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Table A.2

Comparison between the surface brightness profile parameters presented here and other works.

This work (2D) This work (1D) PT06 E08 G11 M16
(1) (2) (3) (4) (5) (6)

Type I % 61.7 34.1 11 27 28 16.4
hin(kpc) 4.88 ± 1.15 4.02 ± 0.79 2.8 ± 0.8 2.89 ± 0.67 5.98 ± 2.70 4.53 ± 2.21
Rbreak (kpc)
Rbreak/hin

Type II % 32.2 39.7 66 42 21 52.8
hin(kpc) 8.92 ± 3.80 6.38 ± 1.91 3.8 ± 1.2/6.9 ± 2.25 6.07 ± 2.50 4.46 ± 1.83 4.60 ± 0.42
Rbreak (kpc) 12.31 ± 3.25 12.71 ± 2.44 9.2 ± 2.4/9.5 ± 3.3 7.69 ± 1.90 7.86 ± 2.35 10.51 ± 0.48
Rbreak/hin 1.92 ± 0.68 3.57 ± 0.44 2.5 ± 0.6/1.7 ± 0.4 2.07 ± 0.81 2.06 ± 0.38 2.28 ± 0.64

Type III % 6.1 26.2 33 24 51 30.8
hin(kpc) 2.51 ± 0.36 3.47 ± 0.91 1.9 ± 0.6 1.89 ± 0.35 2.27 ± 0.51 3.12 ± 0.21
Rbreak (kpc) 8.50 ± 1.40 12.15 ± 3.44 9.3 ± 3.3 8.24 ± 1.65 9.44 ± 2.23 7.68 ± 0.49
Rbreak/hin 3.51 ± 0.54 3.57 ± 0.37 4.9 ± 0.6 4.40 ± 0.41 4.24 ± 0.62 2.46 ± 0.53

Notes. (1) Results applying the 2D decomposition using GASP2D (see Sect. 3.1 for further details) to the sample of galaxies under analysis; (2) results applying a more classical 1D approach (see text for details) to the sample of galaxies; (3) results from Pohlen & Trujillo (2006); for type II galaxies the parameters are divided into classical truncations and breaks associated with the Outer Lindblad Reso–ce (II-CT/II-o.OLR); (4) results from Erwin et al. (2008); (5) results from Gutiérrez et al. (2011); and (6) results from Marino et al. (2016).

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