Ponente
Descripción
Since its launch, the James Webb Space Telescope (JWST) has opened a new window to study the universe in the infrared with an unprecedented combination of high spatial and spectral resolution. Its spectral capabilities, thanks to the use of integral field spectroscopy (IFS) in both the near and the mid-infrared, allow to analyse the complex interplay between gas, dust, ices and molecules in multiple systems across different scales.
In this talk, I will present the results from the programs MIri Characterization Of Nearby Infrared galaxy Centers (MICONIC) and the GATOS survey. These programs have obtained spatially resolved 5-28micron observations of several local galaxies using the MIRI spectrograph. I will also present the future work on the study of the properties of trans-Neptunian objects with NIRSpec data.