Table 1.
Summary of the galactic parameters of our sample adopted through this work.
| Target | RA | Dec | log10M* | log10MH2 | log10SFR | ΔMS | Distance | Inclination | Mapped area |
|---|---|---|---|---|---|---|---|---|---|
| (°) | (°) | (M⊙) | (M⊙) | (M⊙ yr−1) | (dex) | (Mpc) | (°) | (kpc2) | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| NGC 1087 | 41.60492 | −0.498717 | 9.9 | 9.2 | 0.12 | 0.33 | 15.85 ± 2.08 | 42.9 | 128 |
| NGC 1300 ( • ) | 49.920815 | −19.411114 | 10.6 | 9.4 | 0.07 | −0.18 | 18.99 ± 2.67 | 31.8 | 366 |
| NGC 1365 | 53.40152 | −36.140404 | 11.0 | 10.3 | 1.23 | 0.72 | 19.57 ± 0.77 | 55.4 | 421 |
| NGC 1385 ( • ) | 54.369015 | −24.501162 | 10.0 | 9.2 | 0.32 | 0.5 | 17.22 ± 2.42 | 44.0 | 100 |
| NGC 1433 ( • ) | 55.506195 | −47.221943 | 10.9 | 9.3 | 0.05 | −0.36 | 18.63 ± 1.76 | 28.6 | 441 |
| NGC 1512 | 60.975574 | −43.348724 | 10.7 | 9.1 | 0.11 | −0.21 | 18.83 ± 1.78 | 42.5 | 270 |
| NGC 1566 ( • ) | 65.00159 | −54.93801 | 10.8 | 9.7 | 0.66 | 0.29 | 17.69 ± 1.91 | 29.5 | 212 |
| NGC 1672 | 71.42704 | −59.247257 | 10.7 | 9.9 | 0.88 | 0.56 | 19.4 ± 2.72 | 42.6 | 255 |
| NGC 2835 | 139.47044 | −22.35468 | 10.0 | 8.8 | 0.09 | 0.26 | 12.22 ± 0.9 | 41.3 | 88 |
| NGC 3351 | 160.99065 | 11.70367 | 10.4 | 9.1 | 0.12 | 0.05 | 9.96 ± 0.32 | 45.1 | 76 |
| NGC 3627 | 170.06252 | 12.9915 | 10.8 | 9.8 | 0.58 | 0.19 | 11.32 ± 0.47 | 57.3 | 87 |
| NGC 4254 ( • ) | 184.7068 | 14.416412 | 10.4 | 9.9 | 0.49 | 0.37 | 13.1 ± 1.87 | 34.4 | 174 |
| NGC 4303 ( • ) | 185.47888 | 4.473744 | 10.5 | 9.9 | 0.73 | 0.54 | 16.99 ± 2.78 | 23.5 | 220 |
| NGC 4321 ( • ) | 185.72887 | 15.822304 | 10.7 | 9.9 | 0.55 | 0.21 | 15.21 ± 0.49 | 38.5 | 196 |
| NGC 4535 ( • ) | 188.5846 | 8.197973 | 10.5 | 9.6 | 0.33 | 0.14 | 15.77 ± 0.36 | 44.7 | 126 |
| NGC 5068 | 199.72807 | −21.038744 | 9.4 | 8.4 | −0.56 | 0.02 | 5.2 ± 0.22 | 35.7 | 23 |
| NGC 7496 ( • ) | 347.44702 | −43.42785 | 10.0 | 9.3 | 0.35 | 0.53 | 18.72 ± 2.63 | 35.9 | 89 |
| IC5332 | 353.61453 | −36.10108 | 9.7 | − | −0.39 | 0.01 | 9.01 ± 0.39 | 26.9 | 34 |
Notes. ( • )Galaxies observed with MUSE-AO mode. Values in Cols. (4)–(6) correspond to those presented in Leroy et al. (in prep.). Column (7) shows the vertical offset of the galaxy from the integrated main sequence of galaxies, as defined in Leroy et al. (2019). Distance measurements are presented in Anand et al. (2021) and inclinations in Lang et al. (2020). Uncertainties in Cols. (4)–(7) are on the order of 0.1 dex. Column (10) shows the area mapped by MUSE.
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