Secondary eclipses of two brown dwarfs in the K2 fields: Detection by multiple dataset merging

Open Access

Fig. 11

As in Fig. 10 (same theoretical models and figure setting), but for EPIC 211946007b (HSHJ 430b). We used 100 K higher internal temperature (i.e., T_int = 1724 K) than the theoretical evolutionary value. The green horizontal bar in the inset shows the theoretical depth in the Kepler waveband, assuming 10% Bond albedo. Red dots with error bars show the observed depth.

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