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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] χamp2Mathematical equation: $\chi^2_{amp}$ χcp2Mathematical equation: $\chi^2_{cp}$ χamp,sin2Mathematical equation: $\chi^2_{amp,sin}$ χcp,sin2Mathematical equation: $\chi^2_{cp,sin}$ σpos,av [µas] χorb2Mathematical equation: $\chi^2_{orb}$ 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. χamp2Mathematical equation: $\chi^2_{amp}$ and χcp2Mathematical equation: $\chi^2_{cp}$ 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. χorb2Mathematical equation: $\chi^2_{orb}$ describes the goodness of fit of the MAP orbital solution.

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