Table 3.
Energy fluxes of the optical counterpart of J17407.
| Wavelength | Flux | eflux | Filter | Catalogue | Reference |
|---|---|---|---|---|---|
| μm | 10−6 (Jy) | 10−6 (Jy) | |||
| 0.748 | 14.2 | 0.7(a) | i | Pan-STARRS | 1 |
| 0.876 | 55.9 | 10.2 | Z | VISTA | 2 |
| 1.02 | 113 | 21 | Y | VISTA | 2 |
| 1.25 | 273 | 38 | J | VISTA | 2 |
| 1.25 | 283 | 37 | J | VVV | 3 |
| 1.63 | 429 | 71 | H | VISTA | 2 |
| 1.63 | 436 | 67 | H | VVV | 3 |
| 2.13 | 442 | 76 | Ks | VISTA | 2 |
| 2.19 | 413 | 13 | K | VIRAC | 4 |
| 2.19 | 429 | 68 | K | VVV | 3 |
Notes.
We selected sources within 3σ radius centered on the position of VVV J174042.01−280725.05. Including systematic errors for sources inside the Galactic plane (Magnier et al. 2020).
References. (1) Chambers et al. (2016); (2) Minniti et al. (2017); (3) Herpich et al. (2021); (4) Smith et al. (2018).
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