In the last two decades, Spain has built up a strong infrared community which have successfully contributed, at Co-I level, to the construction and to the scientific exploitation of basically all European InfraRed (IR) space instruments. The IAC has contributed to the construction of infrared instruments for the space telescopes ISO (ISOPHOT-S) and

Multiple communities are now interested in NEOs for very different reasons ranging from science to planetary defence and commercial objectives (e.g., mining). Given the shared scientific and technological basis, all of these communities require knowledge and modelling capabilities of asteroid properties, as well as the capability to perform close

The NRT (New Robotic Telescope) is a project to design and build a 4-meter telescope within five years, which from the ORM will operate in a totally autonomous and robotic way. This form of operation will make it the largest robotic telescope in the world and, together with the exceptional conditions for astronomical observation of the ORM, in the

Based on statistics provided by the Kepler space mission and searches performed with Doppler techniques, super-Earth and Earth-like exoplanets (Rp ~ 0.8-2 times the Earth radius) could exist in about 10-20% of the Sun-like stars and potentially in more than 50% of the stars smaller than the Sun. Despite this, we still do not know which stars in the

Our theoretical understanding of cosmology is, a priori, inconsistent with observations. In a Universe dominated by dark matter, the most massive galaxies are expected to form late and slowly, which is in contradiction with observations whose behavior is just the opposite. In a scenario where our theoretical conception of the Universe is in

The final goal of this project is to guarantee the scientific explotation of the data coming from the QUIJOTE and GroundBIRD experiments, both currently located at the Teide Observatory with the aim of performing highaccuracy observations of the Cosmic Microwave Background (CMB) polarisation.The final goal of these observations is the detection of