Work Package Descriptions

The conceptual architecture [Phase A] has been converted to separate work packages and each of these will be studied. The interaction between the work packages will be controlled by the systems engineering team.

 

  • Simulations (SIM)

The goal of this workpackage is to conduct end-to-end science simulations to assist science trade-offs on the TLRs and provide the tools necessary to  design the MOSAIC Reference Surveys.

  • Data Reduction Software (DRS)

The DRS will look at the requirements for the calibration and seek to inform the other sub- system designers of the impact on the observations of some of the trade-off decisions. This will be done by modelling of the system.

  • Systems Engineering

The systems engineering team will manage the interaction between the sub-systems and between the science and technical teams. The overall light path and calibration system designs will be included in this work package.

  • Instrument Core Sub-System (ICOS)

Design of the overall structure implementation. Manages the telescope mechanical interfaces and ensures that the flexure and field tracking are within the requirements identified from the other work-packages. In implementations which require a carousel, this will be part of this work package.

Cable routing between the other sub-systems will be managed here.

  • Science Optical Signal Correction (SOSC)

SOSC will be in charge of defining the Adaptive Optics configuration that will allow meeting the specifications. This includes System activities (simulations and trade offs), components and modules definition and, finally, implementation at the Telescope Focal Plate.

This WP is linked with the POS since it defines the set of components that will have to be installed on the Focal Plate with the needed accuracy. It also gets a link with SOST WP since it delivers the corrected beams with the appropriate format.

This WP is not responsible for HMM & IGM definition except through the definition of a GLAO mode using M4 only.

  • Positioning Sub-System (POS)

POS will define the way all pick offs (whatever the mode: HMM, HDM,IGM) will be installed on the focal plate with the needed accuracy. It will be highly related to the overall architecture of the instrument.

The configuration time is a highly dependent on this package.Science Optical Signal Transport (SOST)

This WP is responsible for transporting the corrected Science light from the focal plate to the spectrograph. It will include Fibre links (HMM & IGM) and, may be, Fibres or another solution (slicers) for HDM. This is one of the Trade Offs that will be performed in the Phase A study.

  • Spectrograph Sub-System (SPES)

The spectrograph work package will consider possible implementations that cover all of the modes. The best use of detector real estate as well as the fibre feed focal ratio and diameter are key parameters to be considered in this work package. The output will have a significant impact on the overall instrument layout.

  • Electronics and Instrument Control System(EICS)

The instrument mechanisms and cryogenics will be controlled using ESO standard hardware and software. This workpackage is expected to be low risk but a study of the control system will be made to assess the likely space, power and layout implications.

Steering Committee

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

Board

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

Management

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

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

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

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