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The MOSAIC project brings together the design and analysis work done on all previous conceptual designs for a MOS for the ELT. As we saw in previous section, the MOSAIC Consortium includes world-leaders in the design, development, and construction of astronomical instrumentation, located across Europe and Brazil, and supported as high priority by their funding agencies. Partners within the MOSAIC consortium have a long and successful heritage of instrument delivery for ESO, including: FLAMES, KMOS, MUSE, SPHERE, NACO, VIMOS, and X-SHOOTER. This makes available the skills needed to develop MOSAIC whatever the area: Adaptive Optics, Fibres, Spectrograph, Interfaces with the telescope, etc. The MOSAIC instrument concept is now under development and will provide a versatile, facility-class instrument, capable of addressing a broad range of key science topics enabled by the size and adaptive optics of the ELT. Following Figure 3-1 illustrates the skills of the consortium especially with respect to Spectrographs and Adaptive Optics:

 

 

Steering Committee

Alexis Finogenov
Alexis Finogenov
Helsinki Univ., Finland
José Alfonso
José Alfonso
IA, Lisbon Univ., Portugal
Goran Ostlin
Goran Ostlin
Stockholm Univ., Sweden
Fabrizio Fiore
Fabrizio Fiore
INAF-Osservatorio Astronomico di Roma, Italy
Simon Morris
Simon Morris
Durham Univ., U.K
Martin Roth
Martin Roth
AIP, Potsdam, Germany
Olivier Le Fèvre
Olivier Le Fèvre
LAM, Marseille, France
Daniel Schaerer
Daniel Schaerer
University of Geneva, Switzerland
Lex Kaper
Lex Kaper
Amsterdam Univ.,
Netherlands
Jesus Gallego
Jesus Gallego
Madrid, Computense Univ., Spain
Beatriz Barbuy
Beatriz Barbuy
IAG, Sao Paulo, Brazil
Bodo Ziegler
Bodo Ziegler
Vienna Univ., Austria

Board

Simon Morris
Simon Morris
Co-P.I.
François Hammer
François Hammer
Principal Investigator
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Beatriz Barbuy
Beatriz Barbuy
Co-P.I.
Jean-Gabriel Cuby
Jean-Gabriel Cuby
Co-P.I.
Lex Kaper
Lex Kaper
Co-P.I.

Management

Pascal Jagourel
Pascal Jagourel
Project Manager
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Mickaël Frotin
Mickaël Frotin
Deputy Project Manager
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Fatima Defrondat
Fatima Defrondat
Quality Assurance Engineer
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Science

Rubén Janssen
Rubén Janssen
UK ATC Instrument Scientist
Chris Evans
Chris Evans
Project Scientist
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Gavin Dalton
Gavin Dalton
Instrument Scientist
Mathieu Puech
Mathieu Puech
Co-Project Scientist
Simulations (Science)
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Engineering

Andreas Kelz
Andreas Kelz
Light Transport
to Spectrograph (SOST)
Phil Parr Burman
Phil Parr Burman
NIR Spectrograph
(SPES-NIR)
(ICOS)
Fanny Chemla
Fanny Chemla
System Engineer
Optics
Sylvestre Taburet
Sylvestre Taburet
IT/Web Infrastructure
Kacem El Hadi
Kacem El Hadi
AIT
Johan Pragt
Johan Pragt
VIS Spectrograph
(VIS-SPES)
Ian Lewis
Ian Lewis
Positioning System (POS)
Marc Dubbeldam
Marc Dubbeldam
System Engineer
Mechanics
David Le Mignant
David Le Mignant
LAM, Marseille
Isabelle Guinouard
Isabelle Guinouard
Light Transport
to Spectrographs (SOST)
Marie Larrieu
Marie Larrieu
Electronics & ICS (EICS)
Yanbin Yang
Yanbin Yang
DRS
Tim Morris
Tim Morris
System Engineer,
Adaptative Optics
Ramon Navarro
Ramon Navarro
VIS Spectrograph
(SPES-VIS)
Bruno Castilho
Bruno Castilho
Light Transport
to Spectrograph (SOST)
Annemieke Janssen
Annemieke Janssen
VIS-SPES
(VIS Spectrograph)
Kevin Middleton
Kevin Middleton
Positioning system (POS)
Gérard Rousset
Gérard Rousset
Adaptative Optics Expertise

Who are we? Infos on the MOSAIC consortium.

CONSORTIUM

Scientific goals and milestones: why MOSAIC?

SCIENCE

How do we get there? All the technology behind MOSAIC.

INSTRUMENT

What performance can we expect from MOSAIC?

PERFORMANCE

How will MOSAIC fit in the instrumental landscape?

Synergy