Fig. 5.
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Fitting of the LOSVD of the MUSE spectrum of member 8971 with pPXF. The observed spectrum is shown in black, the red curve is the best-fit model, while the green points show the difference between the data and the model. The blue shaded regions along the wavelength axis were excluded in the fitting procedure, due to the presence of sky subtractions around emission lines or laser lines in the spectrum.
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