Spectral Indices in the NIR for Studying Stellar Populations
So far, detailed stellar population studies, based on the absorption line strengths have been concentrated mainly in the optical spectral range. In this work, we supplement spectral indices of the Lick system in the optical with additional indices in the near-infrared (NIR). We optimised the definition of the indices to be sensitive to the main
Eftekhari, E. et al.
Fecha de publicación:
7
2020