Time-domain
Leaders
Richard I. Anderson
Institute of Physics, Ecole Polytechnique Federale de Lausanne, Observatoire de Sauverny, Switzerland
Cyrielle Opitom
Institute for Astronomy, University of Edinburgh, United Kingdom
Paula Sanchez Saez
European Southern Observatory Garching, Germany
Sub-working groups & co-leaders
Alerts group coordinator
Alejandra Melo
BHs group co-leads
Giustina Vetri · Darshan Kakkad
Dormant BHs science case lead
Michał Pawlak
GW EM science case lead
Susanna Vergani · Sofia Bisero
Pulsating stars science case lead
Valentina D’Orazi · Cenk Kayhan
Selection functions and FoM coordinator
Avraham Binnenfeld
Star Formation and evolution science case lead
Fatemeh Zahra Majidi · Amelia Bayo
White Dwarfs science case lead
Anna Pala
WST 2MTDT organizers
Fatemeh Zahra Majidi · Giulia De Somma
Related pages
The dynamic Universe
Black holes growth across time and mass
Star and planet formation
Stars, their end points, feedback, and elements production
Multi-messenger Astrophysics
Main section
Science team
The Science Team plays a key role in proposing and developing transformative science cases and in shaping the science-driven requirements for the WST.