Table 1.
Main properties of the galaxies in our sample.
| Galaxy name | Hubble type (1) | M* (1010 M⊙) (2) | R0, disk (kpc) (3) | Ropt (2) (kpc) | hscale (4) (kpc) |
|---|---|---|---|---|---|
| Au1 | SBb | 2.75 | 4.07 | 20.0 | 2.8 |
| Au2 | SBc | 7.05 | 8.99 | 37.0 | 3.5 |
| Au3 | Sb | 7.75 | 4 | 31.0 | 2.7 |
| Au5 | SBb | 6.72 | 4.58 | 21.0 | 3.6 |
| Au6 | SBbc | 4.75 | 5.43 | 26.0 | 3.3 |
| Au7 | SBb | 4.88 | 5.43 | 25.0 | 5.1 |
| Au8 | Sc | 2.99 | 3 | 25.0 | 3.0 |
| Au9 | SBb | 6.10 | 6.45 | 19.0 | 2.8 |
| Au10 | SBa | 5.94 | 6.45 | 16.0 | 3.3 |
| Au12 | SBab | 6.01 | 3.73 | 19.0 | 13.1 |
| Au14 | SBb | 10.39 | 5.09 | 26.0 | 6.2 |
| Au15 | Sbc | 3.93 | 3 | 23.0 | 4.4 |
| Au16 | Sc | 5.41 | 4 | 36.0 | 4.0 |
| Au17 | SBa | 7.61 | 5.43 | 16.0 | 2.4 |
| Au18 | SBb | 8.04 | 6.45 | 21.0 | 2.8 |
| Au19 | Sbc | 5.32 | 3 | 24.0 | 3.8 |
| Au21 | SBb | 7.72 | 3.39 | 24.0 | 4.3 |
| Au22 | SBa | 6.02 | 6.28 | 13.5 | 2.7 |
| Au23 | SBbc | 9.02 | 9.50 | 25.0 | 2.9 |
| Au24 | SBc | 6.55 | 5.09 | 30.0 | 4.2 |
| Au25 | SBb | 3.14 | 4.41 | 21.0 | 2.1 |
| Au26 | SBa | 10.97 | 5.43 | 18.0 | 3.2 |
| Au27 | SBbc | 9.61 | 5.77 | 26.0 | 3.7 |
| Au28 | SBa | 10.45 | 7.46 | 17.5 | 3.8 |
Notes. (1) Hubble types from Walo-Martín et al. (2021); (2) Stellar mass M* and optical radius Ropt (defined as the radius where the B-band surface brightness drops below 25 mag arcsec−2) are from Grand et al. (2017); (3) R0, disk, the minimum radius at which the thin disk dominates over the central component. When the galaxy is barred, this value is the length of the bar taken from Blázquez-Calero et al. (2020), following Walo-Martín et al. (2021). When the galaxy is unbarred, R0, disk is the approximate radius where the disk starts to dominate over the bulge, according to Fig. 4 in Grand et al. (2017); (4) The hscale parameter was calculated here as the standard deviation of the vertical position of particles at 0.5 Ropt, following García de la Cruz et al. (2021).
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