Table E.2.
Galaxy centres vs discs.
| log10(Y) | environment | (16th, 50th, 84th) perc. (S/N ≥ 3) | median (all S/N) |
|---|---|---|---|
| HCN/CO | disc | ( − 1.96, −1.72, −1.51) | −1.87 |
| centre | ( − 1.60, −1.35, −1.04) | −1.35 | |
| centre (AGN) | ( − 1.43, −1.30, −1.03) | −1.28 | |
| centre (non-AGN) | ( − 1.62, −1.43, −1.22) | −1.43 | |
| SFR/HCN | disc | ( − 7.21, −6.93, −6.56) | −6.85 |
| centre | ( − 7.39, −7.13, −6.57) | −7.11 | |
| centre (AGN) | ( − 7.44, −7.19, −6.70) | −7.23 | |
| centre (non-AGN) | ( − 7.31, −7.11, −6.57) | −7.11 | |
Notes. – 16th percentiles, medians, and 84th percentiles of HCN/CO and SFR/HCN across significant data (S/N ≥ 3) in disc and centre environments. For the centres, we also present percentile values among centres with and without AGNs. The last column additionally lists the median values across all S/N data, this means including non-detections, which yields 0.15 dex lower HCN/CO and 0.08 dex higher SFR/HCN across galaxy discs, which are affected by S/N-clipping (and similar values in centres, which have S/N ≥ 3 for 29 out of 31 galaxies).
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