J. Astrophys. Astr. (0000) 000: #### DOI UBV(RI)KC Photometry of NGC 2323 and NGC 2539 Open Clusters Inci˙ Akkaya Oralhan1,*, Raul´ Michel2, William J. Schuster2,Yuksel¨ Karatas¸3,Yonca Karslı1 and Carlos Chavarr´ıa2 1Erciyes University, Astronomy and Space Science Observatory, TR-38039, Kayseri, Turkey 2Observatorio Astronomico Nacional, Universidad Nacional Autonoma de Mexico,´ Apartado Postal 106, C.P. 22800, Ensenada, B.C., Mexico.´ 3Department of Astronomy and Space Sciences, Science Faculty, Istanbul University, 34119, Istanbul, Turkey. *Corresponding author. E-mail:
[email protected] MS received ?? ?? 2019; accepted ?? ?? 2019 Abstract. The open clusters NGC 2323 and NGC 2539 have been analysed using CCD UBV(RI)KC photo- metric data, observed at the San Pedro Martir´ Observatory. Cluster memberships have been determined with the proper motion and parallax measures from the GaiaDR2 astrometric data release. Photometric metal and heavy element abundances have been obtained as ([M=H]; Z) = (−0:10; 0:012) (NGC 2323) and (−0:31; 0:007) (NGC 2539), from the δ(U–B) technique in the two colour diagrams, which are used to select the appropriate PARSEC isochrones. The estimated reddening of NGC 2323 is E(B-V)=0.23±0.04 using 11 early type stars. For NGC 2539, we find E(B-V)= 0.02±0.06. For (B–V) colour, distance moduli and distances for NGC 2323 and NGC 2539 are de- rived as (V0–MV, d (pc)) = (10.00±0.10, 1000±50) and (V0–MV, d (pc)) = (10.00±0.04, 1000±20), respectively. The median GaiaDR2 distance d=1000±140 pc ($=0.998±0.136 mas) for the likely members of NGC 2323 is in concordance with its four colour photometric distances 910–1000 pc.