activity
20122026
most citedGaia-DR2 extended kinematical maps. Part II: Dynamics in the Galactic disk explaining radial and vertical velocities

36 citations · 119 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026

A machine learning approach to estimating HI deficiency in galaxies

Filip Janák, Boris Deshev, Roman Nagy +1

Measurements of the HI content of galaxies serve as an important tracer for probing the impact of environment on galaxy evolution. More specifically, the HI deficiency (defined as…

astro-ph.GA2025★ 1 cited

Comparing radial migration in dark matter and MOND regimes

R. Nagy, F. Janák, M. Šturc +2

Multiple studies on radial migration in disc galaxies have proven the importance of the effect of resonances with non-axisymmetric components on the evolution of galactic discs. Ho…

astro-ph.GA2024

Deep Learning-based Detection and Segmentation of Edge-on and Highly Inclined Galaxies

Z. Chrobakova, V. Kresnakova, R. Nagy +2

Edge-on galaxies have many important applications in galactic astrophysics, but they can be difficult to identify in vast amounts of astronomical data. To facilitate the search for…

astro-ph.IM2022

Per aspera ad astra simul: Through difficulties to the stars together

David Jones, Petr Kabath, Jorge Garcia-Rojas +5

In this article, we detail the strategic partnerships "Per Aspera Ad Astra Simul" and "European Collaborating Astronomers Project: España-Czechia-Slovakia". These strategic partner…

astro-ph.GA2022★ 25 cited

Warp and flare of the Galactic disc revealed with supergiants by Gaia EDR3

Ž. Chrobáková, R. Nagy, M. López-Corredoira

The outer Galactic disc contains some features such as the warp and flare, whose origin is still debated. The Gaia data provide an excellent opportunity to probe the Galactic disc…

astro-ph.GA2020★ 23 cited

Gaia-DR2 extended kinematical maps. Part III: Rotation curves analysis, dark matter, and Modified Newtonian dynamics tests

Ž. Chrobáková, M. López-Corredoira, F. Sylos Labini +2

Recent statistical deconvolution methods have produced extended kinematical maps in a range of heliocentric distances that are a factor of two to three larger than those analysed i…