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Table C.1
Comparison with data from the literature, as reported by Baan et al. (2008) (B08), and this work (EMIR). Exact references for the observations can be found in Table B.1 in Baan et al. (2008). Differences (in %) between B08 and EMIR line intensity ratios are shown in column Δ%.
| Galaxy | HCN 1–0 | HNC 1–0 | HCO+ 1–0 | HNC/HCN | HCO+/HCN | |||||||
| [Jy km s-1] | [Jy km s-1] | [Jy km s-1] | ||||||||||
|
|
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| B08 | EMIR | B08 | EMIR | B08 | EMIR | B08 | EMIR | Δ% | B08 | EMIR | Δ% | |
| NGC 1068 | 158 | 130 | 61.9 | 52.4 | 143 | 86.6 | 0.39 | 0.40 | 3 | 0.91 | 0.67 | 26 |
| NGC 660 | 33 | 28.3 | 18.9 | 14.7 | 32.8 | 29.5 | 0.57 | 0.52 | 9 | 0.99 | 1.04 | 5 |
| Mrk 231 | 17.6 | 11.2 | 12.1 | 4.24 | 12.6 | 6.3 | 0.69 | 0.38 | 45 | 0.72 | 0.56 | 21 |
| NGC 6240 | 31.2 | 16.4 | 8 | 3.24 | 23.4 | 26.7 | 0.26 | 0.2 | 23 | 0.75 | 1.63 | 117 |
| NGC 1614 | 7.2 | 4.83 | – | 1.59 | – | 8.84 | – | 0.33 | – | – | 1.83 | – |
| UGC 5101 | 10.4 | 6.48 | – | 5.3 | – | 2.36 | – | 0.82 | – | – | 0.36 | – |
| NGC 3079 | 43.1 | 24.6 | 32.3 | 6.54 | – | 27.7 | 0.75 | 0.27 | 65 | – | 1.12 | – |
| NGC 3556 | 16.8 | 3.18 | – | 1.18 | – | 5.01 | – | 0.37 | – | – | 1.57 | – |
| NGC 7469 | 10.8 | 11.8 | 17 | 6.48 | 15.8 | 13.2 | 1.57 | 0.55 | 65 | 1.46 | 1.12 | 23 |
| NGC 7771 | 22.7 | 21.2 | – | 9.42 | 21.5 | 20 | – | 0.44 | – | 0.95 | 0.94 | 0.3 |
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