Images obtained from MUSE data for WRAY 15-1880 in the following lines: Hα (top left), [O I] 6300 Å (top right), [N II] 6583 Å (bottom left), and [S II] 6730 Å (bottom right). The images are in units of contrast with respect to the local continuum. In all cases, the stellar PSF obtained from adjacent continuum wavelengths and the first three principal components have been subtracted. The dashed red line indicates the position of the front side of the polar microjet from the star with PA=297.63 ± 0.37 degrees. The red circle in the top left panel marks the position expected for the candidate planet possibly present in the SPHERE data at the epoch of the MUSE data.