activity
20132021
most citedAn eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent

691 citations · 779 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR202119 cited

An absolute calibration of the near-infrared Period-Luminosity Relations of Type II Cepheids in the Milky Way and in the Large Magellanic Cloud

Piotr Wielgórski, Grzegorz Pietrzyński, Bogumił Pilecki +29

We present time-series photometry of 21 nearby Type II Cepheids in the near-infrared J, H and Ks passbands. We use this photometry, together with the Third Gaia Early Data Release…

astro-ph.SR201649 cited

The occurrence of Binary Evolution Pulsators in the classical instability strip of RR Lyrae and Cepheid variables

P. Karczmarek, G. Wiktorowicz, K. Iłkiewicz +5

Single star evolution does not allow extremely low-mass stars to cross the classical instability strip (IS) during the Hubble time. However, within binary evolution framework low-m…

astro-ph.GA2016

OGLE Collection of Star Clusters. New Objects in the Outskirts of the Large Magellanic Cloud

M. Sitek, M. K. Szymański, D. M. Skowron +13

The Magellanic System (MS), consisting of the Large Magellanic Cloud (LMC), the Small Magellanic Cloud (SMC) and the Magellanic Bridge (MBR), contains diverse sample of star cluste…

astro-ph.SR201620 cited

A solar twin in the eclipsing binary LL Aqr

D. Graczyk, R. Smolec, K. Pavlovski +11

In the course of a project to study eclipsing binary stars in vinicity of the Sun, we found that the cooler component of LL Aqr is a solar twin candidate. This is the first known s…

astro-ph.GA2013691 cited

An eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent

G. Pietrzyński, D. Graczyk, W. Gieren +25

In the era of precision cosmology it is essential to determine the Hubble Constant with an accuracy of 3% or better. Currently, its uncertainty is dominated by the uncertainty in t…