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Table C.1.

Other properties of combined sample.

Source DL log(Mout) tflow Ṁout log(Pkin) log(Ṁoutv) log(ΣFIR) log(LBol) log(LAGN) Ref. (AGN)
(Mpc) (M⊙) (Myr) (M⊙ yr−1) (erg s−1) (g cm s−2) (L⊙ kpc−2) (L⊙) (L⊙)
NGC 253 3.40 7.20 4.30 3.71 39.47 33.07 12.14 10.58 <7.07 Cicone et al. (2014)
I Zw 1 273.98 <7.62 10.87 12.01 11.96 Veilleux et al. (2013)
III Zw 035 119.91 8.59 6.88 56.70 42.24 35.05 11.81 11.71 <7.76 González-Martín et al. (2015)
PG 0157+001 781.80 7.99 1.54 63.81 42.51 35.21 > 11.18 12.68 12.50 Veilleux et al. (2013)
NGC 1068 14.40 6.93 1.02 8.27 40.42 33.72 11.36 11.37 10.15 Ricci et al. (2017)
NGC 1266 29.90 7.67 1.21 38.31 42.10 34.89 > 11.89 10.54 9.73 Cicone et al. (2014)
IRAS F03158+4227 632.90 8.88 6.92 110.83 43.43 35.79 12.68 12.36 Fluetsch et al. (2019)
NGC 1377 21.00 6.88 1.42 5.36 40.51 33.67 > 11.49 10.09 9.35 Cicone et al. (2014)
NGC 1433 9.90 5.82 0.94 0.70 39.34 32.64 9.24 8.32 Fluetsch et al. (2019)
NGC 1614 68.88 7.51 1.52 21.33 41.94 34.68 11.21 11.73 <8.94 Brightman & Nandra (2011)
IRAS F05081+7936 239.20 7.98 1.22 28.23 43.20 35.60 10.61 12.05 <8.79 Fluetsch et al. (2019)
IRAS F05189−2524 189.47 7.87 2.30 32.56 42.31 34.96 11.78 12.22 12.09 Veilleux et al. (2013)
NGC 2146 17.20 7.94 10.20 8.49 41.03 34.03 10.46 11.16 <7.51 Cicone et al. (2014)
NGC 2623 80.03 7.05 1.01 11.21 42.09 34.62 11.93 11.62 10.62 Evans et al. (2008)
NGC 2623 fossil 6.66 12.80 0.36 40.26 32.96
IRAS F08572+3915 260.32 8.56 1.00 363.80 43.87 36.26 11.73 12.20 12.06 Veilleux et al. (2013)
IRAS F09111−1007 W 242.11 8.01 1.81 57.12 42.29 35.08 11.64 12.01 <10.80 Nardini et al. (2010)
M 82 3.90 7.86 9.78 7.34 40.36 33.67 11.08 10.90 <7.96 Cicone et al. (2014)
IRAS F10035+4852 291.20 <8.45 12.06 <11.52 Fluetsch et al. (2019)
IRAS F10173+0828 217.64 <7.29 11.77 11.90 <8.18 Iwasawa et al. (2011)
NGC 3256 N 35.00 7.26 0.57 31.93 42.69 35.15 10.79 11.60 <8.39 Cicone et al. (2014)
NGC 3256 S 7.13 1.33 10.11 41.90 34.50
IRAS F10565+2448 190.70 8.34 2.39 91.90 42.77 35.42 11.54 12.12 11.79 Veilleux et al. (2013)
IRAS F11119+3257 920.20 8.75 6.85 81.43 43.41 35.71 12.72 12.63 Veilleux et al. (2013)
NGC 3628 7.70 6.98 4.46 2.13 39.74 33.08 11.13 10.08 <7.21 Cicone et al. (2014)
ESO 320−G030 46.60 6.81 2.36 2.76 41.00 33.77 11.28 11.33 <9.33 Alonso-Herrero et al. (2012)
IRAS F12112+0305 SW 330.34 7.53 2.31 14.62 41.68 34.47 12.38 11.64 Veilleux et al. (2013)
IRAS F12112+0305 NE 8.80 3.36 188.41 43.11 35.74
IRAS F12224−0624 115.71 6.95 0.46 19.42 42.29 34.84 11.83 11.35 <10.75 This work
NGC 4418 25.35 5.73 0.09 6.29 41.32 34.11 12.50 10.94 10.68 Veilleux et al. (2013)
Mrk 231 186.42 8.43 0.84 323.84 43.70 36.15 > 12.26 12.61 12.51 Veilleux et al. (2013)
IC 860 56.11 <6.55 12.07 11.19 <9.19 Alonso-Herrero et al. (2012)
IRAS 13120−5453 136.14 8.18 1.35 111.53 42.50 35.33 11.99 12.33 11.85 Veilleux et al. (2013)
Mrk 273 166.43 8.21 0.83 196.30 43.42 35.91 > 12.13 12.24 11.77 Veilleux et al. (2013)
4C 12.50 568.50 <8.11 12.41 12.11 Fluetsch et al. (2019)
SDSS J135646.10+102609.0 574.70 8.09 0.59 207.49 43.21 35.82 12.43 12.41 Sun et al. (2014)
IRAS F14348−1447 SW 375.26 8.76 3.80 151.34 42.92 35.60 12.42 11.66 Veilleux et al. (2013)
IRAS F14348−1447 NE 8.05 2.44 45.91 42.30 35.03
IRAS F14378−3651 306.70 <7.87 11.81 12.26 11.59 Veilleux et al. (2013)
Zw 049.057 56.40 6.96 0.26 35.09 42.00 34.82 11.90 11.26 <9.26 Alonso-Herrero et al. (2012)
Arp 220 78.70 7.02 0.19 54.93 42.40 35.12 12.53 12.24 11.01 Veilleux et al. (2013)
Mrk 876 605.21 9.38 3.31 720.05 44.40 36.68 10.70 12.30 12.17 Ricci et al. (2017)
NGC 6240 106.81 8.59 1.43 272.00 43.24 35.89 11.28 11.91 11.66 Veilleux et al. (2013)
IRAS F17020+4544 270.52 8.27 0.59 315.95 44.44 36.52 11.61 11.13 Giroletti et al. (2017)
IRAS F17132+5313 226.60 <8.16 12.00 8.70 Iwasawa et al. (2011)
IRAS F17207−0014 189.20 7.52 3.33 98.96 43.59 35.84 11.97 12.48 <11.18 Veilleux et al. (2013)
PDS 456 898.60 8.61 3.37 120.03 43.39 35.83 13.42 13.41 Bischetti et al. (2019)
NGC 6764 32.00 6.44 20.00 0.14 38.09 31.67 10.46 8.65 Cicone et al. (2014)
IRAS F20100−4156 608.20 8.86 2.43 295.08 43.90 36.24 12.73 12.16 Spoon et al. (2013)
IC 5063 48.71 7.23 0.90 18.61 42.17 34.77 10.24 10.92 10.84 Ricci et al. (2017)
IRAS F20551−4250 190.20 7.43 0.46 59.44 42.65 35.26 11.64 12.11 11.87 Veilleux et al. (2013)
IRAS F22491−1808 352.74 8.13 1.55 86.73 42.46 35.25 11.26 12.26 11.42 Veilleux et al. (2013)
NGC 7479 34.31 <6.22 11.31 10.89 9.95 Ricci et al. (2017)
IRAS F23060+0505 834.25 9.42 5.66 463.76 43.85 36.31 12.59 12.48 Cicone et al. (2014)
IRAS 23365+3604 289.17 8.12 2.67 49.46 42.50 35.15 11.65 12.27 11.92 Veilleux et al. (2013)

Notes. Molecular outflow masses, flow times, and outflow rates for the combined sample, as computed using the observed quantities from Tables 3 and 4. We also list adopted distances, far-infrared surface brightnesses (from Lutz et al. 2016, 2018), and bolometric and AGN luminosities. Some references quote AGN fractions to the bolometric luminosity which we have converted to LAGN for consistency. The limit for IRAS F12224−0624 was estimated from Spitzer-IRS data with methods as used by Veilleux et al. (2013). We note that AGN luminosities are a mixture of X-ray-based (reacting rapidly to accretion variations) and mid-infrared-based (averaging over typically tens of years).

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