activity
20162021
most citedA distance to the Large Magellanic Cloud that is precise to one per cent

686 citations · 755 across the 4 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2021

The Araucaria Project. Distances to Nine Galaxies Based on a Statistical Analysis of their Carbon Stars (JAGB Method)

Bartłomiej Zgirski, Grzegorz Pietrzyński, Wolfgang Gieren +13

Our work presents an independent calibration of the J-region Asymptotic Giant Branch (JAGB) method using Infrared Survey Facility (IRSF) photometric data and a custom luminosity fu…

astro-ph.GA20213 cited

The Araucaria Project: Deep near-infrared photometric maps of Local and Sculptor Group galaxies. I. Carina, Fornax, Sculptor

Paulina Karczmarek, Grzegorz Pietrzyński, Wolfgang Gieren +12

Deep near-infrared - and -band photometry of three Local Group dwarf spheroidal galaxies: Fornax, Carina, and Sculptor, is made available for the community. Until now, these…

astro-ph.GA2020

A distance determination to the Small Magellanic Cloud with an accuracy of better than 2 percent based on late-type eclipsing binary stars

Dariusz Graczyk, Grzegorz Pietrzynski, Ian B. Thompson +17

We present a new study of late-type eclipsing binary stars in the Small Magellanic Cloud (SMC) undertaken with the aim of improving the distance determination to this important gal…

astro-ph.GA202057 cited

Empirical calibration of the reddening maps in the Magellanic Clouds

Marek Gorski, Bartlomiej Zgirski, Grzegorz Pietrzynski +9

We present reddening maps of the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC), based on color measurements of the red clump. Reddening values of our maps were obta…

astro-ph.SR20199 cited

Towards early-type eclipsing binaries as extragalactic milestones: I. Physical parameters of OGLE-LMC-ECL-22270 and OGLE-LMC-ECL-06782

Mónica Taormina, G. Pietrzyński, B. Pilecki +11

In this first paper of the series we describe our project to calibrate the distance determination method based on early-type binary systems. The final objective is to measure accur…

astro-ph.SR2019

Candidates for non-pulsating stars located in the Cepheid instability strip in the Large Magellanic Cloud based on Strömgren photometry

W. Narloch, G. Pietrzyński, Z. Kołaczkowski +14

We present candidates for non-pulsating stars lying in the classical Cepheid instability strip based on OGLE photometric maps combined with Strömgren photometry obtained with the 4…