Fig. 18
Variation of Priam AG with Priam Teff for all stars with clean flags and parallax uncertainty less than 20%. Two unoccupied regions in this plane are marked by “A” and “B”. The black histogram at the bottom shows the total distribution of Teff in our training sample, i.e., the sum over all catalogues shown in Fig. 5. The histogram peaks coincide with the vertical stripes.
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