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20112023
most citedMasses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets

497 citations · 8.9k across the 119 of their papers we have counts for

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Showing 2020Show all

10 papers · 1 filter

astro-ph.SR2020★ 28 cited

The K2 Galactic Archaeology Program Data Release 2: Asteroseismic results from campaigns 4, 6, & 7

Joel C. Zinn, Dennis Stello, Yvonne Elsworth +18

Studies of Galactic structure and evolution have benefitted enormously from Gaia kinematic information, though additional, intrinsic stellar parameters like age are required to bes…

astro-ph.SR2020★ 44 cited

PBjam: A Python package for automating asteroseismology of solar-like oscillators

M. B. Nielsen, G. R. Davies, W. H. Ball +14

Asteroseismology is an exceptional tool for studying stars by using the properties of observed modes of oscillation. So far the process of performing an asteroseismic analysis of a…

astro-ph.EP2020★ 41 cited

Orbital misalignment of the super-Earth Men c with the spin of its star

Vedad Kunovac Hodžić, Amaury H. M. J. Triaud, Heather M. Cegla +2

Planet-planet scattering events can leave an observable trace of a planet's migration history in the form of orbital misalignment with respect to the the stellar spin axis, which i…

astro-ph.GA2020★ 129 cited

Chronologically dating the early assembly of the Milky Way

Josefina Montalbán, John Ted Mackereth, Andrea Miglio +16

The standard cosmological model (-CDM) predicts that galaxies are built through hierarchical assembly on cosmological timescales. The Milky Way, like other disc galaxies…

astro-ph.SR2020★ 32 cited

Investigating surface correction relations for RGB stars

Andreas Christ Sølvsten Jørgensen, Josefina Montalbán, Andrea Miglio +7

State-of-the-art stellar structure and evolution codes fail to adequately describe turbulent convection. For stars with convective envelopes, such as red giants, this leads to an i…

astro-ph.SR2020★ 60 cited

The TESS light curve of AI Phoenicis

P. F. L. Maxted, Patrick Gaulme, D. Graczyk +10

Accurate masses and radii for normal stars derived from observations of detached eclipsing binary stars are of fundamental importance for testing stellar models and may be useful f…

astro-ph.GA2020★ 65 cited

Unveiling the Distinct Formation Pathways of the Inner and Outer Discs of the Milky Way with Bayesian Machine Learning

Ioana Ciucă, Daisuke Kawata, Andrea Miglio +2

We develop a Bayesian Machine Learning framework called BINGO (Bayesian INference for Galactic archaeOlogy) centred around a Bayesian neural network. After being trained on the APO…

astro-ph.SR2020★ 21 cited

Solar cycle variation of in helioseismic data and its implications for asteroseismology

Rachel Howe, William J. Chaplin, Sarbani Basu +7

The frequency, , at which the envelope of pulsation power peaks for solar-like oscillators is an important quantity in asteroseismology. We measure for t…

astro-ph.GA2020★ 84 cited

Age dating of an early Milky Way merger via asteroseismology of the naked-eye star Indi

William J. Chaplin, Aldo M. Serenelli, Andrea Miglio +81

Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies. While these accreted stellar populations can be forensically identified as kinematic…

astro-ph.EP2020★ 51 cited

TOI-257b (HD 19916b): A Warm sub-Saturn Orbiting an Evolved F-type Star

Brett C. Addison, Duncan J. Wright, Belinda A. Nicholson +91

We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal was detected by TESS…