Fig. 5
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Distance of the P1/P2 and P5 samples in LOPS2. Left panel: distribution of the 8235 P1+P2 stars in LOPS2 in the (R⋆, distance) plane. The stellar effective temperature from the PIC v2.0.0 is color coded. Right panel: same but for the P5 sample (167 149 stars; P1/P2 not included). The distribution moves to larger distances due to the fainter magnitude limit of P5 (V < 13 vs. V < 11).
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