activity
20142019
most citedPlanetary Candidates Observed by Kepler V: Planet Sample from Q1-Q12 (36 Months)

188 citations · 818 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR201959 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…

astro-ph.SR201974 cited

Period spacings of Doradus pulsators in the \textit{Kepler} field: Rossby and gravity modes in 82 stars

Gang Li, Timothy Van Reeth, Timothy R. Bedding +2

Rossby modes are the oscillations in a rotating fluid, whose restoring force is the Coriolis force. They provide an additional diagnostic to understand the rotation of stars, which…

astro-ph.SR2017100 cited

First Results From The Hertzsprung Song Telescope: Asteroseismology Of The G5 Subgiant Star {\Mu}Her

F. Grundahl, M. Fredslund Andersen, J. Christensen-Dalsgaard +26

We report the first asteroseismic results obtained with the Hertzsprung SONG Telescope from an extensive high-precision radial-velocity observing campaign of the subgiant muHerculi…

astro-ph.SR201655 cited

Do A-type stars flare?

M. G. Pedersen, V. Antoci, H. Korhonen +5

For flares to be generated, stars have to have a sufficiently deep outer convection zone (F5 and later), strong large--scale magnetic fields (Ap/Bp-type stars) or strong, radiative…

astro-ph.SR201657 cited

Pulsation versus metallicism in Am stars as revealed by LAMOST and WASP

B. Smalley, V. Antoci, D. L. Holdsworth +13

We present the results of a study of a large sample of A and Am stars with spectral types from LAMOST and light curves from WASP. We find that, unlike normal A stars, Sct pulsa…

astro-ph.SR2016136 cited

A new asteroseismic diagnostic for internal rotation in Doradus stars

Rhita-Maria Ouazzani, S. J. A. J. Salmon, V. Antoci +3

With four years of nearly-continuous photometry from Kepler, we are finally in a good position to apply asteroseismology to Doradus stars. In particular several analyses have d…