UK Role in the European Extremely Large Telescope -CANARY Phase B
Lead Research Organisation:
Durham University
Department Name: Physics
Abstract
See original proposal 'UK Role in the European Extremely Large Telescope' H68780X, ST/G00109X/1, 1 April 2008; 'Response to RMR', 16 May 2008 and 'Response to PPRP Questions for the Visiting Panel ', V1.2, 4 August 2008.
Publications
Barr D
(2015)
Reducing adaptive optics latency using Xeon Phi many-core processors
in Monthly Notices of the Royal Astronomical Society
Basden A
(2015)
Investigation of POWER8 processors for astronomical adaptive optics real-time control
in Monthly Notices of the Royal Astronomical Society
Basden A
(2015)
Analysis of electron multiplying charge coupled device and scientific CMOS readout noise models for Shack-Hartmann wavefront sensor accuracy
in Journal of Astronomical Telescopes, Instruments, and Systems
Basden A
(2010)
Durham adaptive optics real-time controller.
in Applied optics
Basden A
(2015)
Sensitivity improvements for Shack-Hartmann wavefront sensors using total variation minimization
in Monthly Notices of the Royal Astronomical Society
Basden A
(2015)
Monte Carlo modelling of multiconjugate adaptive optics performance on the European Extremely Large Telescope
in Monthly Notices of the Royal Astronomical Society
Basden A
(2012)
The Durham adaptive optics real-time controller: capability and Extremely Large Telescope suitability DARC: capability and ELT suitability
in Monthly Notices of the Royal Astronomical Society
Basden A
(2015)
Simulation and laboratory demonstration of measurement and mitigation of dome seeing
in Journal of Physics: Conference Series
Description | The funding secured the UK leadership of the CANARY UK-France project, with Durham as overall PI. CANARY has achieved the following world firsts, which are fully consistent with the goals of this funding: Laser Multi-Object AO (MOAO) demonstrated on-sky - this is a technology required for the MOS (Multi-Object Spectrograph) on the forthcoming European Extremely Large Telescope. The technology will allow, for example, a survey of the first galaxies to form in the universe, exploring the mechanisms which give the universe its particular form. It overcomes the effects of atmospheric turbulence on ground-based telescopes and does so over a very wide field of view. Artificial stars, produced by powerful lasers, are used to sense the atmospheric turbulence above the telescope and and to correct its effects. Laser Tomographic AO (LTAO) demonstrated on-sky - this is an atmospheric correction technology required by the UK-led HARMONI first-light instrument on the forthcoming European Extremely Large Telescope. Full Linear Quadratic Gaussian Conreol demonstrated on-sky - optimally removes the effects of windshake on telescope images. AO feed of a photonic lantern spectrograph demonstrated on-sky optimal feeding of a new photonic technology spectrograph using adaptive optics Artificial Neural Net tomographic reconstructor demonstrated on-sky, - technology allowing adaptive optics turbulence correction to adapt automatically to changes in the atmospheric configuration CuReD and HWR wavefront reconstructors demonstrated on-sky - new high-speed computational methods for adaptive optics for exoplanet imaging. MOAO and LTAO are required for the ELT-MOS, ELT-IFU (HARMONI), METIS, and possibly HIRES. This work has secured our position in the MOS and HIRES projects, including the position of AO Systems Engineer and Real-time control lead for the MOS. The success of CANARY has secured EU funding (OPTICON) and ESO support for CANARY Phase D (Na LGS Spot Elongation) We note that MOAO technology is used in Keck's future NGAO system and LTAO is a workhorse mode of GMT. |
Exploitation Route | We note that MOAO technology is used in Keck's future NGAO system and LTAO is a workhorse mode of GMT. |
Sectors | Pharmaceuticals and Medical Biotechnology |
URL | https://www.dur.ac.uk/cfai/projects/canary/ |
Description | Yes, the funding secured the UK leadership of the CANARY UK-France project, with Durham as overall PI. CANARY has achieved the following world firsts, which are fully consistent with the goals of this funding: Laser Multi-Object AO (MOAO) demonstrated on-sky Laser Tomographic AO (LTAO) demonstrated on-sky Full Linear Quadratic Gaussian Conreol demonstrated on-sky AO feed of a photonic lantern spectrograph demonstrated on-sky Artificial Neural Net tomographic reconstructor demonstrated on-sky, CuReD and HWR wavefront reconstructors demonstrated on-sky MOAO and LTAO are required for the ELT-MOS, ELT-IFU (HARMONI), METIS, and possibly HIRES. This work has secured our position in the MOS and HIRES projects, including the position of AO Systems Engineer and Real-time control lead for the MOS. The success of CANARY has secured EU funding (OPTICON) and ESO support for CANARY Phase D (Na LGS Spot Elongation) I note that MOAO technology is used in Keck's future NGAO system and LTAO is a workhorse mode of GMT. |
First Year Of Impact | 2010 |
Description | EU FP7 OPTICON (2) WP1 |
Amount | £202,000 (GBP) |
Funding ID | 312430 |
Organisation | European Commission |
Department | Seventh Framework Programme (FP7) |
Sector | Public |
Country | European Union (EU) |
Start | 01/2013 |
End | 12/2016 |
Description | European Space Agency TRP |
Amount | £283,554 (GBP) |
Funding ID | TEC-MMO/2014/127 |
Organisation | ESA - ESTEC |
Sector | Public |
Country | Netherlands |
Start | 03/2015 |
End | 05/2018 |
Title | SCIDAR at the ING |
Description | A high-vertical resolution optical turbulence profiler was developed and installed on the 2.5m Isaac Newton Telescope. Observations made in support of the CANARY instrument were used to create a database of turbulence profiles that are of sufficient vertical resolution to design and characterise instruments for the future set of extremely large telescopes. |
Type Of Material | Database/Collection of data |
Year Produced | 2015 |
Provided To Others? | Yes |
Impact | The Thirty Metre Telescope project used the database of atmospheric profiles measured using the SCIDAR instrument to select La Palma as the backup operating site for the major US astronomical facilty. |
Description | CANARY |
Organisation | Heriot-Watt University |
Department | School of Engineering & Physical Sciences |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Overall leadership of the CANARY project. Approximately equal contribution with Obs de Paris to the design, build and test. Real-time controller. |
Collaborator Contribution | Design of Diffractive optical elements for Laser Guide Star constellation projection |
Impact | Proof that Natural Guide Star Multi-Object Adaptive Optics works on-sky |
Start Year | 2007 |
Description | CANARY |
Organisation | Observatory of Paris |
Department | Laboratory for Space Science and Astrophysical Instrumentation |
Country | France |
Sector | Charity/Non Profit |
PI Contribution | Overall leadership of the CANARY project. Approximately equal contribution with Obs de Paris to the design, build and test. Real-time controller. |
Collaborator Contribution | Design of Diffractive optical elements for Laser Guide Star constellation projection |
Impact | Proof that Natural Guide Star Multi-Object Adaptive Optics works on-sky |
Start Year | 2007 |
Description | CANARY |
Organisation | Pontifical Catholic University of Chile |
Department | Department of Industry and System Engineering |
Country | Chile |
Sector | Academic/University |
PI Contribution | Overall leadership of the CANARY project. Approximately equal contribution with Obs de Paris to the design, build and test. Real-time controller. |
Collaborator Contribution | Design of Diffractive optical elements for Laser Guide Star constellation projection |
Impact | Proof that Natural Guide Star Multi-Object Adaptive Optics works on-sky |
Start Year | 2007 |
Description | CANARY |
Organisation | UK Astronomy Technology Centre (ATC) |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Overall leadership of the CANARY project. Approximately equal contribution with Obs de Paris to the design, build and test. Real-time controller. |
Collaborator Contribution | Design of Diffractive optical elements for Laser Guide Star constellation projection |
Impact | Proof that Natural Guide Star Multi-Object Adaptive Optics works on-sky |
Start Year | 2007 |
Description | CANARY |
Organisation | University of Oviedo |
Department | Gijón Polytechnic School of Engineering |
Country | Spain |
Sector | Academic/University |
PI Contribution | Overall leadership of the CANARY project. Approximately equal contribution with Obs de Paris to the design, build and test. Real-time controller. |
Collaborator Contribution | Design of Diffractive optical elements for Laser Guide Star constellation projection |
Impact | Proof that Natural Guide Star Multi-Object Adaptive Optics works on-sky |
Start Year | 2007 |
Description | E-ELT MOS |
Organisation | Observatory of Paris |
Country | France |
Sector | Academic/University |
PI Contribution | Adaptive Optics for the E-ELT MOS |
Collaborator Contribution | Full co-partners in the study with key roles divided |
Impact | Phase A Design study for EAGLE Adaptive Optics |
Start Year | 2010 |