Keplerian fit to the ¹²CO (2−1) line emission of MP Mus using eddy. The observed first moment (left), model (middle), and corresponding residuals (right) are shown. The 0.17″ × 0.15″ beam is shown on the bottom left corner. The area inside the black ellipse shown in the residuals was masked during the fit. The tentative localized residuals mentioned in the text are also marked with a red line. Only the extended configuration from 2017.1.01419.S was used for this analysis.