Fig. 2
A comparison of our sample with some previous disc profile studies (Pohlen & Trujillo 2006; Erwin et al. 2008; Gutiérrez et al. 2011; Herrmann et al. 2013; Muñoz-Mateos et al. 2013; Laine et al. 2014). Upper panel: Hubble types; lower panel: absolute B-band magnitudes. Note that the values are taken from HyperLeda (Makarov et al. 2014).
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