HB221027
Binary or Planetary
Binary lens models
|
Model L1 χ2=3200.55 gMOA I=10.0918±1.17422
s=0.196562±0.115222 q=0.0830592±0.0990055 u0=0.00587138±0.000454981 α=4.90626±0.0844067 ρ*=0.000921277±0.000460419 tE=93.9449±11.1806 t0=9781.81±0.0452069
|
|
Model L2 χ2=3321.37 gMOA I=6.22852±0.419324
s=4.0552±0.0630655 q=0.0831886±0.00113213 u0=0.294074±0.00149252 α=4.93614±0.00725837 ρ*=0.00126923±0.00155882 tE=62.9198±4.89401 t0=9777.71±0.413594
|
|
Model L3 χ2=3332.36 gMOA I=9.31488±1.41227
s=0.109259±0.0639408 q=0.38304±1.00729 u0=0.00649059±0.000811512 α=3.30125±0.0813225 ρ*=0.000995859±0.000373258 tE=91.8029±13.836 t0=9781.84±0.0580614
|
|
Model L4 χ2=3394.26 gMOA I=5.29516±0.365593
s=4.0552±0.066447 q=0.0972019±0.00135558 u0=0.339156±0.00202384 α=4.93661±0.0077595 ρ*=0.00140061±0.00208388 tE=55.1201±4.39528 t0=9777.66±0.440213
|
Binary lens models with parallax
|
Model X1 χ2=3155.86 gMOA I=14.5302±2.08323
s=0.191434±0.165643 q=0.059068±0.10074 u0=0.00413842±0.000658621 α=4.90174±0.0910687 ρ*=0.000630605±0.000486123 tE=133.906±22.5225 t0=9781.81±0.0462358 πE,N=1.51738±3.49204 πE,E=-0.297909±0.83476 |
Extended source Point-lens model
|
Model EP χ2=24325.1 gMOA I=96.9682±6.6867
u0=0.000562747±0.00190967 tE=809.711±2759.02 t0=9781.74±0.0960946 ρ*=0.000644792±0.00223105 |
|