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Table 1.
General properties of the PHANGS-MUSE sample.
| Name | Distance (a) | Log(M⋆) (b) | Log(SFR) (b) | ΔSFMS (b) | R25 (c) | PA (d) | i (d) | Scale | PSF (e) | Copt PSF (f) |
|---|---|---|---|---|---|---|---|---|---|---|
| [Mpc] | [M⊙] | [M⊙ yr−1] | [dex] | [arcmin] | [deg] | [deg] | [pc/arcsec] | [arcsec] | [arcsec] | |
| IC5332 | 9.0 | 9.67 | −0.39 | 0.01 | 3.0 | 74.4 | 26.9 | 43.7 | 0.72 |
0.87 |
| NGC0628 | 9.8 | 10.34 | 0.24 | 0.18 | 4.9 | 20.7 | 8.9 | 47.7 | 0.73 |
0.92 |
| NGC1087 | 15.9 | 9.93 | 0.12 | 0.33 | 1.5 | 359.1 | 42.9 | 76.8 | 0.74 |
0.92 |
| NGC1300 | 19.0 | 10.62 | 0.07 | −0.18 | 3.0 | 278.0 | 31.8 | 92.1 | 0.63 |
0.89 |
| NGC1365 | 19.6 | 10.99 | 1.23 | 0.72 | 6.0 | 201.1 | 55.4 | 94.9 | 0.82 |
1.15 |
| NGC1385 | 17.2 | 9.98 | 0.32 | 0.50 | 1.7 | 181.3 | 44.0 | 83.5 | 0.49 |
0.77 |
| NGC1433 | 18.6 | 10.87 | 0.05 | −0.36 | 3.1 | 199.7 | 28.6 | 90.3 | 0.65 |
0.91 |
| NGC1512 | 18.8 | 10.71 | 0.11 | −0.21 | 4.2 | 261.9 | 42.5 | 91.3 | 0.80 |
1.25 |
| NGC1566 | 17.7 | 10.78 | 0.66 | 0.29 | 3.6 | 214.7 | 29.5 | 85.8 | 0.64 |
0.80 |
| NGC1672 | 19.4 | 10.73 | 0.88 | 0.56 | 3.1 | 134.3 | 42.6 | 94.1 | 0.72 |
0.96 |
| NGC2835 | 12.2 | 10.00 | 0.09 | 0.26 | 3.2 | 1.0 | 41.3 | 59.2 | 0.85 |
1.15 |
| NGC3351 | 10.0 | 10.36 | 0.12 | 0.05 | 3.6 | 193.2 | 45.1 | 48.3 | 0.74 |
1.05 |
| NGC3627 | 11.3 | 10.83 | 0.58 | 0.19 | 5.1 | 173.1 | 57.3 | 54.9 | 0.77 |
1.05 |
| NGC4254 | 13.1 | 10.42 | 0.49 | 0.37 | 2.5 | 68.1 | 34.4 | 63.5 | 0.58 |
0.89 |
| NGC4303 | 17.0 | 10.52 | 0.73 | 0.54 | 3.4 | 312.4 | 23.5 | 82.4 | 0.58 |
0.78 |
| NGC4321 | 15.2 | 10.75 | 0.55 | 0.21 | 3.0 | 156.2 | 38.5 | 73.7 | 0.64 |
1.16 |
| NGC4535 | 15.8 | 10.53 | 0.33 | 0.14 | 4.1 | 179.7 | 44.7 | 76.5 | 0.44 |
0.56 |
| NGC5068 | 5.2 | 9.40 | −0.56 | 0.02 | 3.7 | 342.4 | 35.7 | 25.2 | 0.73 |
1.04 |
| NGC7496 | 18.7 | 10.00 | 0.35 | 0.53 | 1.7 | 193.7 | 35.9 | 90.8 | 0.79 |
0.89 |
(a)
Notes.From the compilation of Anand et al. (2021).
(b)
Derived by Leroy et al. (2021a), using GALEX UV and WISE IR photometry, following a similar methodology to Leroy et al. (2019).
(c)
From LEDA (Makarov et al. 2014).
(d)
From Lang et al. (2020), based on CO(2–1) kinematics.
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