Best-fit SED models of the host system of LSQ14mo from magphys, for three components, A, B, and C, are shown in blue, green, and red lines. The colour circles show the different bands’ photometry (shifted to the rest-frame) for the three components of host system where it was possible to have a clear detection. For instance, for component A, the colour circles from left to right are from NUV, griz to JHK-bands photometry. The median and a 1σ range of stellar masses of components A, B, and C are: , and  log M/M_⊙ , respectively.