The main goal of the Araucaria Project is to improve the calibration of the cosmic distance scale in the local Universe. We trace down environmental dependencies on the brightness of various standard candles by comparing distances to their host galaxies and clusters, obtained with different methods.
Discover our most recent results:
Other important results:
- RR Lyrae stars in binary systems have companions with masses showing trimodal distribution — paper
- Metallicity affects the Leavitt Law for Classical Cepheids in the Milky Way and Magellanic Clouds — paper
- The surface brightness-colour relations based on eclipsing binary stars and calibrated with Gaia EDR3 — paper
- Metallicities and ages for 35 star clusters and their surrounding fields in the Small Magellanic Cloud — paper
- Deep near-infrared photometric maps of Carina, Fornax, and Sculptor — paper — photometric maps
- Period-luminosity relation for classical Cepheids in the Milky Way from Gaia parallaxes — paper
See our team’s activities:
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