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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_BW.jpg)
Celine Peroux
European Southern Observatory - Germany
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Martin Zwaan
European Southern Observatory - Germany
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Varsha Kulkarni
University of South Carolina - USA
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Simon Weng
European Southern Observatory/Sydney University - Australia
![](Arjun.png)
Arjun Karki
University of South Carolina - USA
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Ramona Augustin
Space Telescope Institute - USA
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Roland Szakacs
European Southern Observatory - Germany
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Anne Klitsch
DARK/University of Copenhagen - Denmark
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Aleksandra Hamanowicz
Space Telescope Institute - USA
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Alejandra Fresco
Max Planck Institute for Extraterrestrial Physics - Germany
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Andrew Biggs
European Southern Observatory - Germany
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Andrew Fox
Space Telescope Institute - USA
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Matthew Hayes
Stockholm University - Sweden
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Chris J. Howk
University of Notre Dame - USA
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Rob Ivison
European Southern Observatory - Germany
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Glenn Kacprzak
Swinburne University of Technology/ASTRO 3D - Australia
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Susan Kassin
Space Telescope Institute - USA
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Harald Kuntschner
European Southern Observatory - Germany
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Dylan Nelson
University of Heidelberg - Germany
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Max Pettini
University of Cambridge - UK