Objectives of the Joint Research Activity 1

The primary goal of this Joint Research Activity (JRA) is to develop the concepts, designs and technologies required for the next generation of Adaptive Optics (AO) capabilities which will equip large telescopes over the next decade. Three possible AO systems will be investigated in parallel, Natural Guide Star (NGS) Extreme AO (XAO); Multi-Conjugate Adaptive Optics (MCAO) with multiple Fields of View; and multi Laser Guide Star (LGS) systems.

The participants will perform feasibility studies, develop prototypes and support R&D for the enabling technologies. R&D will be pursued for high accuracy and high dynamic range wavefront sensing, high computing power real time computer (RTC) hardware and software, MCAO control theory, large deformable mirrors, high-density piezo stack deformable mirrors, high-density large stroke micro-mirrors and associated control electronics.

The Chair of the Adaptive Optics Joint Research Activity is N Hubin (ESO): nhubin @ eso.org

Next JRA 1 General Meeting March 30 & 31st 2006
at La Palma

Management of JRA1

This Joint Research Activity is  coordinated by the European Southern Observatory and involves 8 institutes in Europe:
The organisation chart of the JRA is described here
The official start of OPTICON and therefore of JRA1 was January 1st 2004.
The deliverables associated to each Workpackages of the JRA1 are listed here and corresponding milestones listed here

Relevant Management documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Detailed predicted cost breakdown and commitments for the JRA 1
April 2004
.xls
Y
Detailed schedule for the JRA  1
April 2004
.mpp
Y
Template for Manpower time report for 2004 (NEW!)
Nov 2004
.xls
N
Template for Hardware expenditure report for 2004 (NEW!)
Nov 2004
.xls
N
Kick-off meeting Agenda
Action list
March 2004
March 2004
.doc
.doc
N
N
OPTICON contractual description of Work
March 2004
.pdf
Y
JRA1 presentation at OPTICON KO meeting in Ghent (April 1st and 2nd 2004)
April 2004
.ppt
N
Kick-off meeting: Objectives of the JRA1 (presentation from ESO)
March 2004
.ppt
Y
Kick-off: Project Control (ESO)
March 2004
.ppt
Y
General meeting 1 Agenda
Action list
Sept. 2004
.doc
.doc
N
N
General Meeting: 1 JRA1 Management (ESO)
Sept. 2004
.ppt
.ppt
N
N
Executive progress report 1 to OPTICON board
Sept. 2004
.doc
N
Template for Manpower time report for 2005 (NEW!)
Jan.2005
.xls
N
Template for Hardware expenditure report for 2005 (NEW!)
Jan.2005
.xls
N
Status of JRA1 expenditures and projections as per period 1 report
Jan.2005
.xls
Y
Draft report of JRA1 for period 1
Jan.2005
.doc
Y
VLT Planet FInder Feasibility and conceptual design studies:
  • LAOG et al. 
  • MPIA et al.

Dec. 2004
Dec. 2004

.zip
.zip

Y
Y
OPTICON report for year 1 (2004)
April 2005
.doc
Y
General Meeting: 2 JRA1 Management (ESO)
July 2005
.ppt
Y
General Meeting 2: Action list
July 2005
.doc
Y
General Meeting 2: Agenda
July 2005
.pdf
Y
Executive progress report 2 to OPTICON board
July 2005
.pdf
Y

Adaptive Optics System Studies

The purpose of this workpackage (WP 2) is to perform system and design studies of the next generation of Adaptive Optics systems for the existing 8-10 m telescopes in Europe. The following systems will be studied:
Relevant documentation is available in the following table
Description of the documents
Date
Type
Prot.
Kick-off Meeting: Simulations of 2nd generation AO system for the VLT (ESO)
March 2004
.ppt N
General Meeting 1: Status of 2nd Gen. AO systems for VLT: Planet Finder, MUSE-AO, HAWK-I AO (ESO)
Sept. 2004
.ppt
.ppt
N
N
General Meeting 2: Status of XAO simulations (ESO)
July 2005
.ppt
Y





Extreme Adaptive Optics System design study

The purpose of this workpackage (WP2.1) is to perform feasibility studies and conceptual design for an Extreme Adaptive Optics system dedicated to searching for extra solar planets. Definition of the high level specification of all key components required for this system and intended to be developed within this JRA (Deformable mirror, wavefront sensor, real time computer control). If the feasibility study is successful, a preliminary design will be pursued.

Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
VLT Planet Finder Phase A study technical specifications and Statement of Work
May 2003
.pdf
N
VLT Planet Finder Milestone 1: ESO-OPTICON inputs
Dec. 2003
.ppt
N
Real Time computer Platform for VLT Planet Finder
Dec. 2003
.ppt
N
Software Standards for VLT Planet Finder
Dec. 2003
.ppt
N
VLT Planet Finder Science case Specifications
Feb. 2004
.pdf
Y
Kick-off Meeting: CHaracterising Exoplanet  by Opto-IR Polarimetry and Spectroscopy (CHEOPS: MPIA)
March 2004
.ppt
N
Kick-off Meeting: VLT Planet Finder feasibility study (INSU-LAOG)
March 2004
.ppt
N
256x256 CCD detector technical specification issue 1 (VLT-SPE-ESO-14690-3320) (ESO-INSU)
July 2004
.pdf
N
256x256 CCD detector Statement of Work issue 1 (VLT-SOW-ESO-14690-3383) (ESO-INSU)
July 2004
.pdf
N
JRA1 General Meeting 1: Status of the Planet Finder Conceptual design study (MPIA, LAOG)
Sept. 2004
.ppt
.ppt
.ppt
N
N
N
Executive summary of the Planet Finder phase A study of MPIA and LAOG
Jan. 2005
.pdf
.pdf
Y
Y
240x240 CCD detector technical specification issue 2 (VLT-SPE-ESO-14690-3320) (ESO-INSU)
240x240 CCD detector Statement of Work issue 3 (VLT-SOW-ESO-14690-3383) (ESO-INSU)
March 2005
March 2005
.doc
.doc
Y
Y
General Meeting 2:
  • A Planet Finder instrument for the ESO VLT (INSU-MPIA)
  • A CCD for Adaptive Optics Applications (JRA2) (ESO)

July 2005

.ppt

.ppt

Y
Y







Laser / Natural Guide Star Multi Conjugate Adaptive Optics design studies

The purpose of this workpackage (WP2.2) is to perform Laser/Natural Guide Star (L/NGS) MCAO designs for the VLT: 
  • Conceptual and preliminary design of a Laser based ground layer Adaptive Optics system for MUSE. This system should be able to provide a large (1') FOV correction at short wavelengths. 
  • Conceptual and preliminary design of a Laser based ground layer Adaptive Optics system for HAWK-I. This system should be able to provide a large (8') FOV correction at Near IR wavelengths
  • Feasibility and conceptual design of a very large FOV multi-WFS AO system: FALCON
Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Second Generation Instrument MCAO Study - FALCON- Statement of Work
Feb.2003
.pdf
N
Kick-off Meeting: L/NGS MCAO Status and Plans(ESO)
March 2004
.ppt
N
Kick-off Meeting: NOVA contribution to MUSE (NOVA-Leiden))
March 2004
.ppt
N
MUSE Adaptive Optics Top Level requirements (ESO-Leiden)
March 2004
.pdf
Y
MUSE Adaptive Optics Technical Specifications (ESO-Leiden)
Feb. 2004
.pdf
Y
MUSE Ground Layer Adaptive Optics System Analysis Report (at Conceptual design Review) (ESO-Leiden)
March 2004
.pdf
Y
MUSE Ground Layer Adaptive Optics Conceptual design report (ESO-Leiden)
March 2004
.pdf
Y
MUSE Ground Layer Adaptive Optics Management Plan (at Conceptual Design Review) (ESO)
March 2004
.pdf
Y
MUSE Ground Layer Adaptive Optics Conceptual design review presentation (ESO)
March 2004
.ppt
N
General Meeting 1: Status of GLAO conceptual design studies (ESO, Leiden)
Sept. 2004
.ppt
.ppt
N
N
HAWK-I AO : Ground Layer Adaptive Optics: Top Level requirements (ESO)
Nov. 2004
.pdf
Y
HAWK-I AO : Ground Layer Adaptive Optics: Conceptual design report (ESO)
Nov. 2004
.pdf
Y
HAWK-I AO : Ground Layer Adaptive Optics: Analysis report (ESO)
Nov. 2004
.pdf
Y
HAWK-I AO : Ground Layer Adaptive Optics: Management plan report (ESO)
Nov. 2004
.pdf
Y
HAWK-I AO Ground Layer Adaptive Optics Conceptual design review presentation (ESO)
Nov. 2004
.ppt
N
FALCON strawman design and analysis (INSU-Paris)
Nov.2004
.pdf
.pdf
.pdf
Y
Y
Y
JRA1 General Meeting 2: GRAAL for HAWK-I and GALACSI for MUSE (ESO)
MUSE- ASSIST & GLAO update (NOVA)
July 2005
.ppt
.ppt
Y
Y















Multi-object WFS prototype for GTC

The purpose of this workpackage (WP2.3) is to design and develop a prototype of a Multi-object wavefront sensor for the Gran Telescopio Canarias (GTC) in view of its MCAO system. The prototype will be a laboratory demonstration.

Relevant documentation is listed in the following table
Description of the documents
Date
Type
Prot.
Kick-off meeting: The GTC Multi-Object WFS prototype presentation at Kick-off
March 2004
.pdf
N
General meeting 1: Status of the GTC multi-object WFS (GTC)
Sept. 2004
.ppt
N
GTC Multi-Object Curvature Wavefront Sensor Report
March 2005
.pdf
Y


Multiple FOV MCAO with Natural Guide Star for LBT

The purpose of this workpackage (WP2.4) is to design and develop a Multiple Fields of view WFS for the Large Binocular Telescope (LBT). The Prototype will be tested on the sky.

Relevant documentation is listed in the following table
Description of the documents
Date
Type
Prot.
Kick-off meeting: LBT Multiple Field of View NGS WFS (MPIA-INAF)
March 2004
.ppt
N
General meeting 1: Status of LBT Multi- FOV NGS WFS (MPIA-INAF) Sept. 2004
.ppt
N
Design and analysis of the LBT multi-object wavefront sensor (INAF-MPIA)
Nov.2004
.doc
.pdf
Y
Y
General Meeting 2: Multiple FoV NGS Wavefront sensor for LBT (INAF-MPIA)
July 2005
.ppt
Y






Enabling Technology for Adaptive Optics

This Workpackage (WP 3) contains all Research & Development  activities required to support the development of AO and MCAO systems described in WP 2. It includes the following items

Real Time Computer Platform

This Workpackage (WP 3.1) will develop the second Generation of Real Time Computer (RTC) platform for XAO and MCAO systems: A new hardware and software real time control architecture will be designed and prototyped. Performance according to WP 2.1 and 2.2 will be demonstrated.

Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Kick-off Meeting: 2nd generation of Real Time Computer  (ESO)
March 2004
.ppt
N
Kick-off Meeting: Use of FPGA forReal Time Control (U. Durham)
March 2004
.ppt
N
Real Time computer Platform for VLT Planet Finder
Dec. 2003
.ppt
N
General Meeting 1: Status of 2nd generation Real TIme Computer Platform (ESO)
Sept. 2004
.ppt
N
General Meeting 1: Use of FPGA forReal Time Control (U. Durham)
Sept. 2004 .ppt
N
General Meeting 2:  Standard Platform for Adaptive Optics Real Time Applications (SPARTA) (ESO)
Use for FPGA for Real Time Control Design (Durham)
July 2005

.ppt
.ppt
Y
Y


















Optimal Control & high performance WFS for Multi-Conjugate Adaptive Optics

This Workpackage (WP 3.2) will develop optimal control methods for MCAO systems: A theoretical study and experimental demonstration of an optimal MCAO control will be performed on the ESO MCAO demonstrator. This WP includes also a theoretical study and experimental validation of high performance WFS dedicated to MCAO.

Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Kick-off Meeting: Optimal control method for MCAO (ONERA)
March 2004
.pdf
N
Kick-off Meeting: High Performance WFS for MCAO (ONERA)
March 2004
.pdf
N
General Meeting 1: Optimal Control Methods and High Performance WFS for MCAO Systems (ESO)
Sept. 2004
.ppt
N
General Meeting 1: Optimal Control Methods & High Performance WFS for  MCAO Systems
Sept. 2004
.ppt
N
Optimal Control Methods and high performance WFS for MCAO systems SOW (ESO-ONERA)
Dec. 2004
.pdf
Y
Sky Coverage in MCAO (ONERA)
Dec. 2004
.pdf
N
General Meeting 2: MAD Status (SCAO & GLAO) (ESO)
July 2005
.ppt
Y
General Meeting 2: Optimal Control method for MCAO (ONERA)
Performance of wavefront measurements for GLAO (ONERA)
July 2005

.ppt
.ppt
Y
Y





 

Piezo Deformable Mirror & drive electronics

This Workpackage (WP 3.3 & WP 3.4) will develop and test a prototype of a Piezo stack Deformable Mirror with more than1200 actuators. A demonstration prototype of a Piezo stack deformable mirror control electronic able to drive the deformable mirror in WP3.3 will be developed and tested. (NB The prototype will not necessarily control the 1200 actuators.)

Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Kick-off Meeting: High order piezo deformable mirror for XAO (ESO)
March 2004
.ppt
N
High Order Deformable Mirror Specifications and Statement of Work Issue 1 (VLT-SPE-ESO-14690-3375)
July 2004
.pdf
Y
General Meeting 1: Status of high-order piezo deformable mirror (ESO)
Sept. 2004
.ppt
N
High Order Deformable Mirror Specifications and Statement of Work Issue 2 (VLT-SPE-ESO-14690-3375)
March 2005
.doc
Y
General Meeting 2: High Order Piezo Deformable Mirror (Specs and Status) (ESO)
July 2005
.ppt
Y





 

VLT Adaptive secondary design Study

This Workpackage (WP 3.4) will perform the feasibility, conceptual, preliminary and final design of the VLT adaptive secondary.  Sub-systems prototypes will be developed as required to overcome issues identified during the design phase.

Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Kick-off Meeting: VLT Adaptive Secondary Study Plans,specs and proposed solutions (Microgate)
March 2004
.ppt
N
Kick-off Meeting: VLT Adaptive Secondary Design Study (INAF-Arcetri) March 2004
.ppt
N
Development of an Adaptive Secondary at the VLT (ESO Presentation at Kick-Off)
March 2004
.ppt
N
Technical Specification for the design study of an Adaptive secondary Mirror for the VLT Issue 1 (VLT-SPE-ESO-11250-3068) (ESO)
May 2004
.pdf
Y
Statement of Work for a design  study of an Adaptive Secondary Mirror for the VLT Issue 1 (VLT-SOW-ESO-11250-3069) (ESO)
May 2004
.pdf
Y
Interface Control Document VLT- Adaptive Secondary (ESO)
May 2004
.pdf
Y
General Meeting 1:
  • VLT Adaptive Secondary Design (ESO)
  • VLT Adaptive Secondary study I/Fs analysis and straw-man design (Microgate & ADS)
  • VLT Adaptive Secondary design study (Straw-man design phase) (INAF)
  • Calibrating an interaction matrix on the sky ( Ecole d’Ingénieurs du Canton de Vaud)



Sept. 2004


.ppt
.ppt
.ppt
.ppt


N
N
N
N
Optical figuring specifications for thin shell to be used in Adaptive Telescope mirror (INAF)
Nov. 2004
.pdf
Y
Adaptive mirror design tool (INAF)
Nov.2004
.xls
Y
General Meeting 2:
  • VLT DSM Unit: Feasibility Study (ADS)
  • VLT DSM Design Study status Electronics (Microgate)
  • Fitting Error Analysis for the VLT DSM
  • VLT Adaptive Secondary Design (Status & complementary studies) (ESO)
  • Interaction Matrix calibration for systems with large deformable mirror(s) (ESO)
  • High SNR interaction matrix measurement  (INAF)


July 2005

.ppt
.ppt
.ppt
.ppt
.ppt
.ppt

Y
Y
Y
Y
Y
Y
VLT Deformable Secondary Mirror Conceptual design study (Microgate/ ADS/ INAF)

July 2005
.zip
Y









 

Large Convex thin shell for large DM

This Workpackage (WP3.6) will design, manufacture and test a large (~1m) convex glass shell for a VLT like large deformable mirror.

Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Kick-off Meeting: Demonstration of a large Convex glass shell (INSU-LAM)
March 2004
.pdf
N
General Meeting 1:Demonstration of a Large Convex Glass shell (INSU-LAM)
Sept. 2004
.pps
N
Specification of the Thin Shell for the VLT Adaptive Secondary (draft) (INAF)
Nov. 2004
.pdf
Y
General Meeting 2:
  • DSM Thin Shell procurement (ESO)
  • Demonstration of a large Convex Glass Shell (INSU)

July 2005
July 2005

.ppt
.ppt

Y
Y
Statement of  Work for the Manufacturing of a 1.1 m Glass Thin Shell (VLT-SOW-ESO-11255-3621) (ESO)
June 2005
.pdf
Y
 

Micro-Deformable Mirrors (MDM)

This Workpackage (WP 3.7) will perform a full design and develop prototypes of a 2k actuator and low order MDM. Corresponding control electronics will be designed and prototyped. Testing of these prototypes will be done on a best effort basis depending on remaining funds.

Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Kick-off Meeting: 2K actuator deformable mirror (INSU-LAOG)
March 2004
.ppt
N
Kick-off Meeting: MOEMS deformable mirrors characterisation and plans (INSU-LAM)
March 2004
.pdf
N
General Meeting 1: 2K micro deformable mirror (INSU-LAOG)
Sept. 2004
.ppt
N
Test report of the Magnetic 60 actuator MDM (INSU-LAOG)
Nov.2004
.doc
.jpg
.jpg
Y
Y
Y
Request for Information on 2k actuator Micro Deformable Mirror (INSU)
Nov. 2004
.doc
Y
2k Actuator MDM specifications (draft) (INSU)
Nov.2004
.doc
Y
General Meeting 2:
  • Micro-Deformable mirror (INSU)
  • Characterisation bench developments for MOEMS based DM (INSU)

July 2005

.ppt
.ppt

Y
Y

 

High Order wavefront sensor experiment

This Workpackage (WP3.8) will design and develop a high order wavefront sensor experimental laboratory bench. This bench will include a Pyramid and Shack Hartmann wave front sensors and will be used to evaluate their relative performance in open and closed loop for XAO systems.

Relevant documentation is listed in the following table

Description of the documents
Date
Type
Prot.
Kick-off Meeting: High Order WFS test bench (ESO)
March 2004
.ppt
N
Kick-off Meeting: High Order WFS experimental Study (INAF)
March 2004
.ppt
N
Kick-off Meeting: Design Possibilities for a very High order Shack Hartmann WFS (U. Durham)
March 2004
.ppt
N
General Meeting 1:
  • High Order Test bench: Goals, TLR and Status (ESO)
  • HOWFS: progress in Arcetri  (INAF)
  • Design for a high-order Shack Hartmann WFS: HOT (Durham)


Sept.2004


.ppt
.ppt
.ppt


N
N
N
High Order  Test bench (HOT): Top Level Requirements (ESO-INAF-Durham)
Sept.2004
.pdf
N
General Meeting 2:
  • High Order Test bench (HOT) (ESO)
  • Pyramid WFS for JRA1 Wp 3.8 (INAF)
  • Status of the SH WFS for HOT (Durham)

July 2005

.ppt
.ppt
.ppt

Y
Y
Y





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