Table 1.
Optical and MIR magnitudes of PSO J191+86.
| Filter | Central λ | Mag | Ref. survey |
|---|---|---|---|
| (μm) | (AB) | ||
| (1) | (2) | (3) | (4) |
| rPS1 | 0.680 | 21.34 ± 0.15 | PS1 |
| iPS1 | 0.745 | 19.78 ± 0.04 | PS1 |
| zPS1 | 0.870 | 19.49 ± 0.03 | PS1 |
| yPS1 | 0.978 | 19.22 ± 0.06 | PS1 |
| W1 | 3.4 | 18.502 ± 0.035 | WISE |
| W2 | 4.6 | 18.386 ± 0.051 | WISE |
Notes. Column (1): optical and MIR filters; Col. (2): filter central wavelength in μm; Col. (3): observed AB de-reddened magnitude; Col. (4): reference catalog. The offset between the Pan-STARRS PS1 optical and WISE MIR positions is 0.85″. The relations to convert from Vega to AB systems are: W1AB = W1 + 2.683; W2AB = W2 + 3.319 (Cutri et al. 2012).
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