Projects

Recently, in Lambert et al. (2024, A&A, accepted, arXiv:2402.06870), we carried out the largest area, narrow-band survey of Lyman Alpha Emitter (LAE)

The COSMOS High-z ALMA-MIRI Population Survey (CHAMPS; PI: A. Faisst, co-PI: M. Aravena et al.) is an ALMA large program in Cycle

One of the most interesting findings of recent ALMA [CII]158um galaxy surveys (e.g. ALPINE, REBELS, CRISTAL) has been the clear presence of

In recent years a major effort was dedicated to collecting large data sets of high-quality spectra of stars in the Milky Way

The Vera Rubin Observatory (VRO) will be fully operational for a ten-year survey commencing in 2025. It is expected to detect many

Comets serve as remarkable remnants of the primordial protoplanetary disk, offering invaluable insights into the origins of our Solar System, planetary formation,

We use precision radial-velocity instruments in Chile to uncover the first Jupiter-analogues orbiting metal-rich stars.  The key to our project is the

The importance of chemical characterization for studying the history of the Milky Way (MW) and its accretion events is well established. However,

A consistent picture has emerged on the average flow of baryons in and out of galaxies and its role in regulating galaxy

The many faces and personalities of galaxies are shaped by physical processes that affect their different components – like bulges and discs

Laboratory studies of cosmic dust are urgently needed for the modeling of protoplanetary disk observations. By studying samples of meteorites’ properties at

The objective of this project is to create advanced and realistic models of X-ray radiation within Active Galactic Nuclei (AGN), and apply