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The Sensitivity of TESS to Transiting Planets in TOIs with Close-in Stellar Companions

Authors: Colin Littlefield, Kathryn V. Lester, David R. Ciardi, Steve B. Howell

Colin Littlefield et al 2026 The Astronomical Journal 172 .

Provider: AAS Journals

Caption: Figure 3.

Representative sensitivity grid. The true period and radius of the planet are marked with an “x” and result in SNR = 349, while the color map and contours indicate the scaled SNR of hypothetical planets of various periods and radii.

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