Fig. 2.

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Pan-STARRS (a), 2MASS (b), VVVX (c), and WISE (d) images centred on Garro 02. These fields of view are about 21′×14′, oriented along Galactic coordinates, with the longitude increasing to the left and the latitude increasing to the top. We show the Pan-STARRS and WISE images for comparison just to illustrate that the cluster is present at these wavelengths. The over-density is certainly better seen in the near-IR images (which is what we study in this paper), due to extinction and incompleteness of RGB stars in the other bands.
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