Table 1
TFOP photometric follow-up observations.
| Observatory/location | UTC date | Aperture (m) | Filter | Coverage | Result |
|---|---|---|---|---|---|
| Perth Exoplanet Survey Telescope, Perth, Australia | 2018-10-24 | 0.3 | Rc | Full | No NEB detected |
| Myers Observatory, Siding Spring, Australia | 2018-10-24 | 0.4 | Rc | Full | No NEB detected |
| LCOGT CTIO, Chile | 2018-11-01 | 0.4 | i′ | Full | Inconclusive |
| LCOGT SAAO, South Africa | 2018-11-07 | 0.4 | r′ | Full | On-target detection |
| Myers Observatory, Siding Spring, Australia | 2018-11-10 | 0.4 | Lum | Full | No NEB detected |
| LCOGT CTIO, Chile | 2018-11-19 | 1.0 | r′ | Ingress | On-target detection |
Notes. The filter designation Lum indicates a luminance filter with central wavelength 550 nm and bandwidth 300 nm. LCOGT indicates observations from the Las Cumbres Observatory Global Telescope (Brown et al. 2013) 1.0m and 0.4m network nodes at the Cerro Tololo Inter-American Observatory (CTIO) and at the South Africa Astronomical Observatory (SAAO).
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