Table 2.
Fluxes, flux densities and/or count rates of the observations reported.
| Date | MJD– | ATCA | ALMA | VLT/VISIR | Swift/XRT | Swift/BAT | |||
|---|---|---|---|---|---|---|---|---|---|
| 57590 | 5.5 GHz | 9 GHz | 97.49 GHz | 302.99 GHz | 8.7–11.5 μm | 0.4–9 keV | 15–50 keV | ||
| [μJy] | [μJy] | [μJy] | [μJy] | [mJy] | [mJy] | [10−9 erg cm−2 s−1] | [cts cm−2 s−1] | ||
| 02 Aug 2016 | 12 | 515 ± 26 | 428 ± 28 | – | – | – | – | – | 0.033 ± 0.002 (d) |
| 03 Aug 2016 | 13 | – | – | 636 ± 24 | 532 ± 42 | <1.603 (B10.7) | – | 5.60 ± 0.04 | 0.025 ± 0.004 |
| 04 Aug 2016 | 14 | 494 ± 19 | 208 ± 18 | – | – | <1.931 (B11.7) | <1.820 (J8.9) | – | 0.009 ± 0.002 (d) |
| 05 Aug 2016 | 15 | – | – | – | <189 | – | – | 23.1 ± 0.1 | 0.014 ± 0.004 |
| 07 Aug 2016 | 17 | 810 ± 19 | 528 ± 19 | 406 ± 26 | – | – | – | 28.6 ± 0.3 | 0.011 ± 0.004 |
| 19 Sep 2016 | 60 | 259 ± 13 | 366 ± 12 | 753 ± 29 | – | – | – | 1.94 ± 0.02 | 0.009 ± 0.003 |
| 20 Sep 2016 | 61 | – | – | – | 598 ± 63 | – | – | – | 0.002 ± 0.003 (d) |
| SMARTS H | SMARTS J | LCO Y | SMARTS I | LCO i′ | SMARTS/LCO R | SMARTS/LCO V | LCO B | ||
| 1.650 μm | 1.250 μm | 1.004 μm | 0.798 μm | 0.755 μm [mJy] |
0.641 μm | 0.545 μm | 0.436 μm | ||
| 02 Aug 2016 | 12 | – | – | – | – | 1.82 | 1.79 | 1.71 | 1.63 |
| 03 Aug 2016 | 13 | – | 1.69 | – | – | – | 1.82 | 1.86 | – |
| 04 Aug 2016 | 14 | – | 2.40 | – | 3.41 | – | 4.02 | 4.66 | – |
| 05 Aug 2016 | 15 | – | – | – | – | – | – | 4.66 | – |
| 07 Aug 2016 | 17 | 2.07 | 3.08 | 3.86 | 3.47 | 4.01 | 3.53 | 3.97 | 3.02 |
| 19 Sep 2016 | 60 | 0.41 | 0.68 | 0.65 | 0.82 | 0.89 | 0.78 | 0.86 | 0.61 |
Notes. For Swift/BAT we list either the orbital count rate closest in time to the Swift/XRT observation within a given day, or the daily count rate (d) if no Swift/XRT observations were available on the same day. For SMARTS/LCO, the errors are typically smaller than 0.1 magnitudes, making the flux errors typically smaller than 10% and smaller than the symbols in Fig. 5. Upper limits are given at a 3σ significance level.
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