Abstract We have obtained [Mg/Fe] measurements for 76.3 per cent of the stars in the Mid-
resolution Isaac Newton Telescope Library of Empirical Spectra (MILES) spectral library …

We present models that predict spectra of old-and intermediate-aged stellar populations at
2.51 Å (FWHM) with varying [α/Fe] abundance. The models are based on the MILES library …

We present a new library of semi-empirical stellar spectra that is based on the empirical
Medium resolution Isaac Newton Library of Empirical Spectra (MILES) library. A new, high …

We present a catalog of Fe, Mg, Si, Ca, and Ti abundances for 2961 stars in eight dwarf
satellite galaxies of the Milky Way (MW): Sculptor, Fornax, Leo I, Sextans, Leo II, Canes …

We have obtained high-resolution spectra of 23 very metal-poor stars and present an
abundance analysis for 19 of these for elements between Mg and Eu. The sample …

Historically, photometry has been largely used to identify stellar populations [multiple
populations (MPs)] in globular clusters (GCs) by using diagrams that are based on colours …

A method that is widely used to analyse stellar populations in galaxies is to apply the
theoretically derived responses of stellar spectra and line indices to element abundance …

Using narrow-band indices observed with the Cambridge spectrophotometer and analysed
using synthetic spectra computed from model atmospheres, the iron abundances of a further …

We present atmospheric parameters for about 300 stars of different chemical composition,
whose spectra will be used to study the galactic enrichment of Fe and light elements. These …

We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity
stellar populations (SSPs) covering the full optical spectral range at moderately high …