TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow UpChristina Hedges, J. Villaseñor, Alex Hughes et al.|DSpace@MIT (Massachusetts Institute of Technology)|2021Cited by 33
NEID Rossiter–McLaughlin Measurement of TOI-1268b: A Young Warm Saturn Aligned with Its Cool Host StarJiayin Dong, Steven Giacalone, Elisabeth Newton et al.|The Astrophysical Journal Letters|2022Cited by 22
Outbursts and stellar properties of the classical Be star HD 6226Noel D. Richardson, Franck Houpert, O. Thizy et al.|Monthly Notices of the Royal Astronomical Society|2021Cited by 19
An extreme-mass ratio, short-period eclipsing binary consisting of a B dwarf primary and a pre-main-sequence M star companion discovered by KELTDaniel J. Stevens, Keivan G. Stassun, George Zhou et al.|Monthly Notices of the Royal Astronomical Society|2020Cited by 13
The Unusual M-dwarf Warm Jupiter TOI-1899 b: Refinement of Orbital and Planetary ParametersAndrea S. J. Lin, Jason T. Wright, Jessica E. Libby-Roberts et al.|The Astronomical Journal|2023Cited by 11