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Table 3.
Photometric data sets used for the modelling (after binning), removal of outliers, and filtering out images taken during the bad weather.
| Observatory | Filters | Data points | γ |
|---|---|---|---|
| Gaia | G | 79 | 4.4 |
| Spitzer | 3.6 μm | 34 | 4.3 |
| OGLE | I | 210 | 1.78 |
| LCOGT SSO (cleaned): | |||
| coj1m003 | I, V | 129 | 3.5, 1.5 |
| coj1m011 | I, V | 215 | 3.5, 2.8 |
| LCOGT CTIO (cleaned): | |||
| lsc1m004 | I, V | 120 | 1.3, 1.8 |
| lsc1m005 | I, V | 164 | 1.2, 1.5 |
| LCOGT SAAO (cleaned): | |||
| cpt1m010 | I, V | 111 | 1.3, 1.8 |
| cpt1m012 | I, V | 168 | 1.2, 1.3 |
| cpt1m013 | I, V | 195 | 1.2, 1.3 |
| ROAD (binned) | V | 676 | 1.2 |
| μFUN: | |||
| Kumeu | R | 234 | 0.9 |
| KKO (binned) | R | 175 | 3.0 |
| AO | R | 439 | 0.9 |
| FCO | – | 311 | 0.7 |
| CT13 | I | 535 | 0.5 |
Notes. The γ parameter is an error-rescaling factor.
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