Description
We have mosaicked Two Micron All Sky Survey (2MASS) images to derive surface brightness profiles in J, H, and Ks for 104 Galactic globular clusters. We fit these with King profiles and show that the core radii are identical to within the errors for each of these IR colors and are identical to the core radii at V in essentially all cases. We derive integrated-light colors V-J, V-H, V-Ks, J-H, and J-Ks for these globular clusters.
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