The objective of the Juan de la Cierva-formacion grants is to promote the hiring of people with a doctorate degree by research organizations in Spain for a period of two years in order to strengthen the skills acquired during a first stage of postdoctoral training in a different center from the one where they completed their PhD. The annual amount

The objective of the Juan de la Cierva-training grants is to promote the hiring of work by research organizations or centros i+D españoles other than those in which they carried out their pre-doctoral training. The aids whose annual amount is 26,300 euros, are used to co-finance the salary and the business contribution of Social Security of the

The objective of the Juan de la Cierva-formacion grants is to promote the hiring of people with a doctorate degree by research organizations in Spain for a period of two years in order to strengthen the skills acquired during a first stage of postdoctoral training in a different center from the one where they completed their PhD. The annual amount

The objective of the Juan de la Cierva-training grants is to promote the hiring of work by research organizations or Spanish i+D centers other than those in which they carried out their pre-doctoral training. The aids whose annual amount is 26,300 euros, are used to co-finance the salary and the business contribution of Social Security of the

The aim of NanoSpace is to determine the abundance, formation mechanisms and astrochemical role of carbonaceous nanoparticles in space. Carbon is ubiquitous in space; from small carbon and hydrocarbon molecules to fullerenes and large but currently unidentified polycyclic aromatic hydrocarbons, carbonaceous dust particles and ultimately life. The

Galaxy discs are made of two components, the thin and the thick disc. Thick discs contain up to 50% of the baryonic mass of a galaxy. Because their stars are among the oldest in the Universe, thick discs are relics of the infancy of galaxies. Thus, understanding the origin of thick discs is key to unveil how galaxies themselves form, which in turn