Table 1.
Key properties of the PHANGS–MUSE sample of galaxies used in this work.
| Name | Distance | Log(M⋆) | Log(SFR) | ΔSFMS | R25 | PA | i | pc/″ | Survey areas | PSF | fDIG |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [Mpc] | [M⊙] | [M⊙ yr−1] | [dex] | [arcmin] | [deg] | [deg] | [kpc2] | [arcsec] | |||
| NGC 0628 | 9.8 | 10.34 | 0.24 | 0.18 | 4.9 | 20.7 | 8.9 | 47.7 | 89 | 0.73 |
0.45 |
| NGC 1087 | 15.9 | 9.93 | 0.12 | 0.33 | 1.5 | 359.1 | 42.9 | 76.8 | 126 | 0.74 |
0.38 |
| NGC 1300 | 19.0 | 10.62 | 0.07 | −0.18 | 3.0 | 278.0 | 31.8 | 92.1 | 356 | 0.63 |
0.52 |
| NGC 1365 | 19.6 | 10.99 | 1.23 | 0.72 | 6.0 | 201.1 | 55.4 | 94.9 | 409 | 0.82 |
0.19 |
| NGC 1385 | 17.2 | 9.98 | 0.32 | 0.50 | 1.7 | 181.3 | 44.0 | 83.5 | 101 | 0.49 |
0.30 |
| NGC 1433 | 18.6 | 10.87 | 0.05 | −0.36 | 3.1 | 199.7 | 28.6 | 90.3 | 426 | 0.65 |
0.53 |
| NGC 1512 | 18.8 | 10.71 | 0.11 | −0.21 | 4.2 | 261.9 | 42.5 | 91.3 | 266 | 0.80 |
0.48 |
| NGC 1566 | 17.7 | 10.78 | 0.66 | 0.29 | 3.6 | 214.7 | 29.5 | 85.8 | 208 | 0.64 |
0.33 |
| NGC 1672 | 19.4 | 10.73 | 0.88 | 0.56 | 3.1 | 134.3 | 42.6 | 94.1 | 250 | 0.72 |
0.23 |
| NGC 2835 | 12.2 | 10.00 | 0.09 | 0.26 | 3.2 | 1.0 | 41.3 | 59.2 | 87 | 0.85 |
0.43 |
| NGC 3351 | 10.0 | 10.36 | 0.12 | 0.05 | 3.6 | 193.2 | 45.1 | 48.3 | 73 | 0.74 |
0.30 |
| NGC 3627 | 11.3 | 10.83 | 0.58 | 0.19 | 5.1 | 173.1 | 57.3 | 54.9 | 85 | 0.77 |
0.32 |
| NGC 4254 | 13.1 | 10.42 | 0.49 | 0.37 | 2.5 | 68.1 | 34.4 | 63.5 | 169 | 0.58 |
0.43 |
| NGC 4303 | 17.0 | 10.52 | 0.73 | 0.54 | 3.4 | 312.4 | 23.5 | 82.4 | 214 | 0.58 |
0.36 |
| NGC 4321 | 15.2 | 10.75 | 0.55 | 0.21 | 3.0 | 156.2 | 38.5 | 73.7 | 191 | 0.64 |
0.41 |
| NGC 4535 | 15.8 | 10.53 | 0.33 | 0.14 | 4.1 | 179.7 | 44.7 | 76.5 | 124 | 0.44 |
0.37 |
| NGC 5068 | 5.2 | 9.40 | −0.56 | 0.02 | 3.7 | 342.4 | 35.7 | 25.2 | 23 | 0.73 |
0.32 |
| NGC 7496 | 18.7 | 10.00 | 0.35 | 0.53 | 1.7 | 193.7 | 35.9 | 90.8 | 92 | 0.79 |
0.37 |
| IC 5332 | 9.0 | 9.67 | −0.39 | 0.01 | 3.0 | 74.4 | 26.9 | 43.7 | 34 | 0.72 |
0.55 |
Notes. Distances are taken from the compilation of Anand et al. (2021). Stellar masses, star-formation rate (SFR), and offsets from the star-formation main sequence (ΔSFMS) are taken from the PHANGS sample paper (Leroy et al. 2021) and are based on a combined WISE+GALEX analysis (Salim et al. 2018; Leroy et al. 2019). R25 is the B-band isophotal radius recovered via HyperLEDA (Makarov et al. 2014). Position angle (PA) and inclination (i) are taken from analysis of the CO velocity fields from Lang et al. (2020). The median (maximum and minimum) PSF across each MUSE mosaic is taken from Emsellem et al. (2022). The integrated fraction of extinction-corrected Hα emission in the DIG (fDIG) is computed in Sect. 3.1.
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