Quantifying biases in orbit-superposition modelling with (non-)parametric kinematics

Open Access

Fig. B.2.

Spectrum fits for NGC 4550 and 2768 for the non-regularised fits with Bayes-LOSVD. The four individual spectra correspond to the four regions noted in Figs. 4 and B.6 in descending order. The grey regions define the masked regions during the spectral fit.

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