Magnetic fields are primary drivers of stellar formation and have profound implications on stellar evolution (on the transport of chemical species and angular momentum), as well as on the formation of planetary systems around the hosting star. Yet, stellar magnetic fields are often overlooked since they are elusive, difficult to detect, and

The ALBA Network: The first Lights of the Universe, intends to detect the first sources to appear in the Universe. The ALBA collaboration started from a sub-group of researchers from the Consolider-Ingenio2010 project (CSD2006-00070): First science with the GTC, whose principal Investigator was the PI of this Red Temática. The ALBA collaboration

The aim of this project is to combine two unique datasets, the nine Planck all-sky (30-857 GHz) maps and the four QUIJOTE Northern sky (10-20 GHz) maps, to provide the best possible characterization of the physical properties of polarized emissions in the microwave domain, together with an unprecedentedly thorough description of the intensity

The main goal of this project is to ensure the scientific exploitation of the experiments, missions and surveys in which the Cosmology group at the IAC is involved in the period 2015-2017: PLANCK, QUIJOTE and SDSS (BOSS and eBOSS). The specific goals of this project are: I) To continue the scientific exploitation of the PLANCK mission during the

The main goal of this project is to ensure the scientific and technical participation of IAC and UPCT in the ESA space mission EUCLID (Cosmic Vision Program) during the period 2016-2018. In particular, the spanish scientific participation includes researchers belonging to IAC, UPCT, IFCA, CAB, IFT, Univ. of Salamanca and CEFCA. Currently, the NISP

This is a proposal to construct a new building with 3 floors and basement, to be built in the same plot where the current headquarters are located, and that would include 50 new offices, meeting rooms, services and facilities.