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 μm, respectively. We present the photometry of point sources in each cluster, as well as their precise positions and finding charts.
CITATION STYLE
Tanabe, T., Kučinskas, A., Nakada, Y., Onaka, T., & Sauvage, M. (2004). ISOCAM Observations of Globular Clusters in the Magellanic Clouds: The Data. The Astrophysical Journal Supplement Series, 155(2), 401–419. https://doi.org/10.1086/424929
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