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Two Long-period Low-mass Eclipsing Binaries Recovered from Gaia DR3 Spectroscopic Orbits and TESS Eclipses at the Predicted Conjunctions

Authors: Théo Chopard-Vilhem

Théo Chopard-Vilhem 2026 Research Notes of the AAS 10 .

Provider: AAS Journals

Caption: Figure 1.

Left: eclipse times minus the primary conjunctions predicted by the Gaia orbits, against cycle; the drift is the period difference. Centre and right: primary and secondary eclipses folded on the fitted ephemerides, with the detached-binary model and its parameters (M₂: minimum mass, i = 90°).

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