Table C.3
Supplementary test case summary.
| Case | Fν,tot [Jy] | q | Pobs [yr] | Separation [µas] | e [-] | i [°] | M [108 M⊙] | FWHM1/2 [µas] |
|---|---|---|---|---|---|---|---|---|
| 4 | 0.03/0.02 | 0.6 | 4.41 | 15 | 0 | 0 | 17.3 | 2/1.6 |
| 5 | 0.47/0.03 | 0.06 | 5 | 10 | 0 | 0 | 3.37 | 5/0.3 |
| 6 | 0.03/0.02 | 1 | 10 | rp = 7.5, ra = 22.5 | 0.5 | 80 | 3.37 | 2/2 |
| 7 | 0.03/0.02 | 1 | 30 | 30 | 0 | 0 | 3.00 | 2/2 |
| νLν [ergs−1] | ![]() |
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σpos,av [µas] | ![]() |
FAR [%] | |
|---|---|---|---|---|---|---|---|---|
| 4 | 6.07/4.05 × 1041 | 0.11 | 0.02 | 0.48 | 0.27 | 2.39 | 0.02 | 48 |
| 5 | 9.90/0.55 × 1042 | 0.03 | 0.24 | 0.47 | 0.36 | 0.12 | 0.06 | 0 |
| 6 | 5.54/3.68×1O41 | 0.20 | 0.21 | 7.27 | 0.38 | 0.64 | 0.02 | 81 |
| 7 | 5.54/3.68×1041 | 0.08 | 0.05 | 0.91 | 0.17 | 1.16 | 0.14 | 100 |
Notes. For all cases, Ω, ω and τ are set to 0, as they are expected to have less impact on the orbit fitting than the varied parameters.
and
describe the average goodness of fit of the binary Gaussian model in amplitude and closure phase to the observed data in eht-imaging, across the three observation epochs. The subscript sin describes the χ2 values for fitting a single Gaussian source to the observed data.
describes the goodness of fit of the MAP orbital solution.
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