The Science Team plays a key role in proposing and developing transformative science cases and in shaping the science-driven requirements for the WST.

The WST project is committed to an open-science policy, allowing any professional astronomer to join the Science Team .

Currently, more than 800 members from 41 countries across five continents have joined the team. The Science Team has led the publication of a first version of the WST Science White Paper, which already shows the transformative scientific impact that the WST will have on a very broad range of scientific topics.

The Science Team is fully engaged in further developing the science drivers for the WST to be published soon.

The Science Team is led by the project scientist, Vincenzo Mainieri, and is organised into five working groups:

Vincenzo Mainieri

PROJECT SCIENTIST

European Southern Observatory Garching, Germany

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

Vanessa Hill

Observatoire de la Cote d’Azur, Universitè Cote d’Azur, CNRS, Laboratoire Lagrange, France

Rodolfo Smiljanic

Nicolaus Copernicus Astronomical Center, Poland

Eline Tolstoy

University of Groningen, The Netherlands

Sebastian Kamann

John Moores University Liverpool, United Kingdom

Anna McLeod

Durham University, United Kingdom

Martin M. Roth

Leibniz-Institut für Astrophysik Potsdam, Germany

Francesco Belfiore

European Southern Observatory Garching, Germany

Richard Ellis

University College London, United Kingdom

Mark Sargent

École Polytechnique Fédérale de Lausanne, Switzerland

Sofia Contarini

Max Planck Institute für Extraterrestriche Physik, Germany

Jean-Paul Kneib

École Polytechnique Fédérale de Lausanne, Switzerland

Michele Moresco

University of Bologna, Italy

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the WST needs to be placed in an adequate site

Excellent seeing, clear nights, and low light pollution. Selecting such a site is part of a comprehensive process that involves the investigation and simulation of multiple aspects.

Acronyms

TECHNICAL

WST: Wide-field Spectroscopic Telescope

FoV: Field-of-View

IFS: Integral Field Spectrograph

IFU: Integral Field Unit

MOS: Multi-Object Spectrograph

MOS-HR: High-resolution Multi-Object Spectrograph

MOS-LR: Low-resolution Multi-Object Spectrograph

ToO: Targets of Opportunity

INSTITUTES & UNIVERSITIES

AIP: Leibniz Institute for Astrophysics Potsdam

ANU/Astralis: The Australian National University / Astralis

CRAL/CNRS: Centre de Recherche Astrophysique de Lyon / French National Centre for Scientific Research

EPFL: Swiss Federal Institute of Technology in Lausanne

ESO: European Southern Observatory

IA/CAUP: Institute of Astrophysics and Space Sciences / Centre for Astrophysics of the University of Porto

IASF-MI/INAF: Institute for Space Astrophysics and Cosmic Physics of Milan / National Institute for Astrophysics

IP2I/CNRS: Institute of Physics of the Two Infinities of Lyon / French National Centre for Scientific Research

IRFU/CEA: Institute for Research into the Fundamental Laws of the Universe / French Alternative Energies and Atomic Energy Commission

Lagrange/CNRS: Lagrange Laboratory / French National Centre for Scientific Research

LAM/CNRS: Marseille Astrophysics Laboratory / French National Centre for Scientific Research

MAQC/Astralis: Macquarie University / Astralis

NCAC: Nicolaus Copernicus Astronomical Center

OAArcetri/INAF: Arcetri Astrophysical Observatory / National Institute for Astrophysics

OABrera/INAF:Brera Astronomical Observatory / National Institute for Astrophysics

OACapodimonte/INAF: Capodimonte Astronomical Observatory / National Institute for Astrophysics

OASBologna/INAF:Bologna Observatory of Astrophysics and Space Science / National Institute for Astrophysics

UKRI: UK Research and Innovation

UNIBO: University of Bologna

UNIGRO/NOVA: University of Groningen / The Netherlands Research School for Astronomy

UNISYD: The University of Sydney

UNIVIE: University of Vienna

UWA: The University of Western Australia

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Join the community

ue-logo-h
This project has received funding from the European Union Horizon Europe Research and Innovation Action under grant agreement no. 101183153 -WST.
Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or European Research Executive Agency (REA). Neither the European Union nor the granting authority can be held responsible for them.

Acronyms

TECHNICAL

WST: Wide-field Spectroscopic Telescope

FoV: Field-of-View

IFS: Integral Field Spectrograph

IFU: Integral Field Unit

MOS: Multi-Object Spectrograph

MOS-HR: High-resolution Multi-Object Spectrograph

MOS-LR: Low-resolution Multi-Object Spectrograph

ToO: Targets of Opportunity

INSTITUTES & UNIVERSITIES

AIP: Leibniz Institute for Astrophysics Potsdam

ANU/Astralis: The Australian National University / Astralis

CRAL/CNRS: Centre de Recherche Astrophysique de Lyon / French National Centre for Scientific Research

EPFL: Swiss Federal Institute of Technology in Lausanne

ESO: European Southern Observatory

IA/CAUP: Institute of Astrophysics and Space Sciences / Centre for Astrophysics of the University of Porto

IASF-MI/INAF: Institute for Space Astrophysics and Cosmic Physics of Milan / National Institute for Astrophysics

IP2I/CNRS: Institute of Physics of the Two Infinities of Lyon / French National Centre for Scientific Research

IRFU/CEA: Institute for Research into the Fundamental Laws of the Universe / French Alternative Energies and Atomic Energy Commission

Lagrange/CNRS: Lagrange Laboratory / French National Centre for Scientific Research

LAM/CNRS: Marseille Astrophysics Laboratory / French National Centre for Scientific Research

MAQC/Astralis: Macquarie University / Astralis

NCAC: Nicolaus Copernicus Astronomical Center

OAArcetri/INAF: Arcetri Astrophysical Observatory / National Institute for Astrophysics

OABrera/INAF:Brera Astronomical Observatory / National Institute for Astrophysics

OACapodimonte/INAF: Capodimonte Astronomical Observatory / National Institute for Astrophysics

OASBologna/INAF:Bologna Observatory of Astrophysics and Space Science / National Institute for Astrophysics

UKRI: UK Research and Innovation

UNIBO: University of Bologna

UNIGRO/NOVA: University of Groningen / The Netherlands Research School for Astronomy

UNISYD: The University of Sydney

UNIVIE: University of Vienna

UWA: The University of Western Australia

Edit Template
ue-logo-h
This project has received funding from the European Union Horizon Europe Research and Innovation Action under grant agreement no. 101183153 -WST.
Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or European Research Executive Agency (REA). Neither the European Union nor the granting authority can be held responsible for them.