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20022026
most citedKepler Asteroseismology Program: Introduction and First Results

480 citations · 3.6k across the 52 of their papers we have counts for

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astro-ph.SR2026

Forward Modeling of the Sct Star V1790 Ori: , , Resolution and Non-adiabatic Effects

Xiaoya Sun, Antonio García Hernández, Zhaoyu Zuo +5

We investigate the role of large separation, rotational correction order, structural resolution, and non-adiabatic effects in modelling the rotating Scuti star V1790 Ori. From…

astro-ph.SR2019★ 125 cited

The first view of Scuti and Doradus stars with the TESS mission

V. Antoci, M. S. Cunha, D. M. Bowman +63

We present the first asteroseismic results for Scuti and Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilise the 2-min cadence TESS data for a sample…

astro-ph.SR2017★ 19 cited

Semi-empirical seismic relations of A-F stars from CoRoT and Kepler legacy data

A. Moya, J. C. Suárez, A. García Hernández +1

Asteroseismology is witnessing a revolution thanks to high-precise asteroseismic space data (MOST, CoRoT, Kepler, BRITE), and their large ground-based follow-up programs. Those ins…

astro-ph.SR2017

What CoRoT tells us about δ Scuti stars existence of a regular pattern and seismic indices to characterize stars

Eric Michel, Marc-Antoine Dupret, Daniel Reese +8

Inspired by the so appealing example of red giants, where going from a handful of stars to thousands revealed the structure of the eigenspectrum, we inspected a large homogeneous s…

astro-ph.SR2016★ 51 cited

Spectroscopic Survey of γ Doradus Stars I. Comprehensive atmospheric parameters and abundance analysis of γ Doradus stars

F. Kahraman-Alicavus, E. Niemczura, P. De Cat +11

We present a spectroscopic survey of known and candidate \,Doradus stars. The high-resolution, high signal-to-noise spectra of 52 objects were collected by five different spectr…

astro-ph.SR2014★ 274 cited

Rotation and magnetism of Kepler pulsating solar-like stars. Towards asteroseismically calibrated age-rotation relations

R. A. Garcia, T. Ceillier, D. Salabert +16

Kepler ultra-high precision photometry of long and continuous observations provides a unique dataset in which surface rotation and variability can be studied for thousands of stars…

astro-ph.SR2014★ 68 cited

Measuring mean densities of delta Scuti stars with asteroseismology. Theoretical properties of large separations using TOUCAN

J. C. Suárez, A. García Hernández, A. Moya +4

We aim at studying the theoretical properties of the regular spacings found in the oscillation spectra of delta Scuti stars. We performed a multi-variable analysis covering a wide…

astro-ph.SR2013★ 1 cited

On the necessity of a new interpretation of the stellar light curves

J. Pascual-Granado, R. Garrido, J. C. Suárez

The power of asteroseismology relies on the ability to infer the stellar structure from the unambiguous frequency identification of the corresponding pulsation mode. Hence, the use…

astro-ph.SR2013★ 15 cited

CoRoT 102749568: mode identification in a delta Scuti star based on regular spacings

M. Paparo, Zs. Bognar, J. M. Benko +10

The high accuracy of space data increased the number of the periodicities determined for pulsating variable stars, but the mode identification is still a critical point in the non-…

astro-ph.SR2013★ 45 cited

Asteroseismology of KIC 11754974: a high-amplitude SX Phe pulsator in a 343-day binary system

S. J. Murphy, A. Pigulski, D. W. Kurtz +13

The candidate SX Phe star KIC 11754974 shows a remarkably high number of combination frequencies in the Fourier amplitude spectrum: 123 of the 166 frequencies in our multi-frequenc…

astro-ph.SR2012★ 43 cited

Pulsation spectrum of Delta Sct stars: the binary HD 50870 as seen with CoRoT and HARPS

L. Mantegazza, E. Poretti, E. Michel +14

We present the results obtained with the CoRoT satellite for HD 50870, a Delta Sct star which was observed for 114.4 d. The 307,570 CoRoT datapoints were analysed with different te…

astro-ph.SR2011★ 46 cited

Fundamental properties of five Kepler stars using global asteroseismic quantities and ground-based observations

O. L. Creevey, G. Dogan, A. Frasca +34

We present an asteroseismic study of the solar-like stars KIC 11395018, KIC 10273246, KIC 10920273, KIC 10339342, and KIC 11234888 using short-cadence time series of more than eigh…

astro-ph.SR2011★ 1 cited

Fast Rotating solar-like stars using asteroseismic datasets

R. A. García, T. Ceillier, T. Campante +27

The NASA Kepler mission is providing an unprecedented set of asteroseismic data. In particular, short-cadence lightcurves (~60s samplings), allow us to study solar-like stars cover…

astro-ph.SR2011★ 345 cited

The Kepler characterization of the variability among A- and F-type stars. I. General overview

K. Uytterhoeven, A. Moya, A. Grigahcene +38

The Kepler spacecraft is providing time series of photometric data with micromagnitude precision for hundreds of A-F type stars. We present a first general characterization of the…

astro-ph.SR2011★ 142 cited

Kepler observations of variability in B-type stars

L. A. Balona, A. Pigulski, P. De Cat +27

The analysis of the light curves of 48 B-type stars observed by Kepler is presented. Among these are 15 pulsating stars, all of which show low frequencies characteristic of SPB sta…

astro-ph.SR2010★ 70 cited

Regularities in frequency spacings of Delta Scuti stars: The Kepler star KIC 9700322

M. Breger, L. Balona, P. Lenz +15

In the faint star KIC 9700322 observed by the Kepler satellite, 76 frequencies with amplitudes from 14 to 29000 ppm were detected. The two dominant frequencies at 9.79 and 12.57 c/…

astro-ph.SR2010★ 163 cited

A precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764

T. S. Metcalfe, M. J. P. F. G. Monteiro, M. J. Thompson +55

The primary science goal of the Kepler Mission is to provide a census of exoplanets in the solar neighborhood, including the identification and characterization of habitable Earth-…

astro-ph.SR2010★ 43 cited

Atmospheric parameters and pulsational properties for a sample of \,Sct, \,Dor, and hybrid {\it Kepler} targets

G. Catanzaro, V. Ripepi, S. Bernabei +14

We report spectroscopic observations for 19 \,Sct candidates observed by the {\it Kepler} satellite both in long and short cadence mode. For all these stars, by using spectral s…

astro-ph.SR2010

Towards a detection of individual g modes in the Sun

R. A. Garcia, J. Ballot, A. Eff-Darwich +10

Since the detection of the asymptotic properties of the dipole gravity modes in the Sun, the quest to find the individual gravity modes has continued. A deeper analysis of the GOLF…

astro-ph.SR2010

Asteroseismic study of gamma Doradus members of the cluster NGC 2506

A. Grigahcene, A. Moya, J. -C. Suarez +1

The present work performs an asteroseismic study of a gamma Doradus star member of the open cluster NGC 2506. This work conjugates the observational information of the star and the…

astro-ph.SR2010

Modelling delta Scuti stars using asteroseismic space data

A. Moya, A. García Hernández, J. -C. Suárez +2

In the last years, space missions such as COROT, Kepler or MOST have provided very accurate photometric observational data. In the particular case of Scuti stars, the observed…

astro-ph.SR2010★ 223 cited

Hybrid gamma Doradus - delta Scuti pulsators: New insights into the physics of the oscillations from Kepler observations

A. Grigahcene, V. Antoci, L. Balona +39

Observations of the pulsations of stars can be used to infer their interior structure and test theoretical models. The main sequence Doradus (Dor) and Scuti (Sct) stars wit…

astro-ph.SR2009★ 480 cited

Kepler Asteroseismology Program: Introduction and First Results

Ronald L. Gilliland, T. M. Brown, J. Christensen-Dalsgaard +32

Asteroseismology involves probing the interiors of stars and quantifying their global properties, such as radius and age, through observationsof normal modes of oscillation. The te…

astro-ph.SR2009★ 68 cited

Detection of solar-like oscillations from Kepler photometry of the open cluster NGC 6819

Dennis Stello, Sarbani Basu, Hans Bruntt +49

Asteroseismology of stars in clusters has been a long-sought goal because the assumption of a common age, distance and initial chemical composition allows strong tests of the theor…