Table 3.
Global properties of the PHANGS–MUSE galaxies.
Galaxy | T type | Slope α | 12 + log(O/H)⟨rgal⟩ | log M* | logSFR | logsSFR | logΣSFR | ΔrSFMS | ΔrKS | ΔrMGMS |
---|---|---|---|---|---|---|---|---|---|---|
(M⊙) | (M⊙ yr−1) | (yr−1) | (M⊙ yr−1 kpc−2) | |||||||
NGC 5068 | 6.0 | 1.58 ± 0.09 | 8.31 | 9.33 | 0.14 | −10.17 | −2.20 | 0.10 | −0.31 | 0.03 |
IC 5332 | 6.8 | 1.82 ± 0.13 | 8.37 | 9.49 | 0.05 | −10.76 | −2.82 | −0.49 | − | − |
NGC 1087 | 5.2 | 1.71 ± 0.10 | 8.40 | 9.96 | 0.70 | −10.11 | −2.25 | 0.36 | 0.09 | 0.39 |
NGC 1385 | 5.9 | 1.52 ± 0.08 | 8.42 | 9.94 | 0.98 | −9.95 | −2.10 | 0.52 | 0.24 | 0.45 |
NGC 7496 | 3.2 | 1.69 ± 0.10 | 8.49 | 10.01 | 0.29 | −10.52 | −2.49 | −0.09 | −0.03 | 0.02 |
NGC 2835 | 5.0 | 1.76 ± 0.11 | 8.38 | 9.87 | 0.37 | −10.28 | −2.36 | 0.11 | −0.00 | −0.22 |
NGC 0628 | 5.2 | 1.71 ± 0.10 | 8.48 | 10.15 | 0.37 | −10.50 | −2.36 | − | − | − |
NGC 3351 | 3.1 | 1.98 ± 0.16 | 8.59 | 10.41 | 0.11 | −11.26 | −2.81 | −0.86 | −0.25 | −0.45 |
NGC 4254 | 5.2 | 1.61 ± 0.08 | 8.53 | 10.37 | 1.29 | −10.19 | −2.11 | 0.38 | 0.06 | 0.43 |
NGC 4303 | 4.0 | 1.56 ± 0.09 | 8.56 | 10.71 | 2.02 | −10.36 | −2.02 | 0.16 | 0.18 | 0.11 |
NGC 4535 | 5.0 | 1.63 ± 0.09 | 8.54 | 10.44 | 0.42 | −10.81 | −2.47 | −0.21 | −0.18 | 0.04 |
NGC 1300 | 4.0 | 1.77 ± 0.12 | 8.52 | 10.61 | 0.40 | −10.96 | −2.94 | −0.45 | −0.06 | −0.42 |
NGC 1512 | 1.2 | 2.04 ± 0.17 | 8.55 | 10.66 | 0.23 | −11.21 | −3.05 | −0.73 | −0.17 | −0.58 |
NGC 1672 | 3.3 | 1.67 ± 0.10 | 8.52 | 10.73 | 1.23 | −10.56 | −2.30 | 0.04 | 0.02 | 0.11 |
NGC 4321 | 4.0 | 1.95 ± 0.15 | 8.56 | 10.62 | 0.80 | −10.64 | −2.42 | −0.01 | −0.13 | 0.15 |
NGC 1566 | 4.0 | 1.57 ± 0.09 | 8.55 | 10.73 | 1.46 | −10.51 | −2.15 | −0.04 | 0.03 | 0.06 |
NGC 3627 | 3.1 | 1.57 ± 0.09 | 8.55 | 10.69 | 0.84 | −10.71 | −2.00 | 0.06 | −0.07 | 0.18 |
NGC 1433 | 1.5 | 1.96 ± 0.16 | 8.54 | 10.85 | 0.38 | −11.20 | −3.04 | −0.85 | −0.23 | −0.67 |
NGC 1365 | 3.2 | 1.74 ± 0.11 | 8.52 | 10.99 | 1.29 | −10.77 | −2.49 | 0.03 | −0.02 | 0.07 |
Notes. The table reports the galaxy name (Col. 1), morphological T type taken from HyperLEDA (Makarov et al. 2014) (Col. 2), the LF slope (Col. 3), the metallicity at the median H II regions’ galactocentric radius (Col. 4), the stellar mass (Col. 5), the SFR (Col. 6), the specific SFR (Col. 7), the SFR density (Col. 8), the offset from the rSFMS (Col. 9), the offset from the rKS (Col. 10), and the offset from resolved the rMGMS (Col. 11). All the properties reported in Cols. 3–11 have been extracted using the PHANGS-MUSE data.
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