activity
20162023
most citedPeriodic variable A-F spectral type stars in the northern TESS continuous viewing zone

35 citations · 59 across the 6 of their papers we have counts for

collaborators

6 papers

physics.optics2023

Structural color filters with compensated angle-dependent shifts

Katarína Rovenská, Filip Ligmajer, Beáta Idesová +4

Structural color filters use nano-sized elements to selectively transmit incident light, offering a scalable, economical and environmentally friendly alternative to traditional pig…

astro-ph.SR202235 cited

Periodic variable A-F spectral type stars in the northern TESS continuous viewing zone

M. Skarka, J. Žák, M. Fedurco +11

The goal of our study is to provide a reliable classification of variability of A-F stars brighter than 11 mag located in the northern TESS continuous viewing zone. We also aim at…

physics.optics2021

Correlative electron and light spectroscopy of strongly-coupled mid-infrared plasmon and phonon polaritons

Pavel Gallina, Andrea Konečná, Jiří Liška +2

The ability to control and modify infrared excitations in condensed matter is of both fundamental and application interests. Here we explore a system supporting low-energy excitati…

cond-mat.mes-hall2021

Strong coupling in a Au plasmonic antenna-SiO layer system: a hybrid mode analysis

Pavel Gallina, Michal Kvapil, Jiří Liška +5

A detailed analysis of the optical response of a system accommodating several coupled modes is needed for the complete understanding of the strong coupling effect. In this paper, w…

astro-ph.SR2017

Binary systems with an RR Lyrae component - progress in 2016

J. Liška, M. Skarka, Á. Sódor +1

In this contribution, we summarize the progress made in the investigation of binary candidates with an RR Lyrae component in 2016. We also discuss the actual status of the RRLyrBin…

astro-ph.SR201624 cited

KIC 2831097 - A 2-year orbital-period RR Lyrae binary candidate

Á. Sódor, M. Skarka, J. Liška +1

We report the discovery of a new Kepler first-overtone RR Lyrae pulsator, KIC 2831097. The pulsation shows large, 0.1 d amplitude, systematic phase variations that can be interpret…