@bpbowler forgot to tag you sorry.
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We used
#orbitize! to model the individual eccentricity posteriors of 26 systems, then Brendan did some hierarchical Bayesian modeling to get at the underlying population-level eccentricity distributions. Long story short: they're distinct!Prikaži ovu nit -
This project really put orbitize! through its paces. A lot of early development and testing I did for orbitize! was for this project. That's one of the things I love about orbitize! (and open-source astronomy code in general) -- I get to play developer and user.
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Figure 21 says it all. When you split up the population of substellar imaged companions by mass or mass ratio, the eccentricity distributions are distinct. This points to different formation mechanisms.pic.twitter.com/hIPTz7ab28
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