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Table 1.

Main properties of the galaxies in the PHANGS–MUSE sample.

Galaxy RA Dec Morph(1) Distance(2) i(3) PA(3) Log M(∗)(4) SFR(4) ΔSFMS(4) R25(1) FWHMPSF(5) pc/″ rmax
(°) (°) (Mpc) (°) (°) (M) (M yr−1) (″) (″)
IC 5332 353.61453 −36.10108 SABc 9.01 26.9 74.4 9.67 0.41 0.01 182 0.87 43.6 0.68
NGC 0628 24.173855 15.783643 Sc 9.84 8.9 20.7 10.34 1.75 0.18 297 0.92 47.6 0.51
NGC 1087 41.60492 −0.498717 Sc 15.85 42.9 359.1 9.93 1.31 0.33 89 0.92 76.5 1.37
NGC 1300 49.920815 −19.411114 Sbc 18.99 31.8 278.0 10.62 1.17 −0.18 178 0.89 91.6 0.96
NGC 1365 53.40152 −36.140404 Sb 19.57 55.4 201.1 10.99 16.90 0.72 361 1.15 94.4 0.73
NGC 1385 54.369015 −24.501162 Sc 17.22 44.0 181.3 9.98 2.09 0.50 102 0.67 83.1 1.21
NGC 1433 55.506195 −47.221943 SBa 18.63 28.6 199.7 10.87 1.13 −0.36 186 0.91 89.9 1.05
NGC 1512 60.975574 −43.348724 Sa 18.83 42.5 261.9 10.71 1.28 −0.21 253 1.25 90.8 0.62
NGC 1566 65.00159 −54.93801 SABb 17.69 29.5 214.7 10.78 4.54 0.29 217 0.8 85.3 0.73
NGC 1672 71.42704 −59.247257 Sb 19.4 42.6 134.3 10.73 7.60 0.56 185 0.96 93.5 1.00
NGC 2835 139.47044 −22.35468 Sc 12.22 41.3 1.0 10.00 1.24 0.26 192 1.15 59.0 0.69
NGC 3351 160.99065 11.70367 Sb 9.96 45.1 193.2 10.36 1.32 0.05 217 1.05 48.2 0.76
NGC 3627 170.06252 12.9915 Sb 11.32 57.3 173.1 10.83 3.84 0.19 308 1.05 54.7 0.66
NGC 4254 184.7068 14.416412 Sc 13.1 34.4 68.1 10.42 3.07 0.37 151 0.89 63.3 1.28
NGC 4303 185.47888 4.473744 Sbc 16.99 23.5 312.4 10.52 5.33 0.54 207 0.78 82.0 0.66
NGC 4321 185.72887 15.822304 SABb 15.21 38.5 156.2 10.75 3.56 0.21 183 1.16 73.4 0.97
NGC 4535 188.5846 8.197973 Sc 15.77 44.7 179.7 10.53 2.16 0.14 244 0.56 76.1 0.56
NGC 5068 199.72807 −21.038744 Sc 5.2 35.7 342.4 9.40 0.28 0.02 224 1.04 25.2 0.89
NGC 7496 347.44702 −43.42785 Sb 18.72 35.9 193.7 10.00 2.26 0.53 100 0.89 90.3 1.06

Notes. The table reports the galaxy name (Col. 1), galaxy center sky coordinates (Cols. 2–3), Hubble morphological type (Col. 4), distance (Col. 5), inclination (Col. 6), position angle (Col. 7), total stellar mass (Col. 8), total SFR (Col. 9), offset from the star formation main sequence (Col. 10), R25B-band isophotal radius (Col. 11), angular resolution of the copt data (Col. 12), the parsec per arcsecond scaling factor (Col. 13), and the maximum deprojected galactocentric radius in units of R25 (Col. 14).

References.(1)HyperLEDA, Makarov et al. (2014), (2)Anand et al. (2021), (3)Lang et al. (2020), (4)Leroy et al. (2021), (5)Emsellem et al. (2021)

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