The project focuses on the analysis of the scaling-laws of star forming regions in the circumnuclear zone -central kpc- of a sample of six nearby galaxies selected with different star formation morphology (disk, ring or nuclear) and host galaxy type (Sa to EO). The project relies on an unique high-angular resolution dataset that resolves - in the

The project will explore the detection of anomalies in large surveys using deep neural networks.

SHARKS (Southern H-ATLAS Regions Ks-band Survey; IP: Helmut Dannerbauer) is a deep near-infrared survey of a 300-square-degree region of the sky being carried out with the VISTA telescope and its VIRCAM instrument at ESO (European Southern Observatory in Chile) in the Ks-band (at 2 micrometer). With SHARKS we expect to detect about 20-30 million

The dimensions of the instruments in design for the next generation of large telescopes exceed the capacities of the cryogenic and vacuum infrastructures available at the IAC. Cryogenic instrumentation requires a large number of tests to verify its mechanisms and components, as well as of the whole instrument once assembled. These verification

This project is a continuation of the CAMINA project (ProID2017010112). The science objective is the compositional characterization of asteroids, that we have been doing by means of three actions: (1) our participation in the two space missions that have visited and taken a sample of material from two near-Earth asteroids (NEAs), OSIRIS-REx (NASA)

Massive stars are key astronomical objects for the study of the Universe through spaceand time. Ensuring reliable knowledge about the physical properties, evolution, and feedback of massive stars is of utmost importance forseveral topics at the forefront of modern astrophysics, including, e.g., chemodynamical evolution of galaxies, the reionization