A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274)
astro-ph.EP, astro-ph.SR
Submitted: 2026-10-20
Updated: 2026-10-20
Related papers
- PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
- Gravitational Microlensing
- Two-stage disruption of resonant chains
- Detectability of resolved hydrogen lines from the accretion shock at gas giants and their circumplanetary discs
- Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
- Identifying deformed exoplanets with JWST and Ariel: A target selection metric for phase curve observations