SOAR TESS Survey III: Mapping the Stellar Companion Deficit around TESS Planet Candidates

arXiv:2608.26250 · astro-ph.EP · Submitted 2026-08-26 · Read on arXiv

astro-ph.EP

Submitted: 2026-08-26

Updated: 2026-08-26

Terminology

• Alignment — 10× in this paper · explained in 1 episode
• Benchmark — 10× in this paper · explained in 2 episodes
• Aperture — 8× in this paper · explained in 1 episode
• Calibration — 5× in this paper · explained in 7 episodes
• Robustness — 5× in this paper · explained in 5 episodes
• European Space Agency — 4× in this paper
• Consistency — 2× in this paper · explained in 3 episodes
• Core — 2× in this paper · explained in 2 episodes
• Metallicity — 2× in this paper · explained in 3 episodes
• Provenance — 2× in this paper · explained in 3 episodes
• Gaia Data Processing and Analysis Consortium — 1× in this paper

Sources

• Determining the Host Stars of Planets in Binary Star Systems with Asterodensity Profiling: Investigating the Canonical Radius Gap
• Speckle Interferometry at SOAR in 2024 and 2025
• Long-term Spectroscopic Survey of the Hyades Cluster: The Binary Population

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