OB190763
Planetary
Binary lens models
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Model L1 χ2=7384.79 gOGLE I=5.15543±1.37246
s=1.03228±0.0103125 q=0.0000118949±0.000018194 u0=0.00654538±0.00177369 α=2.99869±0.0247673 ρ*=0.000976477±0.00132566 tE=43.8919±11.2005 t0=8625.91±0.0488127
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Model L2 χ2=7435.85 gOGLE I=10.5909±7.40436
s=0.98846±0.0289602 q=0.000020935±0.0000287429 u0=0.0035412±0.00209663 α=5.97486±0.153109 ρ*=0.00261086±0.00105375 tE=90.2376±57.6358 t0=8625.92±0.0507258
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Model L3 χ2=7816.7 gOGLE I=17.1871±7.02491
s=0.994001±0.019743 q=0.000222338±0.000876109 u0=0.00253533±0.000717564 α=2.66355±1.23138 ρ*=0.00242462±0.00101105 tE=134.82±61.4156 t0=8625.96±0.123097
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Binary lens models with parallax
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Model X1 χ2=7279.03 gOGLE I=6.48518±1.68387
s=1.02788±0.00578525 q=0.0000137593±0.0000151589 u0=0.00536336±0.00138543 α=3.00731±0.0350983 ρ*=0.000683481±0.00138558 tE=53.4348±12.9537 t0=8625.92±0.0487072 πE,N=1.61385±3.50316 πE,E=-0.0664842±2.75023 |
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Model X2 χ2=7288.86 gOGLE I=5.80663±1.37372
s=1.03086±0.00657303 q=0.0000175566±0.0000223959 u0=-0.00592695±0.000909888 α=3.26703±0.0429442 ρ*=0.000802009±0.00152818 tE=48.1953±9.97524 t0=8625.92±0.0486421 πE,N=-2.84371±4.09098 πE,E=-1.27571±3.30419 |
Binary source model
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Model BS χ2=7456.3 gOGLE I=58.4711±0.833158
tE=466.098±167.457 FR=0.00803532±0.0624199 u1=0.000584993±0.00037753 u2=0.000132595±0.00868871 t1=8625.91±0.0487968 t2=8628.±0.348908 |
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