Table A.1.
Spiral galaxy sample studied in this paper.
| log(M⋆/M⊙) | log(SFR/[M⊙ yr−1]) | spiral morphology | bar | MUSE | |
|---|---|---|---|---|---|
| IC 1954 | 9.7 | -0.44 | M | 1 | 0 |
| NGC 0628 | 10.3 | 0.24 | M | 0 | 1 |
| NGC 1097 | 10.8 | 0.68 | G | 1 | 0 |
| NGC 1300 | 10.6 | 0.07 | G | 1 | 1 |
| NGC 1365 | 11.0 | 1.23 | G | 1 | 1 |
| NGC 1385 | 10.0 | 0.32 | F | 0 | 1 |
| NGC 1512 | 10.7 | 0.11 | G | 1 | 1 |
| NGC 1566 | 10.8 | 0.66 | G | 1 | 1 |
| NGC 1637 | 9.9 | -0.19 | M | 1 | 0 |
| NGC 1672 | 10.7 | 0.88 | G | 1 | 1 |
| NGC 2090 | 10.0 | -0.39 | G | 0 | 0 |
| NGC 2283 | 9.9 | -0.28 | F | 1 | 0 |
| NGC 2566 | 10.7 | 0.94 | G | 1 | 0 |
| NGC 2835 | 10.0 | 0.09 | G | 1 | 1 |
| NGC 2997 | 10.7 | 0.64 | G | 0 | 0 |
| NGC 3507 | 10.4 | -0.00 | G | 1 | 0 |
| NGC 3627 | 10.8 | 0.58 | G | 1 | 1 |
| NGC 4254 | 10.4 | 0.49 | M | 0 | 1 |
| NGC 4303 | 10.5 | 0.73 | M | 1 | 1 |
| NGC 4321 | 10.7 | 0.55 | G | 1 | 1 |
| NGC 4535 | 10.5 | 0.33 | M | 1 | 1 |
| NGC 4536 | 10.4 | 0.54 | M | 1 | 0 |
| NGC 4548 | 10.7 | -0.28 | G | 1 | 0 |
| NGC 4579 | 11.1 | 0.34 | G | 1 | 0 |
| NGC 4731 | 9.5 | -0.22 | G | 1 | 0 |
| NGC 5248 | 10.4 | 0.36 | G | 1 | 0 |
| NGC 5643 | 10.3 | 0.41 | M | 1 | 0 |
| NGC 6744 | 10.7 | 0.38 | M | 1 | 0 |
Notes. Stellar mass and star formation rates of the spiral galaxies studied in this paper (Leroy et al. 2021b). The spiral morphology lists the spiral family according to Buta et al. (2015) or the definitions adopted in Meidt et al. (2021) for galaxies outside the S4G survey (‘G’ stands for grand-design, ‘M’ for multi-armed, and ‘F’ for flocculent). The bar presence (1 for barred) reflects the environmental masks from Querejeta et al. (2021). The last column indicates if the galaxy is in the PHANGS–MUSE subsample (1) or not (0).
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