activity
19982024
most citedHybrid gamma Doradus - delta Scuti pulsators: New insights into the physics of the oscillations from Kepler observations

223 citations · 1.8k across the 32 of their papers we have counts for

collaborators

33 papers

astro-ph.SR2024

Double-Mode RR Lyrae Stars Observed by K2: Analysis of High-Precision Kepler Photometry

James M. Nemec, Amanda F. Linnell Nemec, Pawel Moskalik +4

The results of a Fourier analysis of high-precision Kepler photometry of 75 double-mode RR~Lyrae (RRd) stars observed during NASA's K2 Mission (2014-18) are presented. Seventy-two…

astro-ph.SR2021

K2 Observations of Galactic RRd Stars

Paweł Moskalik, James M. Nemec, László Molnár +3

We have analysed high-precision photometry of 77 double-mode RR Lyrae (RRd) stars observed by NASA's Kepler-K2 mission during Campaigns 1-18. Among those stars, we have identified…

astro-ph.SR2021★ 7 cited

Four 'Peculiar' RRd Stars Observed by K2

James M. Nemec, Pawel Moskalik

Four stars pulsating simultaneously with a dominant period (0.28,0.39) d and an {\it additional} period (0.20,0.27) d have been identified from among the more t…

astro-ph.SR2020★ 45 cited

TESS observations of Cepheid stars: first light results

E. Plachy, A. Pál, A. Bódi +33

We present the first analysis of Cepheid stars observed by the TESS space mission in Sectors 1 to 5. Our sample consists of 25 pulsators: ten fundamental mode, three overtone and t…

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.SR2019★ 59 cited

Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2

M. S. Cunha, V. Antoci, D. L. Holdsworth +36

We present the first results from the Transiting Exoplanet Survey Satellite (TESS) on the rotational and pulsational variability of magnetic chemically peculiar A-type stars. We an…