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Table 1.

Relations for a G2V star using the Cardelli et al. (1989) and O’Donnell (1994) extinction curve with RV = 3.1 in the SDSS ugriz and 2MASS photometric systems (Marigo et al. 2017).

1.569 1.206 0.871 0.683 0.492 0.294 0.181 0.118

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