HB211150
Planetary
Binary lens models
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Model L1 χ2=14591.5 gMOA I=2.90048±0.913574
s=1.17972±0.00789146 q=0.00174147±0.000711372 u0=0.24751±0.0344816 α=1.58786±0.0140901 ρ*=0.000567513±0.00162149 tE=73.9807±36.4421 t0=9386.96±0.264517
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Model L2 χ2=14608.9 gMOA I=2.11491±0.632297
s=1.19815±0.00727152 q=0.00160884±0.000703848 u0=0.296206±0.0284951 α=1.58544±0.0132145 ρ*=0.000648731±0.0019277 tE=64.448±31.0931 t0=9387.±0.249821
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Model L3 χ2=14623.4 gMOA I=0.234482±0.215687
s=1.3385±0.00327688 q=0.00050342±0.000298244 u0=0.582401±0.00722651 α=1.58738±0.0065257 ρ*=0.000843867±0.0016457 tE=41.841±18.4555 t0=9386.87±0.219809
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Binary lens models with parallax
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Model X1 χ2=14088.6 gMOA I=2.92012±1.02676
s=1.18081±0.00703278 q=0.00182662±0.000970043 u0=0.246317±0.0417426 α=1.58759±0.0272804 ρ*=0.000622123±0.00276722 tE=74.2661±36.5335 t0=9386.97±0.494845 πE,N=-0.0912923±0.111002 πE,E=-0.842767±0.45481 |
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Model X2 χ2=14403. gMOA I=1.39591±0.422353
s=1.22716±0.00415157 q=0.00144264±0.000752983 u0=0.362109±0.02064 α=1.59123±0.0147617 ρ*=0.000758564±0.00252305 tE=55.7328±26.0885 t0=9386.86±0.333962 πE,N=-0.0290474±2.26351 πE,E=-0.672067±1.18676 |
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