Table A.1.
Spiral galaxy sample studied in this paper.
| log(M⋆/M⊙) | log(SFR/[M⊙ yr−1]) | R25 (″) | d (Mpc) | spiral morphology | bar | class | |
|---|---|---|---|---|---|---|---|
| IC 1954 | 9.7 | -0.44 | 89.8 | 12.8 | M | 1 | C |
| NGC 0628 | 10.3 | 0.24 | 296.6 | 9.8 | M | 0 | B |
| NGC 1300 | 10.6 | 0.07 | 178.3 | 19.0 | G | 1 | B |
| NGC 1385 | 10.0 | 0.32 | 102.1 | 17.2 | F | 0 | A |
| NGC 1512 | 10.7 | 0.11 | 253.0 | 18.8 | G | 1 | C |
| NGC 1566 | 10.8 | 0.66 | 216.8 | 17.7 | G | 1 | A |
| NGC 1672 | 10.7 | 0.88 | 184.6 | 19.4 | G | 1 | B |
| NGC 2090 | 10.0 | -0.39 | 134.6 | 11.8 | G | 0 | C |
| NGC 2283 | 9.9 | -0.28 | 82.8 | 13.7 | F | 1 | A |
| NGC 2566 | 10.7 | 0.94 | 127.7 | 23.4 | G | 1 | B |
| NGC 2835 | 10.0 | 0.09 | 192.4 | 12.2 | G | 1 | C |
| NGC 2997 | 10.7 | 0.64 | 307.7 | 14.1 | G | 0 | B |
| NGC 3507 | 10.4 | 0.00 | 87.5 | 23.5 | G | 1 | C |
| NGC 3627 | 10.8 | 0.58 | 308.4 | 11.3 | G | 1 | B |
| NGC 4254 | 10.4 | 0.49 | 151.1 | 13.1 | M | 0 | B |
| NGC 4303 | 10.5 | 0.73 | 206.6 | 17.0 | M | 1 | A |
| NGC 4321 | 10.7 | 0.55 | 182.9 | 15.2 | G | 1 | B |
| NGC 4535 | 10.5 | 0.33 | 244.4 | 15.8 | M | 1 | C |
| NGC 4548 | 10.7 | -0.28 | 166.4 | 16.2 | G | 1 | C |
| NGC 4731 | 9.5 | -0.22 | 189.7 | 13.3 | G | 1 | C |
| NGC 5194 | 10.6 | 0.64 | 411.3 | 8.6 | G | 1 | B |
| NGC 5248 | 10.4 | 0.36 | 122.2 | 14.9 | G | 1 | C |
| NGC 5643 | 10.3 | 0.41 | 157.4 | 12.7 | M | 1 | B |
| NGC 6744 | 10.7 | 0.38 | 470.0 | 9.4 | M | 1 | C |
Notes. Stellar mass and star formation rates are adopted from Leroy et al. 2021a who calculated them using the prescriptions and data from Leroy et al. 2019. These are based on GALEX and WISE radial profiles, translated to physical quantities using recipes (SFR conversion and mass-to-light ratio) designed to match the SED fitting results of Salim et al. 2016, 2018. The optical isophotal radius R25 is adopted from RC3 de Vaucouleurs et al. 1991 via LEDA, and distances come from Anand et al. 2021. 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 the classification according to Fig. 5: class A implies positive mean offsets and a significant radial trend; class B corresponds to mean positive offsets but no radial trend; class C implies mean offsets compatible with zero or negative.
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