With two large deformable mirrors with a total of more than 7000 actuators that need to be driven from the measurements of six 60x60 LGS WFSs (total 1.23Mpixels) at 800Hz with a latency of less than one frame, NFIRAOS presents an interesting real-time computing challenge. This paper reports on a recent trade study to evaluate which current technology could meet this challenge, with the plan to select a baseline architecture by the beginning of NFIRAOS construction in 2014. We have evaluated a number of architectures, ranging from very specialized layouts with custom boards to more generic architectures made from commercial off-the-shelf units (CPUs with or without accelerator boards). For each architecture, we have found the most suitable a...
NFIRAOS is the first-light adaptive optics system planned for the Thirty Meter Telescope, and is bei...
NFIRAOS, the TMT Observatory's initial facility AO system is a multi-conjugate AO system feeding sci...
A proposed solution to the increased computational demands of Extremely Large Telescope (ELT) scale ...
With two large deformable mirrors with a total of more than 7000 actuators that need to be driven fr...
The Real-Time Controller (RTC) for the Thirty Meter Telescope (TMT) Narrow Field Infrared Adaptive O...
Prototyping and benchmarking was performed for the Real-Time Controller (RTC) of the Narrow Field In...
The Thirty Meter Telescope (TMT) will implement a first light facility Laser Guide Star Multi Conjug...
The adaptive optics (AO) simulations at the Thirty Meter Telescope (TMT) have been carried out using...
The Narrow Field Infrared Adaptive Optics System (NFIRAOS) is the first light Adaptive Optics (AO) s...
As a part of the trade study for the Narrow Field Infrared Adaptive Optics System, the adaptive opti...
NFIRAOS, the Thirty Meter Telescope’s first adaptive optics system is an order 60x60 Multi-Conjugate...
This paper reflects, from a computational perspective, on the experience gathered in designing and i...
The high control frequency required of planned E-ELT adaptive optics modules (from several hundreds ...
We propose a many-core CPU architecture for Extremely Large Telescope (ELT) scale adaptive optics (A...
Adaptive optics (AO) systems currently under investigation will require at least two orders of magit...
NFIRAOS is the first-light adaptive optics system planned for the Thirty Meter Telescope, and is bei...
NFIRAOS, the TMT Observatory's initial facility AO system is a multi-conjugate AO system feeding sci...
A proposed solution to the increased computational demands of Extremely Large Telescope (ELT) scale ...
With two large deformable mirrors with a total of more than 7000 actuators that need to be driven fr...
The Real-Time Controller (RTC) for the Thirty Meter Telescope (TMT) Narrow Field Infrared Adaptive O...
Prototyping and benchmarking was performed for the Real-Time Controller (RTC) of the Narrow Field In...
The Thirty Meter Telescope (TMT) will implement a first light facility Laser Guide Star Multi Conjug...
The adaptive optics (AO) simulations at the Thirty Meter Telescope (TMT) have been carried out using...
The Narrow Field Infrared Adaptive Optics System (NFIRAOS) is the first light Adaptive Optics (AO) s...
As a part of the trade study for the Narrow Field Infrared Adaptive Optics System, the adaptive opti...
NFIRAOS, the Thirty Meter Telescope’s first adaptive optics system is an order 60x60 Multi-Conjugate...
This paper reflects, from a computational perspective, on the experience gathered in designing and i...
The high control frequency required of planned E-ELT adaptive optics modules (from several hundreds ...
We propose a many-core CPU architecture for Extremely Large Telescope (ELT) scale adaptive optics (A...
Adaptive optics (AO) systems currently under investigation will require at least two orders of magit...
NFIRAOS is the first-light adaptive optics system planned for the Thirty Meter Telescope, and is bei...
NFIRAOS, the TMT Observatory's initial facility AO system is a multi-conjugate AO system feeding sci...
A proposed solution to the increased computational demands of Extremely Large Telescope (ELT) scale ...