Introducing the 2020 ESO Fellows - Chile

Published: 22 Jul 2020
NAOMI at first light

The Offices for Science and the Astronomy Faculty are very pleased to present the 2020 ESO Fellows. Here is an introduction to the Fellows due to start in Chile later this year.

alcalde

Belén Alcalde (ALMA)

Research Interests: Massive high redshift galaxies in the context of galaxy formation and evolution, analysis and interpretation of large datasets and images through machine learning tools and astronomical instrumentation.

Current Institute: Universidad Complutense de Madrid, Spain

cikota

Aleksandar Cikota (Paranal)

Research Interests: Progenitor systems of Type Ia Supernovae and supernova cosmology; using observations obtained with VLT/FORS2 in (spectro)polarimetry mode to investigate supernova ejecta asymmetries and dust along the sight lines to transients of all kinds.

Current Institute: Lawrence Berkeley National Laboratory, USA

Escorza

Ana Escorza (Paranal)

Research Interests: Stellar and binary evolution, the late stages of the evolution of low- and intermediate-mass stars, binary interactions and their products, barium stars and other polluted binaries and high-resolution optical spectroscopy.

Current Institutes: Institutes of Astronomy of KU Leuven and ULB, Belgium

Harrington

Kevin Corneilus Harrington (ALMA)

Research interests: The build-up of stellar mass across cosmic time; galaxy evolution; radio-IR observations and modeling of the (star-forming) interstellar medium

Current Institute: Argelander-Institut fuer Astronomie, University of Bonn, Germany
 

Masih

Michael Abdul-Masih (Paranal)

Research Interests: Massive star evolution, close binaries, non-spherically symmetric massive stars (rapidly rotating stars, semi-detached and contact binary systems), internal mixing processes, gravitational wave progenitors, and optical and UV spectroscopy

Current Institute: KU Leuven, Belgium

Wevers

Thomas Wevers (Paranal)

Research interests: The scale invariance of accretion processes from X-ray binaries to supermassive black holes; in particular, using tidal disruption events as probes to study this scale invariance, as well as accretion flow properties in SMBHs; data driven studies (detection and follow-up) of TDEs using space-based (e.g. XMM-Newton, Swift in UV and X-rays) and ground-based (e.g. time-resolved spectroscopy in the optical/NIR) telescopes; host galaxy studies of TDEs.

Current institute: Institute of Astronomy, University of Cambridge, UK