We propose to investigate fundamental questions concerning the formation and evolution of galaxies, from the smallest galactic scales to those of large spiral galaxies, by adopting the approach of galactic archaeology. By determining the ages, metallicities and kinematics of individual stars, in particular low-mass stars, whose life-times are

Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch (AGB) - just before they form planetary nebulae (PNe) - where they experience complex nucleosynthetic and molecular processes. AGB stars also experience strong mass loss, efficiently

Contract Ramón y Cajal to develop his research work in the specific research project "Feeding and hiding the monster: Triggering and obscuring the central engine of active galaxies"

CVOPTICON is an Integrated Infrastructure Initiative of the 6th EU I+D+i framework programme for improving the coordination of the European astronomical community in the fields of infrared, optics and solar physics. The OPTICON project which is coordinated by the University of Cambridge and financed by the European Commission, has the objective of

This grant is aimed at providing the IAC with the necessary equipment to have a leading optical laboratory to support and enable the necessary developments for all the future projects at IAC, moreover the creation of a production centre for optical elements up to 40-45 cm in diameter, which represents a first stage of development that aims to

Contract Ramón y Cajal to develop his research work in the specific research project "Heavily Dust Obscured Star Forming Galaxies in the Early Universe"