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Table 1

Fractions of galaxies with various morphological features in the barlens groups a–g.

bl-grp B/AB r+rl l R+RL L Nuclear Ansae ⟨ log M/M
% (N) % (N) % (N) % (N) % (N) % (N) % (N)

a 100/... (8) 100 ± 0 (8) ... 37 ± 17 (3) 12 ± 12 (1) 25 ± 15 (2) 12 ± 12 (1) 10.45 ± 0.11
b 75/25 (12) 100 ± 0 (12) ... 92 ± 8 (11) 8 ± 8 (1) 42 ± 14 (5) 17 ± 11 (2) 10.45 ± 0.11
c 85/15 (7) 71 ± 17 (5) 14 ± 13 (1) 42 ± 19 (3) 57 ± 19 (4) 28 ± 17 (2) 57 ± 19 (4) 10.54 ± 0.13
d 100/... (5) 80 ± 17 (4) ... 60 ± 21 (3) ... 100 ± 0 (5) ... 10.86 ± 0.14
e 69/31 (16) 63 ± 12 (10) 12 ± 8 (2) 38 ± 12 (6) 19 ± 10 (3) 50 ± 12 (8) 44 ± 12 (7) 10.66 ± 0.08
f 17/83 (6) 83 ± 15 (5) ... 67 ± 19 (4) 17 ± 15 (1) 50 ± 20 (3) 33 ± 19 (2) 10.75 ± 0.12
g 0/100 (6) 50 ± 20 (3) 17 ± 15 (1) 83 ± 15 (5) ... 33 ± 19 (2) 33 ± 19 (2) 10.45 ± 0.31

Notes. The classifications of the features are adopted from Buta et al. (2015) and Laurikainen et al. (2011). The second column indicates the fractions of B and AB families, while the number in parenthesis is the total number of galaxies in the group. In other columns the percentage of the galaxies with features is shown together with a binomial uncertainty. By nuclear features we mean nuclear bars and rings. The last column lists the mean galaxy mass in each of the barlens groups. The masses are taken from Muñoz-Mateos et al. (2015).

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