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Table 1.

Host galaxy properties.

Galaxy d i PA M*gal SFRgal M mol gal Mathematical equation: $ M_{\mathrm{mol}}^{\mathrm{gal}} $ M H I gal Mathematical equation: $ M_\mathrm{H{\small { {\text{ I}}}}}^{\mathrm{gal}} $
[Mpc] [°] [°] [109M] [M/yr] [109M] [109M]
(1) (2) (3) (4) (5) (6) (7) (8)
NGC 1097 13.6 ± 2.0 48.6 ± 6.0 122.4 ± 3.6 57 ± 15 4.7 ± 1.2 5.52 ± 0.01 4.1 ± 1.0
NGC 1300 19.0 ± 2.9 31.8 ± 6.0 278.0 ± 1.0 41 ± 11 1.17 ± 0.30 2.51 ± 0.02 2.4 ± 0.6
NGC 1365 19.6 ± 0.8 55.4 ± 6.0 201.1 ± 7.5 98 ± 25 17 ± 4 18.07 ± 0.05 8.7 ± 2.3
NGC 1433 18.6 ± 1.9 28.6 ± 6.0 199.7 ± 0.3 73 ± 19 1.13 ± 0.29 1.97 ± 0.01 2.51 ± 0.7
NGC 1512 18.8 ± 1.9 42.5 ± 6.0 261.9 ± 4.2 52 ± 13 1.28 ± 0.33 1.33 ± 0.02 7.6 ± 2.0
NGC 1566 17.7 ± 2.0 29.5 ± 10.6 214.7 ± 4.1 61 ± 16 4.5 ± 1.2 5.05 ± 0.01 6.4 ± 1.7
NGC 1672 19.4 ± 2.9 42.6 ± 12.9 134.3 ± 0.4 54 ± 14 7.6 ± 2.0 7.24 ± 0.02 16.0 ± 4.2
NGC 2566 23.4 ± 3.5 48.5 ± 6.0 312.0 ± 2.0 51 ± 13 8.7 ± 2.3 7.17 ± 0.02 2.4 ± 0.6
NGC 2903 10.0 ± 2.5 66.8 ± 3.1 203.7 ± 2.0 43 ± 11 3.1 ± 0.8 3.735 ± 0.005 3.4 ± 0.9
NGC 2997 14.1 ± 2.8 33.0 ± 9.0 108.1 ± 0.7 54 ± 14 4.4 ± 1.1 6.786 ± 0.009 7.2 ± 1.9
NGC 3351 9.96 ± 0.33 45.1 ± 6.0 193.2 ± 2.0 23 ± 6 1.32 ± 0.34 1.23 ± 0.01 0.85 ± 0.22
NGC 3489 11.9 ± 1.6 63.7 ± 5.0 70.0 ± 10.0 19 ± 5 0.023 ± 0.006 0.048 ± 0.001 0.025 ± 0.007
NGC 4303 17.0 ± 3.0 23.5 ± 9.2 312.4 ± 2.5 33 ± 9 5.3 ± 1.4 8.12 ± 0.02 4.6 ± 1.2
NGC 4321 15.2 ± 0.5 38.5 ± 2.4 156.2 ± 1.7 56 ± 14 3.6 ± 0.9 7.77 ± 0.02 2.7 ± 0.7
NGC 4459 15.9 ± 2.2 47.0 ± 5.0 108.75 ± 10.0 48 ± 12 0.22 ± 0.06 0.264 ± 0.003
NGC 4476 17.5 ± 2.4 60.1 ± 5.0 27.4 ± 10.0 6.5 ± 1.7 0.04 ± 0.01 0.071 ± 0.002
NGC 4477 15.8 ± 2.4 33.5 ± 5.0 25.7 ± 10.0 39 ± 10 0.08 ± 0.02 0.038 ± 0.002
NGC 5236 4.90 ± 0.18 24.0 ± 5.0 225.0 ± 10.0 34 ± 9 4.2 ± 1.1 2.8 ± 0.2 9.5 ± 2.5
NGC 5248 14.9 ± 1.3 47.4 ± 16.3 109.2 ± 3.5 25 ± 7 2.3 ± 0.6 4.541 ± 0.007 3.2 ± 0.8
NGC 7743 20.3 ± 2.8 37.1 ± 5.0 86.2 ± 10.0 23 ± 6 0.21 ± 0.06 0.360 ± 0.005 0.31 ± 0.08

Notes. The host properties were compiled by Leroy et al. (2021b). Col. 2: galaxy distance and its error based on the distance determination method from Anand et al. (2021). Cols. 3 and 4 (Lang et al. 2020 or Makarov et al. 2014): the inclination and position angle in the stellar mass. Col. 5 (Leroy et al. 2021b): its error in the SFR. Col. 6 (Calzetti et al. 2007; Leroy et al. 2019, 2021b; Belfiore et al. 2023): its error in the molecular gas mass. Col. 7: its error, with values are taken from the PHANGS sample table released together with the ALMA data products described in Leroy et al. (2021b). They include aperture corrections and adopt a varying metallicity-dependent, αCO. The uncertainties include statistical errors only, thus appearing smaller than the conservatively estimated errors on the ring molecular gas mass.). Col. 8 (Leroy et al. 2021b): the atomic gas mass and its error. Here “-” indicates that no data for the H I mass were available from Leroy et al. (2021b).

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