Table A.3
Fit parameters for the 8 distinct planetary models for MOA-2007-BLG-192 consistent with the NACO data.
| Fit | χ2 | tE |
|
u0 | d | θ | q | t∗ | Is | πE | φE |
|
|
|||||||||||
| A | 1121.12 | 82.5 | 5.442 | 0.00309 | 0.912 | 236.9° | 3.7 × 10-5 | 0.040 | 21.61 | 1.51 | 208.5° |
| B | 1121.16 | 83.2 | 5.442 | 0.00306 | 1.120 | 236.8° | 3.7 × 10-5 | 0.041 | 21.62 | 1.49 | 208.7° |
| C | 1121.66 | 82.9 | 5.456 | –0.00349 | 0.807 | 105.5° | 3.4 × 10-4 | 0.041 | 21.60 | 1.47 | 209.2° |
| D | 1122.08 | 83.5 | 5.448 | –0.00296 | 1.113 | 121.9° | 5.8 × 10-5 | 0.041 | 21.62 | 1.44 | 209.8° |
| E | 1125.41 | 83.2 | 5.454 | 0.00306 | 0.890 | 240.1° | 7.6 × 10-5 | 0.048 | 21.61 | 1.19 | 337.5° |
| F | 1125.44 | 82.5 | 5.454 | 0.00309 | 1.118 | 239.9° | 7.5 × 10-5 | 0.049 | 21.60 | 1.16 | 332.3° |
| G | 1125.48 | 81.8 | 5.450 | –0.00313 | 0.897 | 120.3° | 6.4 × 10-5 | 0.049 | 21.60 | 1.13 | 336.5° |
| H | 1125.50 | 80.8 | 5.450 | –0.00309 | 1.110 | 120.6° | 6.1 × 10-5 | 0.048 | 21.61 | 1.19 | 337.8° |
Notes. 
days. t0 and u0 are the time and distance of the closest approach of the source to the lens center-of-mass. q and d are the planet: star mass ratio and separation, and θ is the angle between the source trajectory and the planet-star axis. Is is the best-fit source magnitude, and πE and φE are the magnitude and angle of the microlensing parallax vector. The units for the Einstein radius crossing time, tE, the source radius crossing time, t∗, and are days, and all other parameters are dimensionless.
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