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20222026
most citedSurface brightness-colour relations of dwarf stars from detached eclipsing binaries -- I. Calibrating sample

8 citations · 12 across the 6 of their papers we have counts for

collaborators

6 papers

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.SR2026

The Bochum Survey of the Southern Galactic Disk: III. Complete Data Release

Julia Blex, Moritz Hackstein, Christian Westhues +6

The Southern Galactic Disk Survey (GDS) monitored a mosaic of 268 fields along a -wide stripe in the southern Galactic disk with simultaneous observations in and …

astro-ph.SR2024★ 4 cited

The Infrared Surface Brightness technique applied to RR Lyrae stars from the solar neighborhood

Bartłomiej Zgirski, Wolfgang Gieren, Grzegorz Pietrzyński +9

The Baade-Wesselink method allows us to estimate distances to individual pulsating stars. Accurate geometric parallaxes obtained by the Gaia mission serve us in the calibration of…

astro-ph.SR2024

Projection factor and radii of Type II Cepheids

Piotr Wielgórski, Grzegorz Pietrzyński, Wolfgang Gieren +14

Type II Cepheids are old pulsating stars that can be used to trace the distribution of an old stellar population and to measure distances to globular clusters and galaxies within s…

astro-ph.SR2022★ 8 cited

Surface brightness-colour relations of dwarf stars from detached eclipsing binaries -- I. Calibrating sample

D. Graczyk, G. Pietrzyński, C. Galan +19

Surface brightness -- colour relations (SBCRs) are very useful tools for predicting the angular diameters of stars. They offer the possibility to calculate very precise spectrophot…