Table 2.
Results of the break identification.
| Galaxy | Break | Break | Break | QKar, p | ηk, p | Class |
|---|---|---|---|---|---|---|
| type | radius | μ | ||||
| CIG 11 | II | 19 ± 3 | 24.8 ± 0.7 | −1.23 | 2.03 | – |
| CIG 33 | III | 12 ± 2 | 23.6 ± 0.4 | −3.11 | 2.09 | H |
| CIG 59 | I | – | – | −3.10 | 1.89 | – |
| CIG 94 | II | 10 ± 2 | 22.5 ± 0.4 | – | – | – |
| CIG 96 | III | 17 ± 3 | 25.5 ± 0.2 | – | – | H |
| CIG 100 | II | 5 ± 1 | 21.9 ± 0.2 | −3.01 | 2.16 | – |
| CIG 154 | I | – | – | – | – | C |
| CIG 279 | I | – | – | −3.04 | 2.16 | – |
| CIG 329 | II | 16 ± 3 | 22.0 ± 0.3 | −3.57 | 1.31 | T |
| CIG 335 | II | 15 ± 3 | 23.5 ± 0.5 | −3.48 | 1.42 | H |
| CIG 340 | II | 14 ± 3 | 22.4 ± 0.4 | −3.85 | 1.04 | H+T |
| CIG 512 | II | 9 ± 2 | 24.2 ± 0.5 | −3.40 | 1.38 | – |
| CIG 568 | II | 22 ± 5 | 23.3 ± 0.5 | −2.80 | 2.44 | – |
| CIG 613 | II | 39 ± 7 | 24.9 ± 0.9 | −3.33 | 1.78 | T |
| CIG 616 | I | – | – | −3.02 | 2.55 | H |
| CIG 626 | I | – | – | −3.93 | 1.05 | – |
| CIG 744 | I | – | – | −2.20 | 2.47 | – |
| CIG 772 | II | 17 ± 3 | 23.1 ± 0.4 | – | – | – |
| CIG 800 | II | 17 ± 3 | 23.6 ± 0.5 | – | – | C |
| CIG 838 | I | – | – | – | – | – |
| CIG 947 | I | – | – | – | – | C |
| CIG 971 | I | – | – | – | – | C |
| CIG 1002 | II | 14 ± 3 | 22.8 ± 0.5 | −2.42 | 2.69 | – |
| CIG 1004 | II | 15 ± 3 | 22.3 ± 0.4 | −2.25 | 1.49 | C |
| CIG 1047 | II | 7 ± 2 | 22.6 ± 0.9 | −2.62 | 2.25 | H |
Notes. The first column shows the galaxy CIG name. The second, third, and fourth columns show the type of break, the break radii in kpc if any, and the surface brightness level in mag arcsec−2 of the break, respectively. The fifth and sixth columns show the interaction parameters QKar, p and ηk, p from the AMIGA catalogue (Argudo-Fernández et al. 2013). The seventh column indicates interaction features found in this work. We define three different categories, halo-perturbed (H), tidal streams (T), and cirrus contamination (C). More information about the classification can be found in Sect. 3.5.
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