Four transiting sub-Neptunes with radii measured to <1.7% precision and masses >3 sigma for three planets, plus an outer non-transiting companion, discovered around TOI-5624 via TESS, CHEOPS photometry, and ground-based RV data.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
representative citing papers
NSVS 10653195 is a detached eclipsing binary with two K-type stars of masses 0.6402 and 0.6511 solar masses and radii 0.687 and 0.672 solar radii, showing radius inflation relative to models.
Radial velocity measurements from NIR spectra show one TWA candidate as a spectroscopic binary with 41.9% membership probability and the other as a likely single member with 99.5% probability.
citing papers explorer
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The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
Four transiting sub-Neptunes with radii measured to <1.7% precision and masses >3 sigma for three planets, plus an outer non-transiting companion, discovered around TOI-5624 via TESS, CHEOPS photometry, and ground-based RV data.
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Absolute dimensions of the low-mass eclipsing binary system NSVS 10653195
NSVS 10653195 is a detached eclipsing binary with two K-type stars of masses 0.6402 and 0.6511 solar masses and radii 0.687 and 0.672 solar radii, showing radius inflation relative to models.
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Radial Velocities of Low-mass Candidate TWA Members
Radial velocity measurements from NIR spectra show one TWA candidate as a spectroscopic binary with 41.9% membership probability and the other as a likely single member with 99.5% probability.