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20182025
most citedDensity, not radius, separates rocky and water-rich small planets orbiting M dwarf stars

301 citations · 1.6k across the 75 of their papers we have counts for

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Showing 2022Show all

26 papers · 1 filter

astro-ph.EP2022★ 8 cited

Discovery of TOI-1260d and the characterisation of the multi-planet system

Kristine W. F. Lam, J. Cabrera, M. J. Hooton +83

We report the discovery of a third planet transiting the star TOI-1260, previously known to host two transiting sub-Neptune planets with orbital periods of 3.127 and 7.493 days, re…

astro-ph.EP2022★ 16 cited

Measuring the Obliquities of the TRAPPIST-1 Planets with MAROON-X

Madison Brady, Jacob Bean, Andreas Seifahrt +6

A star's obliquity with respect to its planetary system can provide us with insight into the system's formation and evolution, as well as hinting at the presence of additional obje…

astro-ph.EP2022★ 18 cited

HD 20329b: An ultra-short-period planet around a solar-type star found by TESS

F. Murgas, G. Nowak, T. Masseron +45

We used TESS light curves and HARPS-N spectrograph radial velocity measurements to establish the physical properties of the transiting exoplanet candidate found around the star HD…

astro-ph.EP2022★ 32 cited

HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone

J. Orell-Miquel, G. Nowak, F. Murgas +20

HD 191939 (TOI-1339) is a nearby (d=54pc), bright (V=9mag), and inactive Sun-like star (G9 V) known to host a multi-planet transiting system. Ground-based spectroscopic observation…

astro-ph.EP2022★ 21 cited

TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter

J. Lillo-Box, D. Gandolfi, D. J. Armstrong +60

The current architecture of a given multi-planetary system is a key fingerprint of its past formation and dynamical evolution history. Long-term follow-up observations are key to c…

astro-ph.EP2022★ 301 cited

Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars

R. Luque, E. Pallé

Exoplanets smaller than Neptune are common around red dwarf stars (M dwarfs), with those that transit their host star constituting the bulk of known temperate worlds amenable for a…