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20072023
most citedSkyMapper Southern Survey: First Data Release (DR1)

397 citations · 7k across the 129 of their papers we have counts for

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Showing 2017Show all

12 papers · 1 filter

astro-ph.SR2017★ 69 cited

Modelling Kepler Red Giants in Eclipsing Binaries:Calibrating the Mixing Length Parameter with Asteroseismology

Tanda Li, Timothy R. Bedding, Daniel Huber +4

Stellar models rely on a number of free parameters. High-quality observations of eclipsing binary stars observed by Kepler offer a great opportunity to calibrate model parameters f…

astro-ph.SR2017★ 107 cited

Finding binaries from phase modulation of pulsating stars with Kepler: V. Orbital parameters, with eccentricity and mass-ratio distributions of 341 new binaries

Simon J. Murphy, Maxwell Moe, Donald W. Kurtz +3

The orbital parameters of binaries at intermediate periods (-- d) are difficult to measure with conventional methods and are very incomplete. We have undertaken a new s…

astro-ph.SR2017★ 18 cited

A Spectroscopic and Photometric Investigation of the Mercury-Manganese Star KIC 6128830

Stefan Hümmerich, Ewa Niemczura, Przemysław Walczak +4

The advent of space-based photometry provides the opportunity for the first precise characterizations of variability in Mercury-Manganese (HgMn/CP3) stars, which might advance our…

astro-ph.SR2017★ 130 cited

Theory and evidence of global Rossby waves in upper main-sequence stars: r-mode oscillations in many Kepler stars

Hideyuki Saio, Donald W. Kurtz, Simon Murphy +2

Asteroseismic inference from pressure modes (p modes) and buoyancy, or gravity, modes (g modes) is ubiquitous for stars across the Hertzsprung--Russell diagram. Until now, however,…

astro-ph.SR2017★ 1 cited

The γ Dor stars as revealed by Kepler : A key to reveal deep-layer rotation in A and F stars

S. J. A. J. Salmon, R. -M. Ouazzani, V. Antoci +2

The γ Dor pulsating stars present high-order gravity modes, which make them important targets in the intermediate-and low-mass main-sequence region of the Hertzsprung-Russell diagr…

astro-ph.SR2017★ 78 cited

Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades

T. R. White, B. J. S. Pope, V. Antoci +20

The most powerful tests of stellar models come from the brightest stars in the sky, for which complementary techniques, such as astrometry, asteroseismology, spectroscopy, and inte…