Sample light curve of V0384 Cen from the TESS data. Left panel: data from sector 38 with eclipses of both pairs in time. Right panel: only the phased part of the curve near the primary eclipses of pair A, showing how pair B distorts the shape of the eclipse in different sectors of the data. Moreover, the depth of the eclipse is also obviously different in different sectors. This can be caused by two different phenomena. Firstly, the apsidal motion and change of omega on the eccentric orbit, and secondly an artifact from the TESS reduction causing different third light values in the different sectors of data.