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A new CCD photometry survey of the open cluster NGC7788 in U, B, V, R and Icolors to magnitude V=20 is present. Extensive comparison of our photometrywith other published dataset shows excellent agreement, indicating that CCDphotometry is capable of producing a uniform set of measurements consistentwith the photometric system defined primarily by the Landolt standard sequence.For this study we used the 113 stars considered to be cluster members by Beckeron 1965.

Photometry Study of Open Cluster NGC 7788