VLASS map of the radio structure in MOO J1223+2420. Overplotted are the contours from the same image smoothed to ACA resolution (the levels correspond to the arbitrary values of 0.10 and 0.05 mJy beam⁻¹). The white crosses denote the position of the most significant point sources and respective uncertainties from the 68% credibility interval around each posterior peak. Regardless of the accuracy in the determination of the position of any point-like sources, the low resolution of ACA does not resolve the possible different contributions from the jets and the central galaxy.