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Revisiting the Exo-Mercury Candidate GJ 367 b with ESPRESSO and a Self-consistent Tidal Distortion Model

  • Authors: Rena A. Lee, Fei Dai, Ellen M. Price, Te Han, Davide Gandolfi, Mathias Zechmeister, Gumundur Stefánsson, Jiayin Dong, Simon H. Albrecht, Kristine W. F. Lam, Federica Chiti, Jennifer L. van Saders, Daniel Huber, Heather A. Knutson, Karen A. Collins, Michael Zhang, Leslie A. Rogers, Eleonora Armano, Casey L. Brinkman, Nicholas Saunders, Daniel Hey

Rena A. Lee et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

From left to right: SPOC PDCSAP, TGLC, and JWST photometry. Top: binned (30 s) and phase-folded light curve of GJ 367 confirming the transit signal of GJ 367 b (gray points). The best-fit transit model corresponding to each dataset (see Section 3.2) is overplotted. The blue shaded region in each panel is the adopted transit depth and 1σ uncertainty from the SPOC photometry fit, showing that the transit depths are consistent. Bottom: cata minus model residuals.

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