author={Benjamin A. Thompson and Peter M. Frinchaboy and Karen Kinemuchi and A. Sarajedini and Roger E. Cohen},
  journal={The Astronomical Journal},
The current generation of stellar isochrone models exhibits non-negligible discrepancies due to variations in the input physics. The success of each model is determined by how well it fits the observations, and this paper aims to disentangle contributions from the various physical inputs. New deep, wide-field optical and near-infrared photometry (UBVRIJHKS) of the cluster M35 is presented, against which several isochrone systems are compared: Padova, PARSEC, Dartmouth, and Y2. Two different… 

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