624 | 97.50 | HC3N 11−10 | 100.08 | 0.8 |
| NGC 4418 | 114.47 | CO(1-0) | 115.27 | 117.0 |
| NGC 4418 | 112.70 | CN N=1-0 | 113.49 | 10.5 |
| NGC 4418 | 112.38 | CN N=1-0 | 113.19 | 4.6 |
| NGC 4418 | 101.81 | CH3CCH | 102.54 | 0.7 |
| IC 860 | 113.80 | CO(1-0) | 115.27 | 73.1 |
| IC 860 | 112.05 | CN N=1-0 | 113.49 m | 4.6 |
| IRAS 13120−5453 | 111.80 | CO(1-0) | 115.27 | 234.0 |
| IRAS 13120−5453 | 110.07 | CN N=1-0 | 113.49 m | 24.6 |
| IRAS 13120−5453 | 109.75 | CN N=1-0 | 113.19 m | 14.6 |
| IRAS 13120−5453 | 97.58 | ? | 100.61 m | 0.8 |
| IRAS 13120−5453 | 97.08 | HC3N 11−10 | 100.08 | 1.0 |
| IRAS F14378−3651 | 107.92 | CO(1-0) | 115.27 | 24.7 |
| IRAS F14378−3651 | 106.26 | CN N=1-0 | 113.49 m | 2.4 |
| IRAS F14378−3651 | 105.95 | CN N=1-0 | 113.19 m | 1.3 |
| IRAS F17207−0014 | 110.54 | CO(1-0) | 115.27 | 171.0 |
| IRAS F17207−0014 | 108.83 | CN N=1-0 | 113.49 m | 10.0 |
| IRAS F17207−0014 | 108.53 | CN N=1-0 | 113.19 m | 4.5 |
| IRAS F17207−0014 | 98.33 | CH3CCH | 102.54 | 0.2 |
| IRAS F17207−0014 | 96.50 | ? | 100.63 m | 0.5 |
| IRAS F17207−0014 | 95.97 | HC3N 11−10 | 100.08 | 2.9 |
| IRAS F20551−4250 | 110.52 | CO(1-0) | 115.27 | 54.9 |
| IRAS F20551−4250 | 108.82 | CN N=1-0 | 113.49 | 2.3 |
| IRAS F20551−4250 | 108.50 | CN N=1-0 | 113.19 | 1.0 |
| NGC 7479 (30″) | 114.39 | CO(1-0) | 115.27 | 270.0 |
| NGC 7479 (30″) | 112.60 | CN N=1-0 | 113.49 m | 6.4 |
Notes. Total fluxes, or fluxes in the indicated aperture diameter, for lines detected in the spectral ranges covered by NOEMA and ALMA. For the very rich spectrum of NGC 4418 we list only a few bright lines that are also detected in other targets. The listed frequencies are indicative for identification purposes only, in particular for lines with multiple components marked “m”.
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