activity
20242026
collaborators

9 papers

astro-ph.GA2026

Reddening maps of the Magellanic Clouds using spectral energy distribution fitting of red giants

H. Netzel, G. Pietrzyński, M. Górski +9

Robust reddening maps of the Large and Small Magellanic Clouds (LMC/SMC) are crucial for a wide range of astrophysical studies, including the calibration of the cosmic distance lad…

astro-ph.SR2026

Finding the elusive RR Lyrae companions via speckle imaging

R. Salinas, V. Kalari, G. Hajdu +25

Despite their key role in astrophysics, the binary properties of RR Lyrae stars (RRL) remain almost completely unknown since only a single RRL is confirmed as belonging to a binary…

astro-ph.SR2026

Period-Luminosity Relations, projection factor and radii of Anomalous Cepheids

Piotr Wielgórski, Grzegorz Pietrzyński, Wolfgang Gieren +24

Anomalous Cepheids are radially pulsating stars observed in dwarf galaxies, the Galactic bulge and halo, and globular clusters. Similarly to other radially pulsating stars, they ca…

astro-ph.SR2025

X-ray properties of RR Lyrae and Cepheid variables from eROSITA

Krystian Ilkiewicz, Henryka Netzel

We present a search for X-ray counterparts to RR Lyrae and Cepheid variables using data from the first eROSITA all-sky survey. We identify seven RR Lyrae and eight Cepheid variable…

astro-ph.SR2025

Exploring Low-Amplitude Variability in First Overtone Cepheids with TESS

E. Plachy, H. Netzel, A. Bódi

Classical Cepheid stars that pulsate in the first overtone radial mode often exhibit additional periodicities at the millimagnitude level. Extensive studies of the OGLE data of the…

astro-ph.EP2025

The changing transit shape of TOI-3884 b

Hritam Chakraborty, Jose M. Almenara, Monika Lendl +9

TOI-3884 b is a sub-Saturn transiting a fully convective M-dwarf. Observations indicate that the transit shape is chromatic and asymmetric as a result of persistent starspot crossi…