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Table A.1.

Properties of the 18 galaxies in the literature subsample.

Galaxy Morph. type z Mr Rbar Sbar Ωbar Rcr B/T (Ref.) Ref. Final sample
[mag] [kpc] [km s−1 kpc−1] [kpc]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
ESO 139-G09 SAB00(rs) 0.018 −21.20 6.41 0.44 56.7 ± 15.4 5.54 0.8 ... 1 Yes
ESO 281-G31 SB00(rs) 0.018 −21.22 4.04 ± 0.37 ... 28.6 ± 11.2 7.35 1.8 ... 2 Yes
IC 874 SB00(rs) 0.008 −20.57 3.65 0.57 38.2 ± 13.1 4.93 1.4 ... 1 Yes
NGC 271 (R’)SBab(rs) 0.014 −21.81 7.70 ± 0.27 0.63 29.5 ± 16.0 11.69 1.5 ... 2 No
NGC 936 SB0+(rs) 0.005 −20.71 4.16 0.55 56.8 ± 13.2 5.74 1.4 0.20 (1) 3 Yes
NGC 1023 SB0(rs) 0.002 −21.39 3.94 0.48 89.2 ± 31.5 3.03 0.8 ... 4 Yes
NGC 1308 SB0/a(r) 0.021 −21.71 5.36 0.50 91.8 ± 32.1 3.85 0.8 ... 1 Yes
NGC 1358 SAB0/a(r) 0.013 −21.09 5.16 ± 0.81 ... 34.4 ± 16.6 6.24 1.2 ... 2 Yes
NGC 1440 (R’)SB00 0.005 −18.94 2.53 0.44 71.4 ± 16.4 3.97 1.6 0.15 (2) 1 Yes
NGC 2523 SBbc(r) 0.012 −21.88 8.21 ... 26.8 ± 6.4 10.99 1.3 0.07 (3) 5 Yes
NGC 2950 (R)SB00(r) 0.004 −20.72 3.50 ± 0.21 0.55 109.7 ± 23.5 3.30 1.0 0.45 (2) 6 Yes
NGC 3412 SB00(s) 0.003 −20.45 2.58 ± 0.24 0.41 53.0 ± 14.4 3.90 1.5 ... 1 Yes
NGC 3992 SBbc(rs) 0.004 −19.44 4.89 ± 1.03 0.52 66.7 ± 4.2 3.86 ± 0.26 0.8 0.06 (1) 2 Yes
NGC 4245 SB0/a 0.003 −20.03 3.11 0.48 57.0 ± 23.2 3.49 1.1 0.18 (1) 5 Yes
NGC 4264 SB0 0.008 −20.62 3.19 ± 0.51 0.38 67.7 ± 3.4 2.81 ± 0.17 0.88 0.09 (4) 7 Yes
NGC 4431 dSB0/a 0.003 −18.29 1.94 ± 0.13 0.25 83.6 ± 20.9 1.12 0.6 ... 8 Yes
NGC 4596 SB0+(r) 0.006 −21.84 7.02 0.63 25.1 ± 6.3 7.72 1.1 0.19 (1) 9 Yes
NGC 7079 SB00(s) 0.009 −21.54 4.40 ± 0.61 ... 48.5 ± 1.2 5.30 1.2 0.19 (1) 10 Yes

Notes. (1) Galaxy name. (2) Morphological classification from Corsini (2011), except for NGC 4264 (Cuomo et al. 2019a). (3) Redshift from NED. (4) Absolute SDSS r-band magnitude obtained as described in Sect. 2. (5) Bar radius obtained as described in Sect. 3.1. (6) Bar strength obtained as described in Sect. 3.2. (7) Bar pattern speed obtained as described in Sect. 3.3. (8) Bar corotation radius obtained as described in Sect. 3.4. (9) Bar rotation rate obtained as described in Sect. 3.4. (12) Inclusion in the final analysed sample (galaxies hosting an ultrafast bar at 95% confidence level and with ΔΩbarbar > 0.5 were excluded).

References. (10) Bulge-to-total luminosity ratio provided by 1 = Salo et al. (2015), 2 = Laurikainen et al. (2010), 3 = Treuthardt et al. (2007), 4 = Cuomo et al. (2019a). (11) Reference paper for the direct measurement of the bar pattern speed: 1 = Aguerri et al. (2003), 2 = Gerssen et al. (2003), 3 = Merrifield & Kuijken (1995), 4 = Debattista et al. (2002), 5 = Treuthardt et al. (2007), 6 = Corsini et al. (2003), 7 = Cuomo et al. (2019a), 8 = Corsini et al. (2007), 9 = Gerssen et al. (1999), 10 = Debattista & Williams (2004).

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