Fig. 7
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Distribution of CSTAR_XPM and the training sample on (MG)0 versus the (GBP − GRP)0 diagram. All the samples have been corrected for 3D extinction. Panel a: Distribution of the CSTAR sample. Panel b: Distribution of the training sample. Panel c: Distribution of carbon stars from the training sample. Panel d: Distribution of non-carbon stars from the training sample.
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