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CCD photometry of late-type stars in the young open cluster IC 2602

We present the results of VRI photometry of the young open cluster IC 2602. Two 15 arcmin 15 arcmin elds were observed in February and May 1991 using the 1-m Swope telescope at Las Campanas. Using theoretical isochrones obtained from D'Antona & Mazzitelli (1994), and allowing for observational and other uncertainties, we identify 78 primary candidate members with 12 <V <18:5 from their positions on colour- magnitude diagrams. We compare the cluster eld with an oset eld of similar galactic latitude and estimate the contamination due to background stars to be large, 50%, as might be expected given its low galactic lat- itude. We also compare our photometry with that given for the X-ray detected stars of Randich et al. (1995). We present complimentary narrow band H photometry for a subset of the stars.