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20122026
most citedThe first view of Scuti and Doradus stars with the TESS mission

125 citations · 1.3k across the 85 of their papers we have counts for

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54 papers · 1 filter

astro-ph.SR2026

Revision of the Detached Eclipsing System IR Cas from TESS Observations, Ground-Based Photometry and Spectroscopy

Matúš Kamenec, Pavol Gajdoš, Martin Vaňko +3

We present a new photometric and spectroscopic analysis of detached eclipsing binary IR Cas based on TESS observations, supplementary ground-based photometry in Sloan , $…

astro-ph.SR2026

Rotational characteristics of five photometrically variable stars

Pavlína Rutová, Marek Skarka, Jiří Žák +1

This study explores photometric variability in a sample of hot stars in order to test whether variability arises from rotational modulation due to surface temperature spots. Freque…

astro-ph.SR2026

Variability classification of TESS targets in LOPS2, the first long-term pointing field of PLATO. Version 1 of the public variability catalogue

Mykyta Kliapets, Pablo Huijse, Jeroen Audenaert +28

The PLAnetary Transits and Oscillations of stars (PLATO) mission is expected to launch in January 2027. A total of 8\% of its data rate will be dedicated to complementary science t…

astro-ph.SR2025

On the origin of sinusoidal brightness variations in F to O-type stars through radial velocities

E. Šipková, M. Skarka, M. Vaňko +3

Stellar variability may originate from various phenomena such as binarity, pulsations, or rotation. These mechanisms can induce flux variations of similar magnitudes, shapes, and p…

astro-ph.SR2025

Flares and superflares on the southern active binary CC Eri

M. Leitzinger, P. Odert, R. Greimel +15

Flares and CMEs are known to be the dominating high-energy phenomena on cool stars. Superflares were thoroughly investigated using broadband photometry predominantly from Kepler, K…

astro-ph.SR2025

Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates

D. Jadlovský, L. Molnár, A. Ercolino +26

The majority of massive stars are part of binary systems that may interact during their evolution. However, not many RSGs are known binaries, and only a few have constrained orbita…

astro-ph.SR2025★ 1 cited

50 Dra: Am-type twins with additional variability in a non-eclipsing system

M. Skarka, J. Lipták, E. Niemczura +5

The interplay between radiative diffusion, rotation, convection, and magnetism in metallic-line chemically peculiar stars is still not fully understood. Recently, evidence has emer…

astro-ph.SR2024★ 8 cited

Spectroscopic observations of flares and superflares on AU Mic

P. Odert, M. Leitzinger, R. Greimel +13

The young active flare star AU~Mic is the planet host star with the highest flare rate from TESS data. Therefore, it represents an ideal target for dedicated ground-based monitorin…

astro-ph.SR2024★ 5 cited

Five new eclipsing binaries with low-mass companions

J. Lipták, M. Skarka, E. Guenther +18

Precise space-based photometry from the Transiting Exoplanet Survey Satellite results in a huge number of exoplanetary candidates. However, the masses of these objects are unknown…

astro-ph.SR2024★ 3 cited

Analysis of KIC 7023917 -- spotted low-mass ratio eclipsing binary with Scuti pulsations

Pavol Gajdoš, Štefan Parimucha, Marek Skarka +3

Times of minima of eclipsing binary KIC 7023917 show quasiperiodic anti-symmetric deviations from the calculated one with an amplitude of up to 10 minutes and a period of 200 - 300…

astro-ph.SR2024★ 8 cited

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

M. Skarka, Z. Henzl

We accurately identify and classify the variability of A-F stars in the southern continuous viewing zone of the TESS satellite. The brightness limit was set to 10 mag to ensure the…

astro-ph.SR2023★ 1 cited

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

D. L. Holdsworth, M. S. Cunha, M. Lares-Martiz +46

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

astro-ph.SR2023★ 4 cited

Everything that glitters is not gold: V1315 Cas is not a dormant black hole

J. Zak, D. Jones, H. M. J. Boffin +11

The quest for quiet or dormant black holes has been ongoing since several decades. Ellipsoidal variables possibly indicate the existence of a very high-mass invisible companion and…

astro-ph.SR2023★ 1 cited

Science with a small two-band UV-photometry mission II: Observations of stars and stellar systems

J. Krtička, J. Benáček, J. Budaj +32

We outline the impact of a small two-band UV-photometry satellite mission on the field of stellar physics, magnetospheres of stars, binaries, stellar clusters, interstellar matter,…

astro-ph.SR2022★ 2 cited

Companions to Kepler giant stars: A long-period eccentric substellar companion to KIC 3526061 and a stellar companion to HD 187878

Marie Karjalainen, Raine Karjalainen, Artie P. Hatzes +12

Context. Our knowledge of populations and occurrence of planets orbiting evolved intermediate-mass stars is still incomplete. In 2010 we started a planet-search program among 95 gi…

astro-ph.SR2022★ 35 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…

astro-ph.SR2021★ 20 cited

A tidally tilted sectoral dipole pulsation mode in the eclipsing binary TIC 63328020

S. A. Rappaport, D. W. Kurtz, G. Handler +13

We report the discovery of the third tidally tilted pulsator, TIC 63328020. Observations with the TESS satellite reveal binary eclipses with an orbital period of 1.1057 d, and …

astro-ph.SR2021★ 3 cited

Orbital solutions derived from radial velocities and time delays for four {\it Kepler} systems with A/F-type (candidate) hybrid pulsators

P. Lampens, L. Vermeylen, Y. Frémat +8

The presence of A/F-type {\it Kepler} hybrid stars extending across the entire Sct- Dor instability strips and beyond remains largely unexplained. In order to better underst…

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.SR2020★ 10 cited

First apsidal motion and light curve analysis of 162 eccentric eclipsing binaries from LMC

P. Zasche, M. Wolf, H. Kučáková +6

We present an extensive study of 162 early-type binary systems located in the LMC galaxy that show apsidal motion and have never been studied before. For the ample systems, we perf…

astro-ph.SR2020★ 5 cited

Rotational modulation and single g-mode pulsation in the B9pSi star HD174356?

Z. Mikulasek, E. Paunzen, S. Huemmerich +19

Chemically peculiar (CP) stars of the upper main sequence are characterised by specific anomalies in the photospheric abundances of some chemical elements. The group of CP2 stars,…

astro-ph.SR2020★ 6 cited

Understanding the rotational variability of K2 targets. HgMn star KIC 250152017 and blue horizontal branch star KIC 249660366

J. Krticka, A. Kawka, Z. Mikulasek +6

Ultraprecise space photometry enables us to reveal light variability even in stars that were previously deemed constant. A large group of such stars show variations that may be rot…

astro-ph.SR2020★ 25 cited

Blazhko effect in the Galactic bulge fundamental mode RR Lyrae stars II: Modulation shapes, amplitudes and periods

M. Skarka, Z. Prudil, J. Jurcsik

The number of stars observed by the Optical Gravitational Lensing Experiment (OGLE) project in the Galactic bulge offers an invaluable chance to study RR Lyrae stars in a statistic…

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…