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

Galaxy evolution is one of the hot topics in Astrophysics that have shown tangible progress in the last years. This has been mostly due to advent of large telescopes, both ground based and in space, with state-of-the-art instruments, equipped with high sensitive detectors. They have made possible acquiring the deepest surveys in different

The Alpha Magnetic Spectrometer (AMS-02) is a general purpose high energy particle detector that was deployed to the International Space Station (ISS) on May 19, 2011 to conduct a unique long duration mission of fundamental physics research from space. Among the physics objectives of AMS are a search for Dark Matter, Antimatter, the study of

The IAC cosmology group leads the QUIJOTE experiment, which is a unique project in the polarization of the Cosmic Microwave Background, consisting of two telescopes and three instruments. The aim of the present action is the improvement and acquisition of equipment associated with the MFI (Multi-Frequency Instrument) instrument and the microwave

WHY: 2015 has been named by the United Nations as the International Year of Light (light2015.org). Electricity and light have many obvious benefits for human mankind, but they also pose some relevant threats: the every day increasing excess of light thrown by humans to the sky seriously threatens to remove forever one of humanity’s natural wonders