Table A.3.
Results of the binary fit for GRAVITY data of θ1 Ori B.
| Date | MJD | x | Δ | y | Δy | f | Δf |
|---|---|---|---|---|---|---|---|
| 2017.028 | 57764.11 | −7.10 | 0.02 | −4.68 | 0.02 | 0.224 | 0.003 |
| 2017.138 | 57804.11 | −8.64 | 0.03 | −4.5 | 0.1 | 0.30 | 0.01 |
| 2017.209 | 57830.03 | −9.656 | 0.002 | −4.304 | 0.002 | 0.325 | 0.001 |
| 2017.217 | 57833.03 | −9.897 | 0.002 | −4.196 | 0.002 | 0.330 | 0.005 |
| 2017.777 | 58037.38 | −15.841 | 0.003 | −2.081 | 0.007 | 0.442 | 0.002 |
| 2017.779 | 58038.35 | −15.763 | 0.004 | −2.136 | 0.008 | 0.296 | 0.001 |
| 2017.782 | 58039.38 | −15.841 | 0.003 | −2.081 | 0.007 | 0.442 | 0.002 |
| 2017.782 | 58039.4 | −15.821 | 0.004 | −2.104 | 0.007 | 0.453 | 0.003 |
| 2018.028 | 58129.12 | −17.212 | 0.003 | −0.987 | 0.005 | 0.303 | 0.001 |
Notes. Relative positions x and y in respect to the primary star, with x pointing toward the east and y toward the north. The uncertainties are Δx and Δy. f is the resulting flux ratio, Δf the uncertainty. The first column lists the observation time and the second column the MJD of the observation.
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