The transformations between the Mt. Stromlo/AAO and the Caltech/Tololo infrared photometric systems have been determined by means of observations of 21 stars with both systems. A small zero-point difference but no color term is found at K; color terms are found for the J - K, J - H, and H - K colors. All scatter in the transformations can be attributed to the random errors in the observations.
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Elias et al. (1983) studied this question.
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