Same as top panel of Fig. 4, but for five Gaia candidates outside the LMC bar that are not present in the OGLE4 catalogues of eclipsing binaries, sorted with increasing G_BP − G_RP colour from top to bottom. The sources are Gaia DR3 4655269942119876864, 4651511051157939968, 4651581458546544000, 4651853274236480256, 4651018852223135104; their sky positions are identified in Fig. 24.