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The characterisation of detached eclipsing binaries with low mass componentshas become important when verifying the role of convection in stellarevolutionary models, which requires model-independent measurements of stellarparameters with great precision. However, spectroscopic characterisationdepends on single-target radial velocity observations and only a few tens ofwell-studied low-mass systems have been diagnosed in this way. We characteriseeclipsing detached systems from the {\it Kepler} field with low mass componentsby adopting a purely-photometric method. Based on an extensive multi-colourdataset, we derive effective temperatures and photometric masses of individualcomponents using clustering techniques. We also estimate the stellar radii fromadditional modelling of the available {\it Kepler} light curves. Ourmeasurements confirm the presence of an inflation trend in the mass-radiusdiagram against theoretical stellar models in the low-mass regime.

Detached eclipsing binaries from the Kepler field: radii and photometric masses of components in short-period systems