Showing 1–20 of 38 results
/ Date/ Name
Jan 25, 2021The Araucaria Project: Deep near-infrared photometric maps of Local and Sculptor Group galaxies. I. Carina, Fornax, SculptorJun 10, 2023Period-Luminosity Relations for Galactic classical Cepheids in the Sloan bandsJun 24, 2024Projection factor and radii of Type II CepheidsMar 28, 2023Synthetic Population of Binary Cepheids. II. The effect of companion light on the extragalactic distance scaleMay 8, 2021Studies of RR Lyrae Variables in Binary Systems. I.: Evidence of a Trimodal Companion Mass DistributionMar 19, 2024Cepheids with giant companions. II. Spectroscopic confirmation of nine new double-lined binary systems composed of two CepheidsApr 1, 2022Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companionsNov 9, 2015The Araucaria Project: A study of the classical Cepheid in the eclipsing binary system OGLE LMC562.05.9009 in the Large Magellanic CloudMar 1, 2025Non-evolutionary effects on period change in Magellanic Cepheids II. Empirical constraints on non-linear period changesDec 15, 2025HALO I: Photometric continuum reverberation mapping of Fairall 9Dec 6, 2018Wind Roche Lobe Overflow as a way to make type Ia supernova from the widest symbiotic systemsFeb 1, 2019Testing systematics of Gaia DR2 parallaxes with empirical surface brightness -- color relations applied to eclipsing binariesMay 13, 2018The late type eclipsing binaries in the Large Magellanic Cloud: catalogue of fundamental physical parametersDec 22, 2021An absolute calibration of the near-infrared Period-Luminosity Relations of Type II Cepheids in the Milky Way and in the Large Magellanic CloudMay 20, 2016The Araucaria Project. On the Tip of the Red Giant Branch distance determination to the Magellanic CloudsSep 2, 2017The Araucaria Project. The Distance to the Sculptor Group Galaxy NGC 7793 from Near-Infrared Photometry of Cepheid VariablesJun 4, 2018The Araucaria Project: High-precision Cepheid astrophysics from the analysis of variables in double-lined eclipsing binariesNov 4, 2025Secondary standards in the UKIRT faint standard fieldsOct 17, 2020A distance determination to the Small Magellanic Cloud with an accuracy of better than 2 percent based on late-type eclipsing binary starsJan 22, 2020Empirical calibration of the reddening maps in the Magellanic Clouds