Fig. 6.
Panel a: comparison between the values of the inclination angle obtained from the analysis of the velocity fields, ikin, and from the analysis of the photometric maps, iphot, for our sample of MaNGA galaxies. The points stand for individual galaxies. The line indicates unity. The plus signs indicate data for CALIFA galaxies from Holmes et al. (2015). Panel b: comparison between the kinematic inclination angles derived here and the inclination angles from the HyperLeda database. Panel c: comparison between the photometric inclination angles derived here and the inclination angles from the HyperLeda database.
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