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Opticon JRA5: Smart Focal Planes

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Title: Opticon JRA5: Smart Focal Planes


1
  • Opticon JRA5 Smart Focal Planes
  • Colin Cunningham
  • 5th September 2007
  • UK ATC (UK), Univ Durham (UK), LAM (FR), CRAL
    (FR), IAC (SP), IoA Cambridge (UK), TNO/TPD (NL),
    ESO-INS (Int), ASTRON (NL), CSEM (SW),
    INAF-Padova (IT), UNIBrem (GE), Reflex s r o (CZ)
    , AAO (UK/Aus)

2
Objectives
  • Evaluate, develop and prototype of technologies
    for Smart Focal Planes
  • Build up and strengthen a network of expertise in
    Europe, and encourage mobility between partners
  • Engage European Industry in the development of
    technologies which can be batch produced to
    enable future complex instruments to be built
    economically
  • Enable these technologies to be developed to the
    stage where they can be considered for the next
    generation of telescopes

3
Science Motivation Multi IFU Spectroscopy
  • Prominent Science Cases
  • 1. First light the highest-redshift galaxies
  • 2. Physics of high-redshift galaxies
  • Secondary Science Cases
  • 1. Resolved Stellar populations
  • 2. Initial Mass Function in stellar clusters

4
Multi-Slit Spectroscopy
  • Multi-slit spectroscopy in the NIR provides an
    alternative, which may be better fitted to some
    science cases
  • MOSFIRE on Keck gt TMT instrument
  • Image courtesy Ian McLean (UCLA)

5
Methodology
  • Start with Instrument concepts to define
    technology requirements SmartMOS SmartMOMSI
  • Develop and prototype technology
  • Feed lessons back into iterations of instrument
    concepts
  • Feed this into ELT instrument Design Studies and
    Phase A studies
  • Very successful gt EAGLE SMOS consortia

6
(No Transcript)
7
WP1 Management, systems design and systems
engineering
  • Ensure the JRA meets its goals, within financial
    and time constraints. Enable clear communications
    between teams and to the OPTICON management team.
    Facilitate an open process for deciding which
    technologies to progress. Yes
  • Develop and revise the existing Technology
    Roadmap Use the roadmap to aid decisions making
    on which technologies to prototype. Identify new
    technologies. Yes
  • Fix requirements and specification to provide
    realistic and measurable goals for technology
    studies. Develop and evaluate concepts for future
    instruments using Smart Focal Planes. Yes
  • Evaluate technology requirements and challenges
    which are common to many of the Smart Focal Plane
    devices, such as metrology, cryogenic mechanism
    reliability including tribology, position sensing
    and actuation. Yes

8
Objectives WP2 Technology Development
  • Develop areas of technology which offer key
    performance enhancements for multi-object and
    integral field spectroscopy, and are feasible for
    prototyping in the near-term Yes
  • Develop manufacturing techniques to enable batch
    production. Partial

9
WP2.1 Image slicers
  • Develop smooth image slicer optics for the
    visible, develop transmissive devices, replacing
    linear arrays of mirrors by customised arrays of
    small lenses. Industrialisation of these
    manufacturing processes. Yes used for VLT-MUSE
  • Investigate solutions for the measurement of
    small aperture, complex optical surface. Yes
  • Develop the currently available analysis and
    simulation tools for IFU design. No being done
    for VLT-KMOS
  • Explore optical replication techniques for slicer
    production Yes

10
WP2.2 Beam Manipulators
  • Cryogenic pick-off arms Investigate higher
    angular resolution and alternatives for
    positioning. Investigate methods for improving
    thermal performance. Compare optical designs for
    increasing the field of view. Explore cost
    effective technologies and design options for
    batch production. Develop prototype devices. No
    part of development programme for KMOS
  • Beam Steering Mirrors. Investigate technology
    required for miniaturisation of beam steering
    devices. Explore cost effective technologies and
    design options for batch production . Prototype
    key elements. Yes
  • Robotic manipulators (Starbugs) Develop
    concepts for robotic mirror positioners and
    optical layouts to act as spectrometer feeds.
    Develop prototype devices. Yes and devised and
    developed Starpicker

11
WP3.1 Fibre Systems
  • Study new ways to manufacture high quality
    fibre-based IFUs for the wavelength range 0.35 -
    2.5 microns. No not a priority from Instrument
    concept studies
  • Consider how fibre IFUs can be miniaturised for
    multi-object applications. No as above
  • Identify suitable fibre core material for
    cryogenic operation. No as above
  • Explore concepts for efficiently deploying fibre
    IFUs. Concepts of vacuum-held and robotically
    deployed fibre systems considered

12
WP3.2 Reconfigurable Slits and Masks
  • Investigate concepts and predicted performance of
    Cryo mechanisms for actuators and linear slides.
    Yes
  • Evaluate current availability of data for
    relevant materials properties at cryogenic
    temperatures, and identify where future work is
    needed. Some work done
  • Evaluate challenges for sensing and metrology,
    including slit configuration measuring systems.
    Yes
  • Investigate friction-stiction and particle
    production and contamination issues for slit
    mechanisms. Yes

13
WP3.3 MOEMS
  • Review and visit European micro-technology
    labs/industries to evaluate capabilities and
    stimulate interest in developing programmable
    slit devices using existing technologies
    Investigate exploitation of other research
    programmes, e.g. JWST NIRSpec ESA studies and
    devices from different application sectors Yes
  • Model NIRSpec multi slit device and evaluate
    impact in the design and operation of a future
    spectrograph. Yes
  • Develop existing laboratory test systems for
    MOEMS operating in a cryogenic environment and in
    the infrared regime if possible. Yes

14
WP4 Trade off Study
  • Evaluate the technologies against the science and
    functional requirements. Carry out risk analysis
    and cost estimates. Choose technologies to
    prototype. Yes as part of instrument concept
    studies
  • Identify requirements for future developments of
    other technologies. Yes eg cooled DMs
  • Review technology options to agree most
    productive technologies to progress in Phase B.
    Yes - gt development of Starpicker

15
WP5 Management and Systems Engineering (Phase B)
  • Continuation of Phase A, with specific emphasis
    on roadmapping. Partial
  • Continuation of evaluation of risks and
    challenges in the provision of enabling
    technologies, including identifying routes for
    further development Yes
  • Culminating in a report which details the way
    forward to multiobject and multiple field
    spectroscopy with Extremely Large Telescopes and
    current facilities. Need overtaken by ELT DS
    instrument studies and ELT Instrument working
    group report

16
Phase B
  • WP6 Prototype Technologies Design Build and
    test prototype devices and subsystems. In
    progress
  • WP7 Verify Technology Design, build, and test
    laboratory test equipment, and evaluate the new
    technology prototype devices in test equipment.
    Demonstrate manufacturability of chosen
    technology. In progress
  • WP8 Feasibility studies Continue studies of
    feasibility of technologies with medium to
    long-term availability and potential high
    performance Yes MOEMS devices

17
Technology Highlights
18
Slit mechanism
  • Slit mechanism developed for ESA by CSEM
  • Developed further under SFP programme
  • Improved manufacture techniques for slides

19
Swiss Technology in Keck MOSFIRE instrument
  • UCLA building Keck NIR MOS instrument with CSEM
    slit mechanism
  • first time they have gone to European procurement

Courtesy Ian McLean, UCLA
20
Multi-object Multi-IFU Spectrometers WFSPEC
MOMSI in FP6 ELT design study
S-MOMSI
KMOS
MOMSI
WFSPEC
EAGLE
21
EAGLE Concept
22
Pick-off Mirror Technology
UK ATC/CSEM/Astron
AAO
23
Star-picker
  • Positions Pick-Off Mirrors to better than 5
    micron repeatability
  • 100 repositions per hour will be improved
  • Joint development UK ATC, Astron CSEM

International Patent Application No
PCT/GB2006/002426 (P14214PC)
24
Cryogenic Testings of Star-Picker Elements
Nitrogen bath cold tests conducted on gripper
vertical travel successful, but apparent need to
up gripper current by 20. This to be confirmed
with additional tests.
Rotation stage cold wrap manufactured and
installed, ready for precision measurements in
cold bath and cryostat.
25
Beam Steering Mirror
  • Mirror and support manufactured
  • Mirror being polished
  • Use of a dummy mirror to
  • Test the mount
  • Develop control software
  • Evaluate performances
  • Design and manufacture of Tip/Tilt platform

26
Actuators performances
Opposite
  • Stroke
  • Influence of the flexural pivot

Mirror
Piezo
Angle
  • Perfect linearity of the deformation
  • Fit with FEM

27
Image Slicers
  • Invented by Ira Bowen in 1938, but only now
    coming into use as optical fabrication techniques
    make it possible
  • Now possible to replicate using electroforming
  • For visible light Sub 10nm rms surfaces needed
    still only possible with glass slicers
  • Economic study shows cross-over at about 30
    slicers

28
SMART Focal Planes Programmable slits in Europe
Principle of the micro-mirror array
  • Long slit mode
  • Surface quality

lt 15nm PtV
Tilt accuracy lt 1 arcmin
100 x 200µm
29
ELT Instrument Proposal SMOS
30
Changes to scope of work
  • Removed Pick off arms done by KMOS project
  • Reduced scope of image slicer work
  • Reduced fibre development
  • Added Star-picker development
  • Phase B concentrated on object selection for
    EAGLE and MOEMS for SMOS concepts

31
Planned work to completion
  • WP 3.2 Cryomechanisms Tip-Tilt Focal Plane
    ASTRON
  • WP 5.0 Management and Systems Engineering UK
    ATC / IAC
  • WP 6.2 Pick-off Prototype Gripper Cold Tests
    CSEM/UK ATC
  • WP 6.2 Pick-off Prototype Star-Picker Cold
    Tests UK ATC
  • WP 6.3 Beam manipulator prototype - active optics
    LAM
  • WP 6.4 MOEMS mirror array prototype LAM/CSEM
  • WP6.5 Integration of Star-Picker and Cryo-Mirrors
    in Smart Focal Plane Demonstrator

32
New WP
  • Evaluation of cooled and cryogenic mirrors for
    SFP based NIR MIR instruments with AO built-in
  • Driven by EAGLE and MIDIR requirements
  • Coordinated by TNO-TPD, Delft
  • Partners Astron, Leiden, UK ATC ( Paisley Univ)
  • Kick-off meeting on Friday 6th Sept

33
Dissemination of results publications
  • Proc. SPIE 5382 (2004)
  • Smart focal plane technologies for ELT
    instruments
  • Colin R. Cunningham, Suzanne K. Ramsay-Howat,
    Francisco Garzon, Ian R. Parry, Eric Prieto,
    David J. Robertson, and Frederic Zamkotsian
  • Proc. SPIE 5904 (2005)
  • Progress on smart focal plane technologies for
    extremely large telescopes
  • Colin Cunningham, Eli Atad, Jeremy Bailey, Fabio
    Bortoletto, Francisco Garzon, Peter Hastings,
    Roger Haynes, Callum Norrie, Ian Parry, Eric
    Prieto, Suzanne R.Howat, Juergen Schmoll, Lorenzo
    Zago, and Frederic Zamkotsian
  • Proc. SPIE 6273 (2006)
  • A scalable pick-off technology for multi-object
    instruments
  • Peter Hastings Suzanne Ramsay Howat Peter
    Spanoudakis Raymond van den Brink Callum
    Norrie David Clarke K. Laidlaw S. McLay Johan
    Pragt Hermine Schnetler L. Zago
  • SMART-MOS a NIR imager-MOS for the ELT
  • Francisco Garzón Eli Atad-Ettedgui Peter
    Hammersley David Henry Callum Norrie Pablo
    Redondo Frederic Zamkotsian
  • New beam steering mirror concept and metrology
    system for multi-IFU
  • Fabrice Madec Eric Prieto Pierre-Eric Blanc
    Emmanuel Hugot Sébastien Vivès Marc Ferrari
    Jean-Gabriel Cuby
  • Deployable payloads with Starbug
  • Andrew McGrath Roger Haynes
  • It's alive! Performance and control of prototype
    Starbug actuators
  • Roger Haynes Andrew McGrath Jurek Brzeski
    David Correll Gabriella Frost Peter Gillingham
    Stan Miziarski Rolf Muller Scott Smedley
  • Micro-mirror array for multi-object spectroscopy

34
SPIE Orlando Trade Show
35
What did work!
  • Using ELT instrument concepts to drive technology
    requirements
  • Joint development programmes
  • Replicated Image Slicers
  • Durham, LAM, Reflex, Padua
  • Starpicker
  • UK ATC, ASTRON, CSEM
  • MOEMS mirror device
  • LAM, CSEM, with subcontract to IMT Neuchatel
  • European team-building leading to EAGLE and SMOS
    instrument consortia

36
What didnt work lessons learned
  • Phasing and 18 month planning cycle
  • Some partners didnt work together well
  • Too many partners
  • Work packages with only one partner were less
    successful than the very productive joint
    workpackages
  • Financial and time-sheet tracking
  • Communications.

37
OPTICON SFP achievements
  • 2 ELT Instruments in baseline planning based on
    our Smart Focal Plane Technologies
  • Teams working on proposals for E-ELT Phase A
    studies
  • Working prototypes
  • Starpicker
  • Starbugs
  • Deformable Beam Steering Mirrors
  • MOEMS mirrors
  • Replicated image slicers
  • Reports on enabling technologies actuators,
    positions sensing, slit mechanisms
  • Technology development path foreseen in Opticon
    FP7 and with national funding for future ELT and
    8-10 m instruments

38
Overall Objectives Met?
  • Evaluate, develop and prototype of technologies
    for Smart Focal Planes - YES
  • Build up and strengthen a network of expertise in
    Europe, and encourage mobility between partners
    YES
  • Engage European Industry in the development of
    technologies which can be batch produced to
    enable future complex instruments to be built
    economically Partial image slicers
  • Enable these technologies to be developed to the
    stage where they can be considered for the next
    generation of telescopes - YES

39
Smart Instrument Technologies Proposal for FP7
Summary
  • Smart Focal Plane Technology developments are now
    being carried forward into ELT instrument Phase A
    programme for EAGLE and possible S-MOS
  • Proposal for FP7 addresses 2 further questions
  • How to build lower mass, active instruments to
    meet flexure requirements of wide-field or high
    resolution cryogenic instruments?
  • Are there science and operational gains from
    expanding the Smart Focal Plane concept into a
    Smart Instrument Suite where several different
    instruments a fed from a wide field pick off
    system, and if so what technologies need
    development?
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