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The WST consortium brings together the Horizon Consortium, comprising 23 research institutes, and a much broader Science Team. Although formally distinct, the two groups work seamlessly to advance the concept study, with the Science Team being in charge of defining transformative science cases and shaping the science-driven requirements for the WST.

All consortium members adhere to the WST Code of Conduct and Publication Policy.

The Horizon Consortium brings together all the expertise required to perform the concept study of a facility as ambitious as the WST. This includes all the different aspects involved in such a process, from defining the science goals and requirements, to designing the telescope and the instruments, to planning its operations and data management, to ensuring the sustainability of the project. 

The Science Team is at the heart of the WST scientific vision, uniting an international community of astronomers to define transformative science cases and guide the science-driven development of the telescope.

The Horizon Consortium’s work is broken down into six work packages that cover all the key areas needed for the concept study. Each work package is further split into smaller, task-oriented sub-packages, each led by one or two dedicated coordinators.

Steering CommittEe

The committee provides strategic direction, guides decision-making, tackles challenges, allocates resources, and monitors project progress

Project office

Roland Bacon

COORDINATOR

Roland Bacon (CRAL) has 10 years of managerial experience as director of CRAL, as well as 35 years of unique experience in the design, realisation, and use of integral-field spectrographs.

He has been the PI of the very successful MUSE instrument at the VLT.

Sofia Randich

DEPUTY COORDINATOR

Sofia Randich, former director of INAF-OAA, brings to the project her significant experience in the management of Galactic spectroscopic surveys (e.g., the Gaia-ESO large public spectroscopic survey) and in high-resolution multi-object spectroscopy (MOS).

Vincenzo Mainieri

PROJECT SCIENTIST

Vincenzo Mainieri (ESO) is project scientist for the upcoming multi-object spectrographs at ESO (4MOST, MOSAIC, MOONS till Oct 2018).

He brings to the project his long and successful experience in leading extragalactic MOS and IFS science teams.

Roelof de Jong

FACILITY SCIENTIST

Roelof de Jong (AIP), is PI of 4MOST, leading a large international team of engineers, software developers, and scientists.

He is also head of the Milky Way and Local Volume section at the AIP.

Philippe Dierickx

TELESCOPE WP COORDINATOR

Philippe Dierickx has a long experience as a system engineer and project manager at ESO.

He is an expert in the design and production of large and very large telescopes.

David Lee

INSTRUMENT WP COORDINATOR

David Lee (UKRI-STFC-UKATC) has extensive experience in developing instrumentation and technology for ground and space-based telescopes (MIR/JWST, MOONS/VLT, ANDES/ELT).

Paolo Franzetti

OPERATIONS SCIENTIST

Paolo Franzetti (IASF-Mi) has a long experience in data reduction and analysis software for MOS instruments (e.g., VIMOS, EUCLID, MOONS) and in spectroscopic surveys management (e.g., VIPERS, VANDELS).

Olga Bellido

SYSTEM COORDINATOR

Olga Bellido (AIP), lead system engineer of 4MOST and subsystem system engineer of the ELT/ANDES instrument, bringing 20 years of system engineering experience for ground- and space-based instrumentation.

JOIN US

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

The WST community comprises approximately a thousand researchers, engineers, students, and staff from different academic and cultural backgrounds and across multiple continents. The WST Consortium strives to provide a welcoming and safe environment that promotes engagement, collaboration, and growth for all, grounded in equity, diversity, and inclusion.

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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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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

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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.