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Table 1.

General properties of the PHANGS-MUSE galaxies.

Name Dista vsysb PAc ic r eff d $ r_{\mathrm{eff}}^{d} $ AO?
Mpc km s−1 deg deg arcmin
IC5332 9.0 699 74.4 26.9 1.4 N
NGC0628 9.8 651 20.7 8.9 1.4 N
NGC1087 15.9 1502 359.1 42.9 0.7 N
NGC1300 19.0 1545 278.0 31.8 1.2 Y
NGC1365 19.6 1613 201.1 55.4 3.3e N
NGC1385 17.2 1477 181.3 44.0 0.7 Y
NGC1433 18.6 1057 199.7 28.6 0.8 Y
NGC1512 18.8 871 261.9 42.5 0.9 N
NGC1566 17.7 1483 214.7 29.5 0.6 Y
NGC1672 19.4 1318 134.3 42.6 0.6 N
NGC2835 12.2 867 1.0 41.3 0.9 N
NGC3351 10.0 775 193.2 45.1 1.0 N
NGC3627 11.3 715 173.1 57.3 1.1 N
NGC4254 13.1 2388 68.1 34.4 0.6 Y
NGC4303 17.0 1560 312.4 23.5 0.7 Y
NGC4321 15.2 1572 156.2 38.5 1.2 Y
NGC4535 15.8 1954 179.7 44.7 1.4 Y
NGC5068 5.2 667 342.4 35.7 1.3 N
NGC7496 18.7 1639 193.7 35.9 0.7 Y

Notes. aFrom the compilation of Anand et al. (2021). bFrom LEDA (Makarov et al. 2014). cFrom Lang et al. (2020), based on CO(2–1) kinematics. dFrom Leroy et al. (2021), based on the stellar mass distribution. eDue to AGN bias, derived from the scale length (l*) as reff = 1.41l* following Equation (5) in Leroy et al. (2021).

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