Stellar population models based on new generation stellar library
The spectral predictions of stellar population models are not as accurate in the ultra-violet (UV) as in the optical wavelength domain. One of the reasons is...
Stellar population models in the UV: I. Characterisation of the New Generation Stellar Library
We have fully characterized the NGSL stellar spectral library, which allows us to open the UV stellar spectral range for stellar population studies. We have...
Stellar population study in early-type galaxies: an approach from the K band
A full understanding of the physical properties of integrated stellar systems demands a multiwavelength approach since each spectral window shows us the...