The MUSE-ALMA Haloes Survey
The MUSE-ALMA Haloes project aims at quantifying the physical properties of the gaseous haloes of galaxies with a particular focus on the multi-phase nature of the baryons in the circumgalactic medium. The survey gathers a large observational sample of absorption and emission data probing the atomic, molecular and ionised gas as well as stellar populations in a sample of galaxies. A key component of the MUSE-ALMA Haloes survey is therefore the multi-facility observational campaign conducted with VLT/MUSE, ALMA and HST.
Team
Celine Peroux
European Southern Observatory - Germany
Martin Zwaan
European Southern Observatory - Germany
Varsha Kulkarni
University of South Carolina - USA
Simon Weng
European Southern Observatory/Sydney University - Australia
Arjun Karki
University of South Carolina - USA
Ramona Augustin
Space Telescope Institute - USA
Roland Szakacs
European Southern Observatory - Germany
Anne Klitsch
DARK/University of Copenhagen - Denmark
Aleksandra Hamanowicz
Space Telescope Institute - USA
Alejandra Fresco
Max Planck Institute for Extraterrestrial Physics - Germany
Andrew Biggs
European Southern Observatory - Germany
Andrew Fox
Space Telescope Institute - USA
Matthew Hayes
Stockholm University - Sweden
Chris J. Howk
University of Notre Dame - USA
Rob Ivison
European Southern Observatory - Germany
Glenn Kacprzak
Swinburne University of Technology/ASTRO 3D - Australia
Susan Kassin
Space Telescope Institute - USA
Harald Kuntschner
European Southern Observatory - Germany
Dylan Nelson
University of Heidelberg - Germany
Max Pettini
University of Cambridge - UK