The Transiting Exoplanet Survey Satellite (TESS) is a NASA mission that started scientific operations in July 2018. Over two years it will cover the entire sky...
Unravelling the dark universe from the Canary Island observatories - UNDARK
Astrophysical and cosmological observations imply that only 5% of the energy of the Universe is made of conventional matter. The rest is composed by a new type...
UNVEILING THE COMPLEXITY OF RADIO FOREGROUNDS FOR THE DETECTABILITY OF THE CMB POLARIZATION B-MODE
The aim of RadioForegroundsPlus is to combine the nine Planck all-sky (30-857 GHz) maps, with three unique low-frequency data sets: the QUIJOTE maps (at 11, 13...
Unveiling the missing populations of X-ray binaries: dormant black holes and ultra-compact systems
X-ray binaries are excellent laboratories to study the physics of relativistic stars. On the one hand, they provide robust evidence for the existence of black...
VISION HOLISTICA DE LA EVOLUCION DE LA VIA LACTEA DEL PROGRAMA ATRAE EN EL MARCO DEL PROGRAMA ESTATAL PARA DESARROLLAR, ATRAER Y RETENER TALENTO DEL PLAN ESTATAL DE INVESTIGACIÓN CIENTÍFICA, TÉCNICA Y DE INNOVACIÓN 21-23
Within the general objective of enhancing the competitiveness of SECTI agents, this call specifically promotes the incorporation of consolidated talent in...
Weave: Cluster Surveys: A New Vision of the role of the environment in Galazy Evolution
The environment plays a key role in the formation and evolution of galaxies. Clusters of galaxies are the most massive and virialized structures known in the...
WEAVE: Exploring the Cosmic Original Symphony, from Stars to galaxy clusters
WEAVE-ECOS is an unoriented research project that integrates two senior researchers and their team in order to efficiently exploit the first science data from...
Accreting black-holes and neutron stars in X-ray binaries provide an ideal laboratory for exploring the physics of compact objects, yielding not only...
BRIDGES - Ultracool dwarfs modeling: the bridge between planets and stars
BRIDGES main aim is the study of physical properties of the atmospheres ultracool dwarfs andexoplanets, modelling their spectra and comparison them with...