Stellar atmosphere models for Gaia
Welcome to the web page of the Gaia-SAM collaboration, which is devoted to calculating and testing stellar atmosphere models for late-type stars. The aim is to identify the most realistic atmospheric models by comparing calculated observables to highly accurate and well-calibrated observed data. The results of this work will be important for interpreting data from the Gaia mission, but also from other large stellar surveys.For more information on the project see Background in the menu to the left. For a list of collaborators see Contacts in the menu to the left.