Open Access

Fig. 9.


NIR S4G-3.6 μm band Tully-Fisher relation. The dashed blue line represents the Tully-Fisher relation determined by Sorce et al. (2014) for nearby galaxies, while the solid red line the OLS bisector regression to our data. Colors and symbols as in Fig. 8. Bottom panel: M3.6 μm distributions of the HRS (red) and the Sorce et al. (2014) sample (S2014, blue); dotted lines indicate the median value of the corresponding distribution (HRS is = −19.44, S2014 = −20.32).

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