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Fig. C.2

image

Same as Fig. C.1, for the (ri,JH) plane: here the reddened giant-star sequence is particularly well distinct from the reddened main sequence, while the unreddened M-dwarf locus protrudes upwards near JH ~ 0.6. The reddening-vector slope is here E(ri) /E(JH) = 1.79.

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