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20152025
most citedThe asteroseismic potential of TESS: exoplanet-host stars

134 citations · 460 across the 7 of their papers we have counts for

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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR2025★ 7 cited

Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel Mission Candidate Sample

M. Tsantaki, L. Magrini, C. Danielski +15

The next mission dedicated to the study of planetary atmospheres is the Ariel space mission, planned for launch in 2029, which will observe a variety of planetary systems belonging…

astro-ph.SR2022★ 91 cited

Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra

Gaia Collaboration, P. Montegriffo, M. Bellazzini +27

Gaia Data Release 3 provides novel flux-calibrated low-resolution spectrophotometry for about 220 million sources in the wavelength range 330nm - 1050nm (XP spectra). Synthetic pho…

astro-ph.SR2018★ 101 cited

Establishing the accuracy of asteroseismic mass and radius estimates of giant stars. I. Three eclipsing systems at [Fe/H]~ -0.3 and the need for a large high-precision sample

K. Brogaard, C. J. Hansen, A. Miglio +12

We aim to establish and improve the accuracy level of asteroseismic estimates of mass, radius, and age of giant stars. This can be achieved by measuring independent, accurate, and…

astro-ph.SR2016★ 134 cited

The asteroseismic potential of TESS: exoplanet-host stars

T. L. Campante, M. Schofield, J. S. Kuszlewicz +14

New insights on stellar evolution and stellar interiors physics are being made possible by asteroseismology. Throughout the course of the Kepler mission, asteroseismology has also…

astro-ph.SR2015

Constraining angular momentum transport processes in stellar interiors with red-giant stars in the open cluster NGC6819

N. Lagarde, A. Miglio, P. Eggenberger +2

Clusters are excellent test benches for verification and improvement of stellar evolution theory. The recent detection of solar-like oscillations in G-K giants in the open cluster…