activity
20172021
most citedThe first view of Scuti and Doradus stars with the TESS mission

125 citations · 375 across the 11 of their papers we have counts for

collaborators

13 papers

astro-ph.SR202110 cited

KIC 12602250: A low-amplitude Double-mode Scuti star with Amplitude Modulation

Chenlong Lv, Ali Esamdin, Xiangyun Zeng +3

We propose for the first time that KIC 12602250 is a low-amplitude radial double-mode Scuti star with amplitude modulation. The detailed frequency analysis is given for the lig…

astro-ph.SR202115 cited

Study of rotational splittings in ~Scuti stars using pattern finding techniques

A. Ramón-Ballesta, A. García Hernández, J. C. Suárez +3

Detecting and understanding rotation in stellar interiors is nowadays one of the unsolved problems in stellar physics. Asteroseismology has been able to provide insights on rotatio…

astro-ph.SR202135 cited

TESS Cycle 1 observations of roAp stars with 2-min cadence data

D. L. Holdsworth, M. S. Cunha, D. W. Kurtz +41

We present the results of a systematic search for new rapidly oscillating Ap (roAp) stars using the 2-min cadence data collected by the Transiting Exoplanet Survey Satellite (TESS)…

astro-ph.HE20213 cited

Searching for signatures of chaos in gamma-ray light curves of selected Fermi-LAT blazars

O. Ostapenko, M. Tarnopolski, N. Żywucka +1

Blazar variability appears to be stochastic in nature. However, a possibility of low-dimensional chaos was considered in the past, but with no unambiguous detection so far. If pres…

astro-ph.SR202045 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.SR20208 cited

Self-consistent method to extract non-linearities from pulsating stars light curves I. Combination frequencies

M. Lares-Martiz, R. Garrido, J. Pascual-Granado

Combination frequencies are not solutions of the perturbed stellar structure equations. In dense power spectra from a light curve of a given multi-periodic pulsating star, they can…