OB181011
Binary or planetary
Binary lens models
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Model L1 χ2=16965.8 gOGLE I=0.10449±0.21929
s=0.797383±0.0523929 q=0.0065001±0.00278313 u0=0.0759789±0.0170988 α=4.94459±0.105774 ρ*=0.00280714±0.0152545 tE=9.46452±1.4914 t0=8284.78±0.0808566
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Model L2 χ2=17025.5 gOGLE I=0.0999661±0.412683
s=1.1707±0.123041 q=0.00671669±0.00323952 u0=0.0783823±0.0314785 α=4.94584±0.111338 ρ*=0.00352306±0.0621364 tE=9.4613±2.95078 t0=8284.77±0.0837242
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Model L3 χ2=19671.7 gOGLE I=0.241395±0.0960343
s=0.352125±0.0200905 q=0.591815±0.177466 u0=0.0444594±0.00727275 α=4.5008±0.0786881 ρ*=0.0000101301±3.44969 tE=9.42968±0.751892 t0=8284.56±0.0433632
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Binary lens models with parallax
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Model X1 χ2=16885.5 gOGLE I=0.102972±0.501012
s=0.797634±0.0559184 q=0.00655882±0.00308755 u0=0.0759917±0.0366025 α=4.94227±0.115286 ρ*=0.0035541±0.0264053 tE=9.45095±3.3652 t0=8284.78±0.0885323 πE,N=3.±198.263 πE,E=-3.±193.516 |
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Model X2 χ2=16887.9 gOGLE I=0.102572±0.527211
s=0.797454±0.0785413 q=0.0065688±0.00331334 u0=-0.0760058±0.0383364 α=1.34152±0.117046 ρ*=0.0033776±0.0645451 tE=9.44904±3.8828 t0=8284.78±0.0892801 πE,N=3.±215.245 πE,E=-3.±194.96 |
Binary lens models with parallax and orbital motion
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Model O1 χ2=16433.3 gOGLE I=0.142059±0.598129
s=0.842922±0.0636272 q=0.00358893±0.00292972 u0=-0.0717099±0.0425497 α=1.41818±0.0897603 ρ*=0.00439038±0.0264708 tE=9.67136±4.42852 t0=8284.81±0.117436 πE,N=3.±206.879 πE,E=-3.±187.518 (ds/dt)/s=-0.0247126±0.15612 dα/dt=-0.369774±0.190215 w3=0.31466±0.240654 |
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