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Table 1
Photometry used for the self-consistent grid model fits. References correspond to (1) Luhman & Esplin (2016), (2) Schneider et al. (2016), (3) Kirkpatrick et al. (2019), (4) Wright et al. (2014), and (5) Leggett et al. (2017).
| Filter | Photometry [mag] | Reference |
|---|---|---|
| HST/WFC3_IR F110W | 26.41 ± 0.27 | 1 |
| HST/WFC3_IR F160W | 23.86 ± 0.03 | 2 |
| HST/WFC3_IR F105W | 27.33 ± 0.19 | 1 |
| HST/WFC3_IR F127M | 24.52 ± 0.12 | 1 |
| 24.49 ± 0.11 | 1 | |
| 24.36 ± 0.09 | 1 | |
| HST/ACS_WFC F850LP | 26.85 ± 0.44 | 1 |
| Spitzer/IRAC I1 | 17.470 ± 0.066 | 3 |
| Spitzer/IRAC I2 | 13.923 ± 0.016 | 3 |
| WISE/W1 | 17.819 ± 0.327 | 4 |
| WISE/W2 | 14.016 ± 0.048 | 4 |
| WISE/W3 | 11.9 ± 0.3 | 5 |
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