We present the light curves of the 5 low-mass eclipsing binaries (LMEBs) from the WFCAM Transit Survey (WTS) reported in the paper. These light curves, along with additional spectroscopic data, were simultaneously adjusted to obtain orbital parameters and fundamental properties of the components of each binary system. The obtained results revealed components with inflated radii when compared to evolutionary models.
Cone search capability for table J/MNRAS/476/5253/table3 (LMEBs coordinates and the broad-band photometry used to perform the SED fitting)