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Fig. 7

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Two-color diagram that combines the Ks magnitude of the 2MASS system and the magnitudes [3.4] and [4.6] of the WISE system, used to identify YSOs. We plot the stars in the 15′ × 15′ area centered on IC 1805, for which the magnitudes Ks, [3.4] and [4.6] have observational errors < 0.06 mag. The two straight lines taken from Koenig et al. (2012) divide the plane into three areas in which YSOs of types I and II and young diskless objects are located.

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