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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 8.

Radii of confirmed (circles) and candidate planets (stars) smaller than 4 R vs. effective temperature for hosts with T eff < 3300 K from the Kepler/K2 (orange) and TESS (pink) missions. Detections from a representative iteration of our simulation (with 1347 total detections) are shown in blue. The effective temperature is listed on the bottom axis while the approximate spectral types are given along the top axis. The top panel shows histograms of the number of planet detections as a function of effective temperature for the different missions.

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