Binary lens seven parameter model maximum likelihood solutions of MOA-2003-BLG-0053/OGLE-2003-BLG-0235, showing planetary solutions and the best non-planetary model (Bond et al. 2004) and from our code, based on EMCEE runs using error-normalized data.
| . | Bond et al. (2004) solutions . | This paper . | |||
|---|---|---|---|---|---|
| . | Best . | Early caustic . | Best . | Wide . | Close . |
| Parameter . | planetary . | planetary . | non-planet . | planetary . | planetary . |
| d | 1.120 ± 0.007 | 1.121 | 1.090 | 1.117 | 0.9143 |
| q(×10−3) | |$3.9 ^{+1.1 }_{ -0.7}$| | 7.0 | 30.0 | 6.5 | 11.5 |
| ρ(×10−4) | 9.6 ± 1.1 | 10.4 | 8.8 | 9.9 | 8.6 |
| u0 | 0.133 ± 0.003 | 0.140 | 0.144 | 0.138 | 0.154 |
| ϕ | 0.7644 ± 0.0024 | 0.6789 | 0.1379 | 0.677 | 3.25 |
| t0 | 2848.06 ± 0.13 | 2847.90 | 2846.20 | 2847.91 | 2850.02 |
| tE | 61.5 ± 0.18 | 58.5 | 57.5 | 59.5 | 56.8 |
| χ2/dof | 1508.19/1374 | 1597.67/1374 | |||
| . | Bond et al. (2004) solutions . | This paper . | |||
|---|---|---|---|---|---|
| . | Best . | Early caustic . | Best . | Wide . | Close . |
| Parameter . | planetary . | planetary . | non-planet . | planetary . | planetary . |
| d | 1.120 ± 0.007 | 1.121 | 1.090 | 1.117 | 0.9143 |
| q(×10−3) | |$3.9 ^{+1.1 }_{ -0.7}$| | 7.0 | 30.0 | 6.5 | 11.5 |
| ρ(×10−4) | 9.6 ± 1.1 | 10.4 | 8.8 | 9.9 | 8.6 |
| u0 | 0.133 ± 0.003 | 0.140 | 0.144 | 0.138 | 0.154 |
| ϕ | 0.7644 ± 0.0024 | 0.6789 | 0.1379 | 0.677 | 3.25 |
| t0 | 2848.06 ± 0.13 | 2847.90 | 2846.20 | 2847.91 | 2850.02 |
| tE | 61.5 ± 0.18 | 58.5 | 57.5 | 59.5 | 56.8 |
| χ2/dof | 1508.19/1374 | 1597.67/1374 | |||
Binary lens seven parameter model maximum likelihood solutions of MOA-2003-BLG-0053/OGLE-2003-BLG-0235, showing planetary solutions and the best non-planetary model (Bond et al. 2004) and from our code, based on EMCEE runs using error-normalized data.
| . | Bond et al. (2004) solutions . | This paper . | |||
|---|---|---|---|---|---|
| . | Best . | Early caustic . | Best . | Wide . | Close . |
| Parameter . | planetary . | planetary . | non-planet . | planetary . | planetary . |
| d | 1.120 ± 0.007 | 1.121 | 1.090 | 1.117 | 0.9143 |
| q(×10−3) | |$3.9 ^{+1.1 }_{ -0.7}$| | 7.0 | 30.0 | 6.5 | 11.5 |
| ρ(×10−4) | 9.6 ± 1.1 | 10.4 | 8.8 | 9.9 | 8.6 |
| u0 | 0.133 ± 0.003 | 0.140 | 0.144 | 0.138 | 0.154 |
| ϕ | 0.7644 ± 0.0024 | 0.6789 | 0.1379 | 0.677 | 3.25 |
| t0 | 2848.06 ± 0.13 | 2847.90 | 2846.20 | 2847.91 | 2850.02 |
| tE | 61.5 ± 0.18 | 58.5 | 57.5 | 59.5 | 56.8 |
| χ2/dof | 1508.19/1374 | 1597.67/1374 | |||
| . | Bond et al. (2004) solutions . | This paper . | |||
|---|---|---|---|---|---|
| . | Best . | Early caustic . | Best . | Wide . | Close . |
| Parameter . | planetary . | planetary . | non-planet . | planetary . | planetary . |
| d | 1.120 ± 0.007 | 1.121 | 1.090 | 1.117 | 0.9143 |
| q(×10−3) | |$3.9 ^{+1.1 }_{ -0.7}$| | 7.0 | 30.0 | 6.5 | 11.5 |
| ρ(×10−4) | 9.6 ± 1.1 | 10.4 | 8.8 | 9.9 | 8.6 |
| u0 | 0.133 ± 0.003 | 0.140 | 0.144 | 0.138 | 0.154 |
| ϕ | 0.7644 ± 0.0024 | 0.6789 | 0.1379 | 0.677 | 3.25 |
| t0 | 2848.06 ± 0.13 | 2847.90 | 2846.20 | 2847.91 | 2850.02 |
| tE | 61.5 ± 0.18 | 58.5 | 57.5 | 59.5 | 56.8 |
| χ2/dof | 1508.19/1374 | 1597.67/1374 | |||
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