Abstract
We have conducted an astrometric study of the open cluster Lo 807 using proper motion data from UCAC2 catalog. We applied the maximum likelihood method to determine cluster membership by using the proper motion data. The Padova isochrones lines with solar metallicity were fitted upon the Color Magnitude Diagram in near-infrared to derive physical parameters of the cluster. We do not detect significant variable reddening within the cluster. The present result is compared with our previous study.
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