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Table 1.

Summary of the galactic parameters of our sample adopted through this work.

Target RA Dec Log10(M*) Log10(MH2) Log10(MHI) Log10(SFR) ΔMS Distance Inclination Mapped area R25 Morphol.
(degrees) (degrees) (M) (M) (M) (M yr−1) (dex) (Mpc) (degrees) (kpc2) (″) compon.
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
NGC 0628 24.1739 15.7836 10.3 9.4 9.7 0.24 0.18 9.84±0.61 8.9 98 296±76 D,SA,C
NGC 1087 41.6049 −0.4987 9.9 9.2 9.1 0.12 0.33 15.85±2.08 42.9 128 89±23 D,B
NGC 1300( • ) 49.9208 −19.4111 10.6 9.4 9.4 0.07 −0.18 18.99±2.67 31.8 366 178±46 D,R,SA,B,C
NGC 1365 53.4015 −36.1404 11.0 10.3 9.9 1.23 0.72 19.57±0.77 55.4 421 360±93 D,R,SA,B,C
NGC 1385( • ) 54.3690 −24.5012 10.0 9.2 9.2 0.32 0.50 17.22±2.42 44.0 100 102±26 D,SA
NGC 1433( • ) 55.5062 −47.2219 10.9 9.3 9.4 0.05 −0.36 18.63±1.76 28.6 441 185±48 D,R,B,C
NGC 1512 60.9756 −43.3487 10.7 9.1 9.9 0.11 −0.21 18.83±1.78 42.5 270 253±65 D,R,SA,B,C
NGC 1566( • ) 65.0016 −54.9380 10.8 9.7 9.8 0.66 0.29 17.69±1.91 29.5 212 216±56 D,SA,B
NGC 1672 71.4270 −59.2473 10.7 9.9 10.2 0.88 0.56 19.4±2.72 42.6 255 184±47 D,R,SA,B,C
NGC 2835 139.4704 −22.3547 10.0 8.8 9.5 0.09 0.26 12.22±0.9 41.3 88 192±49 D,SA,B
NGC 3351 160.9906 11.7037 10.4 9.1 8.9 0.12 0.05 9.96±0.32 45.1 76 216±56 D,R,B,C
NGC 3627 170.0625 12.9915 10.8 9.8 9.1 0.58 0.19 11.32±0.47 57.3 87 308±79 D,SA,B,C
NGC 4254( • ) 184.7068 14.4164 10.4 9.9 9.5 0.49 0.37 13.1±1.87 34.4 174 151±39 D,SA,C
NGC 4303( • ) 185.4789 4.4737 10.5 9.9 9.7 0.73 0.54 16.99±2.78 23.5 220 206±53 D,SA,B,C
NGC 4321( • ) 185.7289 15.8223 10.7 9.9 9.4 0.55 0.21 15.21±0.49 38.5 196 182±47 D,R,SA,B,C
NGC 4535( • ) 188.5846 8.1980 10.5 9.6 9.6 0.33 0.14 15.77±0.36 44.7 126 244±63 D,SA,B,C
NGC 5068 199.7281 −21.0387 9.4 8.4 8.8 −0.56 0.02 5.2±0.22 35.7 23 224±58 D,B
NGC 7496( • ) 347.4470 −43.4278 10.0 9.3 9.1 0.35 0.53 18.72±2.63 35.9 89 100±26 D,B
IC 5332 353.6145 −36.1011 9.7 9.3 −0.39 0.01 9.01±0.39 26.9 34 182±47 D,C

Notes. ( • )Galaxies observed with MUSE WFM-AO mode. Values in Cols. (4)–(7) correspond to those presented in Leroy et al. (2021). Column (8) provides the vertical offset of the galaxy from the integrated main sequence of galaxies, as defined in Leroy et al. (2019). The distances in Col. (9) are derived through redshift-independent techniques, whose details are provided in Anand et al. (2021). Inclinations correspond to those reported in Lang et al. (2020). Uncertainties for the values in Cols. (4)–(8) are on the order of 0.1 dex. Column (11) lists the area mapped by MUSE. Column (12) shows the 25th magnitude isophotal B-band radius in arcseconds, from LEDA (Makarov et al. 2014). Column (13) indicates the morphological components identified in each galaxy by Querejeta et al. (2021; see also Sect. 2.3). Different environments are labeled as D (disk), R (ring), SA (sp. arms), B (bar), and C (center).

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