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Predicting the Yield of Small Transiting Exoplanets around Mid-M and Ultracool Dwarfs in the Nancy Grace Roman Space Telescope Galactic Bulge Time Domain Survey

  • Authors: Patrick Tamburo, Philip S. Muirhead, Courtney D. Dressing

Patrick Tamburo et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 10.

Top: distributions of detected planets with radii between 0.5 and 2.5 R and orbital periods between 0.5 and 10 days around M3–M5 dwarfs in our simulations. The results using the DC15 planet occurrence rates for early-M dwarfs are shown in blue, and the results using the HU19 enhanced planet occurrence rates for M3–M5 dwarfs are shown in orange. Bottom: cumulative distribution functions for the two distributions shown in the top panel.

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