Fig. I.1.
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Colour-magnitude diagrams for de-reddened R and I band magnitudes from MUSE. Red hexagons mark stars within the core of Tr 14 (left, 0.9′, Kharchenko et al. 2013) or outside (right). The orange diamonds (top) indicate the NIR excess stars, while the dark blue crosses mark sources with a detected X-ray component (bottom, Townsley et al. 2011).
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