Table 6.
on a pixel-by-pixel basis and on a spaxel-by-spaxel basis.
| Spectrally integrated (pixel-by-pixel basis) |
Spectrally resolved (spaxel-by-spaxel basis) |
||||||||
|---|---|---|---|---|---|---|---|---|---|
| ID | Galaxy | Mean | 25th–50th–75th (IQR) | 90th | Mean | 25th–50th–75th (IQR) | 90th | ||
| 1 | IRAS 17208−0014 | 1.253 | 1.012–1.224–1.513 (0.501) | 1.689 | 1.517 | 1.147–1.447–1.812 (0.664) | 2.173 | ||
| 2 | IRAS 09022−3615 | 0.561 | 0.433–0.539–0.648 (0.215) | 0.788 | 0.641 | 0.482–0.607–0.754 (0.272) | 0.928 | ||
| 3 | IRAS 13120−5453 | 1.395 | 1.056–1.301–1.609 (0.553) | 2.109 | 1.590 | 1.046–1.440–2.024 (0.977) | 2.560 | ||
| 4 | IRAS F14378−365 | 1.129 | 1.004–1.154–1.255 (0.251) | 1.355 | 1.169 | 0.980–1.142–1.305 (0.325) | 1.507 | ||
| 5 | IRAS F05189−252 | 1.452 | 1.246–1.524–1.633 (0.387) | 1.752 | 1.589 | 1.409–1.547–1.717 (0.308) | 2.022 | ||
| 6 | IRAS F10565+244 | 0.801 | 0.667–0.792–0.918 (0.251) | 1.068 | 0.871 | 0.660–0.825–1.023 (0.364) | 1.258 | ||
| 7 | IRAS 19542+1110 | 1.718 | 1.532–1.736–1.873 (0.342) | 2.127 | 1.724 | 1.544–1.697–1.848 (0.304) | 2.124 | ||
| 8 | ESO 148−IG002 | 0.402 | 0.345–0.394–0.437 (0.093) | 0.510 | 0.442 | 0.377–0.424–0.478 (0.101) | 0.544 | ||
| 9 | NGC 6240 | 0.674 | 0.613–0.679–0.736 (0.123) | 0.792 | 0.748 | 0.635–0.736–0.835 (0.200) | 0.954 | ||
| 10 | IRAS F17138-101 | 0.767 | 0.591–0.698–0.886 (0.295) | 1.076 | 0.815 | 0.675–0.802–0.939 (0.264) | 1.060 | ||
| 11 | IRAS 17578−0400 (a) | 1.208 | 1.038–1.215–1.336 (0.298) | 1.514 | 1.237 | 1.081–1.238–1.383 (0.302) | 1.513 | ||
| 12 | ESO 173−G015 | 0.792 | 0.685–0.783–0.884 (0.199) | 1.004 | 0.858 | 0.694–0.830–0.979 (0.285) | 1.143 | ||
| 13 | UGC 11763 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ||
| 14 | NGC 3110 | 1.289 | 1.032–1.176–1.538 (0.506) | 1.802 | 1.147 | 0.932–1.090–1.324 (0.392) | 1.572 | ||
| 15 | IC 4734 | 1.053 | 0.957–1.046–1.121 (0.164) | 1.222 | 1.042 | 0.905–1.024–1.159 (0.254) | 1.319 | ||
| 16 | NGC 5135 | 1.237 | 1.029–1.189–1.405 (0.376) | 1.677 | 1.105 | 0.850–1.038–1.280 (0.430) | 1.594 | ||
| 17 | ESO 221−IG10 | 0.792 | 0.656–0.772–0.906 (0.250) | 1.034 | 0.755 | 0.596–0.715–0.886 (0.290) | 1.054 | ||
| 18 | IC 5179 | 0.985 | 0.804–0.980–1.145 (0.341) | 1.357 | 0.887 | 0.698–0.865–1.054 (0.357) | 1.227 | ||
| 19 | UGC 2982 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ||
| 20 | NGC 2369 | 1.100 | 0.876–1.049–1.294 (0.418) | 1.517 | 1.133 | 0.841–1.055–1.343 (0.502) | 1.663 | ||
| 21 | ESO 286−G035 | 0.778 | 0.680–0.755–0.854 (0.174) | 0.960 | 0.790 | 0.638–0.758–0.922 (0.284) | 1.072 | ||
| 22 | ESO 320−G030 | 2.068 | 1.647–2.073–2.336 (0.689) | 2.791 | 2.156 | 1.735–2.064–2.450 (0.716) | 2.998 | ||
| 23 | NGC 5734 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ||
| Average (excl. 13, 19, 23) | 1.073 | 0.895–1.054–1.216 (0.321) | 1.407 | 1.111 | 0.896–1.067–1.276 (0.380) | 1.514 | |||
Notes. We examined pixels and spaxels within the global aperture (see Sect. 4.1) and within the velocity range listed in Table 3. For pixel-by-pixel analysis, we first performed a spectral integration followed by a 3σ threshold clipping. Each pixel has a size of 0.05″ × 0.05″. In the spaxel-by-spaxel analysis, we focused solely on spaxels where HCN and HCO+ were both detected with > 3σ significance. Each spaxel has a size of 0.05″ × 0.05″ × 20 km s−1. We note that pixels and spaxels within a beam are correlated. IQR stands for the interquartile range.
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