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We look for very low-mass members in open clusters with different ages placedat different distances. The main goal is to produce a reliable census oflow-mass stars for each of the clusters and derive the Initial Mass Function.To achieve this, we combine deep optical and infrared photometry from our ownobserving runs and from different public databases. We also characterise theindividual stellar parameters of our targets.

Towards an unbiased stellar census in open clusters using multi-wavelength photometry