Seventeen globular clusters in the Large and Small Magellanic Clouds were observed in the mid-infrared wavelength region with the ISOCAM instrument on board the Infrared Space Observatory (ISO). Observations were made using the broadband filters LW1, LW2, and LW10, corresponding to the effective wavelengths of 4.5, 6.7, and 12{mu}m, respectively. We present the photometry of point sources in each cluster, as well as their precise positions and finding charts.
Cone search capability for table J/ApJS/155/401/table1 (Magellanic Cloud clusters observed with ISOCAM and aperture corrections applied with the PSF photometry)
Cone search capability for table J/ApJS/155/401/table5 (ISOCAM photometry of individual point sources in the Magellanic Cloud clusters)