Astronomia UDP

Proyectos

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In this project, we compile a catalog of high-redshift (z>5.5) quasars candidates to be followed up by 4MOST as part of the

This project focuses on understanding several physical properties of powerful quasars showing strong radio emission (radio-loud) in the Epoch of Reionization (z~6).

Supernovae are among the most energetic explosions in the Universe, they are extremely important for studying high energy physics, stellar evolution and

Distant comets are recently discovered comets that show activity (coma and/or tail) well beyond the water sublimation limit at 5 au. These

Collaboration between UDP and the astronomy group of Prof. Gregory Herczeg at the Kavli Institute for Astronomy and Astrophysics at the University of

An extension of the ODISEA survey to Band-4 and Band-8 to investigate disk sizes, and substructures, and derive benchmark disk properties (masses, 

We are characterizing the massive and IR bright protoclusters discovered by the SPT SMG survey of the southern sky. We are studying

The ALMA CRISTAL large program (PI: R. Herrera-Camus; co-PIs: M. Aravena, J. González-López et al.) is designed to provide unique constraints on

The main objectives of our DSFG surveys will be to identify and characterize these galaxies (measuring luminosity functions, redshift distributions, correlation functions,

Accreting supermassive black holes (SMBHs) play an important role in the evolution of galaxies. However, it is still unclear how SMBHs accrete

The origin of the compact radio/mm emission observed in the vast majority of Active Galactic Nuclei (AGN) is still largely debated. Over

Extremely rapid episodes of accretion are expected to be fundamental in a large variety of persistent and transient phenomena, and are needed