Fig. B.1.
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Impact of including different observations in a mock eccentric binary. Posteriors on the natal kick (vk) and mass loss (Δm2), when the various observational categories are included. Observational categories include spectroscopy (S), resolved astrometric orbit (O), and constraints on any of radial velocity (VR), transverse velocities (VT), or all three velocity components (V3). All categories include spectroscopy (see Sec. 3.1 for justification). Categories without (with) the astrometric orbit are shown on the left (right). Colors correspond to differences in the available velocity constraints: when there are no velocity constraints (e.g., due to no host association; S, SO: dark green), when there are measured RVs for the source and host (SVR, SOVR: blue), when there are measured transverse velocities for the source and host (SVT, SOVT: yellow), and when there are measured velocities in all three directions for the source and host (SV3, SOV3: red). All results here apply for the eccentric mock system; the results for the circular mock system are shown in Fig. 3. Black dashed lines show the true values. Contours capture the 90% confidence interval of the 2D distributions.
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