Robotic Observations of Open Clusters using LCOGTN

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Scientific paper

Open clusters offer co-evolutionary groups of up to 1000 stars for which many otherwise elusive parameters can be well measured. That the age of the sample can be established is particularly important in order to test evolution-dependent models. Although certain selected clusters are well studied, a large number have limited data available. We present preliminary results from our study utilizing robotic telescopes to obtain photometry of under-studied clusters with the aim of updating their basic parameters and variable census.

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