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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.

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