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Near infrared photometry of WISE J085510 74 071442 5

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Figure

Fig. 1. Identification of WISE J085510.74−071442.5 (at the center of the red circles) on the WFC3 and Hawk-I images sized 24 00 × 24 00
Fig. 2. Spectral energy distribution of J0855−0714 (red and black symbols). Circles denote positive detections and arrows indicate  up-per limits
Fig. 4. Evolution of the absolute W2 magnitude is shown for masses between 1 and 10 M Jup (COND models; Baraffe et al
Fig. 5. Color-magnitude diagram considering the F110W and W2 fil- fil-ters. Our F110W data are plotted as red symbols (J0855−0714 is  la-beled)
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