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Table 1.

Basic properties of the galaxies in our sample.

NGC M D T RC3 type R25 i log M log Mdust logSFR Pixel scale
[Mpc] [arcmin] [deg] [M] [M] [M yr−1] [kpc pix−1]
NGC 0628 M 74 9.0 5 SA(s)c 5.0 7 10.15 7.58 0.382 0.52
NGC 2403 3.5 6 SAB(s)cd 10.0 63 9.47 6.64 −0.135 0.20
NGC 3031 M 81 3.7 2 SA(s)ab 10.7 59 10.65 7.02 −0.462 0.22
NGC 3521 12.0 4 SAB(rs)bc 4.2 73 10.93 7.73 0.499 0.70
NGC 3621 6.9 7 SA(s)d 4.9 65 10.31 7.03 0.153 0.40
NGC 4725 13.6 2 SAB(r)ab pec 4.9 54 10.87 7.39 −0.033 0.79
NGC 4736 M 94 5.2 2 (R)SA(r)ab 3.9 41 10.39 6.39 −0.261 0.30
NGC 5055 M 63 8.2 4 SA(s)b 5.9 59 10.77 7.65 0.391 0.48
NGC 5457 M 101 7.0 6 SAB(rs)cd 12.0 18 10.15 7.67 0.677 0.41

Notes. Redshift-independent distances D and RC3 types are taken from the NED database; Hubble stages T are from Tully (1988); R25 radii are taken from HyperLeda; and inclinations are compiled from different sources, as listed in the caption of Table 1 of Casasola et al. (2017). Stellar masses, dust masses, and SFRs are based on the CIGALE SED fits presented by Nersesian et al. (2019). The pixel scale corresponds to the common 12″ resolution used in our analysis.

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