International audienceEAGLE is the multi-object spatially-resolved near-IR spectrograph instrument concept for the E-ELT, relying on a distributed Adaptive Optics, so-called Multi Object Adaptive Optics. This paper presents the results of a phase A study. Using 84×84 actuator deformable mirrors, the performed analysis demonstrates that 6 laser guide stars (on an outer ring of 7.2' diameter) and up to 5 natural guide stars of magnitude R 2 resolution element at H band whatever the target direction in the centred 5' science field for median seeing conditions. In terms of sky coverage, the probability to find the 5 natural guide stars is close to 90% at galactic latitudes |b| ~ 60 deg. Several MOAO demonstration activities are also on-going
The near-Infrared Multi-Object Spectrograph (IRMOS) for TMT is one of the most powerful astronomical...
The near-Infrared Multi-Object Spectrograph (IRMOS) for TMT is one of the most powerful astronomical...
At first light, the overall AO system architecture for the Thirty Meter Telescope will consist ...
International audienceEAGLE is the multi-object spatially-resolved near-IR spectrograph instrument c...
International audienceEAGLE is the multi-object spatially-resolved near-IR spectrograph instrument c...
spectrographs deployable (via pick-off mir-rors) over a patrol field of 38.5 arcminutes2. Each IFU h...
International audienceContext. A new challenging adaptive optics (AO) system, called multi-object ad...
International audienceEAGLE (Extremely large Adaptive telescope for GaLaxy Evolution) is one of the ...
The next generation of ground-based optical/infrared (IR) telescopes will have primary mirrors of up...
EAGLE is an instrument under consideration for the European Extremely Large Telescope (E-ELT). EAGLE...
International audienceHARMONI is a visible and near-infrared integral field spectrograph equipped wi...
Adaptive Optics (AO) can greatly enhance the resolution of astronomical images, achieving close to d...
To study properties of cold dark matter (CDM), which can only be observed through its gravitational ...
The near-Infrared Multi-Object Spectrograph (IRMOS) for TMT is one of the most powerful astronomical...
The near-Infrared Multi-Object Spectrograph (IRMOS) for TMT is one of the most powerful astronomical...
At first light, the overall AO system architecture for the Thirty Meter Telescope will consist ...
International audienceEAGLE is the multi-object spatially-resolved near-IR spectrograph instrument c...
International audienceEAGLE is the multi-object spatially-resolved near-IR spectrograph instrument c...
spectrographs deployable (via pick-off mir-rors) over a patrol field of 38.5 arcminutes2. Each IFU h...
International audienceContext. A new challenging adaptive optics (AO) system, called multi-object ad...
International audienceEAGLE (Extremely large Adaptive telescope for GaLaxy Evolution) is one of the ...
The next generation of ground-based optical/infrared (IR) telescopes will have primary mirrors of up...
EAGLE is an instrument under consideration for the European Extremely Large Telescope (E-ELT). EAGLE...
International audienceHARMONI is a visible and near-infrared integral field spectrograph equipped wi...
Adaptive Optics (AO) can greatly enhance the resolution of astronomical images, achieving close to d...
To study properties of cold dark matter (CDM), which can only be observed through its gravitational ...
The near-Infrared Multi-Object Spectrograph (IRMOS) for TMT is one of the most powerful astronomical...
The near-Infrared Multi-Object Spectrograph (IRMOS) for TMT is one of the most powerful astronomical...
At first light, the overall AO system architecture for the Thirty Meter Telescope will consist ...