activity
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

collaborators

86 papers

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.IM2026

ASTRAFier: A Novel and Scalable Transformer-based Stellar Variability Classifier

Paul F. X. Gregory, Jeroen Audenaert, Mykyta Kliapets +5

Photometric missions such as Kepler and TESS have generated millions of light curves covering almost the entire sky, offering unprecedented opportunities to study stellar variabili…

astro-ph.EP2026★ 1 cited

Unraveling the Brown Dwarf Desert: Four New Discoveries and a Unifying, Period-Coded Picture

Ján Šubjak, Rafael Brahm, Jozef Lipták +30

We present four newly validated transiting brown dwarfs identified through TESS photometry and confirmed with high-precision radial velocity measurements obtained from the FEROS an…

astro-ph.EP2026

Aligned, Misaligned and Polar Orbits of Hot Jupiters: Measuring Spin-Orbit Angles via Doppler Tomography with HARPS-N

Z. Balkóová, J. Žák, M. Skarka +4

Although the migration of hot Jupiters is not yet fully understood, measurements of the projected spin-orbit angle λ help shed light on the processes involved. Here we present Dopp…

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.IM2025★ 3 cited

The evolution of PUCHEROS from a basic to a competitive tool for stellar astrophysics

Luca Antonucci, Leonardo Vanzi, Abner Zapata +16

We present PUCHEROS +, a new spectrograph developed as an enhanced version of PUCHEROS (Pontificia Universidad Catolica High Echelle Resolution Optical Spectrograph), which was the…

astro-ph.IM2025★ 2 cited

PLATOSpec: a precise spectrograph in support of space missions

P. Kabáth, M. Skarka, A. Hatzes +42

The upcoming space missions that will characterize exoplanets, such as PLATO and Ariel, will collect huge amounts of data that will need to be complemented with ground-based observ…

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.EP2025★ 1 cited

PLATOSpec's first results: planets WASP-35b and TOI-622b are on aligned orbits, and K2-237b is on a polar orbit

J. Zak, P. Kabath, H. M. J. Boffin +10

The spin-orbit angle between a stellar spin axis and its planetary orbital axis is a key diagnostic of planetary migration pathways, yet the mechanisms shaping the observed spin-or…

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.HE2025

Disentangling the stellar atmosphere and the focused wind in different accretion states of Cygnus X-1

M. Brigitte, P. Hadrava, B. Kubátová +8

In high-mass X-ray binaries (HMXBs), the compact object accretes the strong stellar wind of an O-B supergiant companion star. X-ray flux variations alter the stellar wind's ionizat…

astro-ph.EP2025★ 10 cited

Stellar obliquities of eight close-in gas giant exoplanets

J. Zak, H. M. J. Boffin, E. Sedaghati +4

The Rossiter-McLaughlin effect allows us to measure the projected stellar obliquity of exoplanets. From the spin-orbit alignment, planet formation and migration theories can be tes…

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.EP2024★ 10 cited

TOI-4504: Exceptionally large Transit Timing Variations induced by two resonant warm gas giants in a three planet system

Michaela Vítková, Rafael Brahm, Trifon Trifonov +24

We present a joint analysis of TTVs and Doppler data for the transiting exoplanet system TOI-4504. TOI-4504 c is a warm Jupiter-mass planet that exhibits the largest known transit…

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.EP2024★ 23 cited

TOI-1408: Discovery and Photodynamical Modeling of a Small Inner Companion to a Hot Jupiter Revealed by TTVs

Judith Korth, Priyanka Chaturvedi, Hannu Parviainen +60

We report the discovery and characterization of a small planet, TOI-1408 c, on a 2.2-day orbit located interior to a previously known hot Jupiter, TOI-1408 b ( d, $M=1.86\p…

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.EP2024

Stellar obliquity measurements of six gas giants

J. Zak, A. Bocchieri, E. Sedaghati +11

One can infer the orbital alignment of exoplanets with respect to the spin of their host stars using the Rossiter-McLaughlin effect, thereby giving us the chance to test planet for…

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…