Mass of 13.7 Earth masses and density 0.4 g cm^{-3} measured for TOI-1883 b, a super-Neptune in the ridge regime around an early-M dwarf, with implications for disk migration and photoevaporation.
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2026 2verdicts
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Comparison of two exoplanet phase curve surveys shows population-level consistency but individual variations, plus a Kepler's law inconsistency in archival parameters that warrants routine verification.
citing papers explorer
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The mass of TOI-1883 b: A low density super-Neptune in the ridge regime transiting an early-M dwarf
Mass of 13.7 Earth masses and density 0.4 g cm^{-3} measured for TOI-1883 b, a super-Neptune in the ridge regime around an early-M dwarf, with implications for disk migration and photoevaporation.
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Comparing Results from Two Uniform Phase Curve Surveys
Comparison of two exoplanet phase curve surveys shows population-level consistency but individual variations, plus a Kepler's law inconsistency in archival parameters that warrants routine verification.