1st AO4ELT conference - Adaptive Optics for Extremely Large Telescopes
Paris, France, June 22-26, 2009Y. Clénet, J.-M. Conan, T. Fusco and G. Rousset (Eds.)
ISBN: 978-2-7598-0496-2
Astrophysical needs and high level requirements for AO on ELTs
Open Access
Overall science goals and top level AO requirements for the E-ELT 01001
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Science and Adaptive Optics Requirements of MICADO, the E-ELT adaptive optics imaging camera 01002
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EAGLE Spectroscopy of Resolved Stellar Populations Beyond the Local Group 01004
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Scientific Impact of the Operating Temperature for NFIRAOS on TMT 01006
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AO systems and instrumental concepts
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Adaptive Optics Systems for the Thirty Mirror Telescope 02001
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ATLAS: the Laser Tomographic Adaptive Optics module for the E-ELT 02002
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How to break the FoV versus thickness rule in MCAO 02003
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NFIRAOS - first light adaptive optics system for TMT 02004
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Requirements for AO-ELT operation and ELT site monitor 02005
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Extreme Adaptive Optics in the mid-IR: The METIS AO system 02006
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Towards the phase A review of MAORY, the multi-conjugate adaptive optics module for the E-ELT 02007
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EAGLE multi-object AO concept study for the E-ELT 02008
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Status of the LESIA High Contrast Bench development in the framework of the E-ELT 02011
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MCAO for the E-ELT: preliminary design overview of the MAORY module 02013
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AO simulations
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Turbulence and wind sp eed profiles for simulating the TMT AO p erformances 03001
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Comparison of Reconstruction and Control algorithms on the ESO end-to-end simulator OCTOPUS 03002
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Full Physical Optics Sky Coverage Simulation for MCAO Systems on ELT’s 03003
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Closed-loop ground layer adaptive optics simulations with elongated spots : impact of modeling noise correlations 03004
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Simulations of Laser Guide Star Adaptive Optics Systems for the European Extremely Large Telescope 03005
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The Software Package PAOLAC: an embedment of the analytical code PAOLA within the CAOS problem-solving environment 03006
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Fast continuous model of Shack-Hartmann wavefront sensors for atmospheric tomography on ELTs 03009
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Very low flux adaptive optics using spatial and temporal priors 03010
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SCAO Simulation Results with a Pyramid Sensor on an ELT-like Telescope 03011
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Laser guide stars
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High-resolution lidar experiment for the Thirty Meter Telescope 04001
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ELP-OA: status report of the setup of the demonstrator of the Polychromatic Laser Guide Star at Observatoire de Haute-Provence 04002
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End-to-end model for the Polychromatic Laser Guide Star project (ELP-OA) 04006
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Design of an holographic off-axis calibration light source for ARGOS at the LBT 04007
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Active Laser Guide Star refocusing system for EAGLE instrument 04008
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Wave front sensing
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Ultra high precision wavefront sensing for Extreme-AO on ELTs 05001
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Evaluation of the T/T Conditions at Gemini South using NICI AO Telemetry Data 05002
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Study of centroiding algorithms to optimize Shack-Hartmann WFS in the context of ELTs 05004
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Lessons learned with the Active Phasing Experiment: comparison of four optical phasing sensors on a segmented Very Large Telescope 05005
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Sensing Quasi-Static Aberrations of Adaptive Optics Systems On-Line with Long-Exposure Phase Diversity 05006
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The Self-Coherent Camera : a focal plane sensor for EPICS ? 05008
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Correction of quasi-static wavefront errors for ELT with two sequential DMs 05009
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Shack-Hartmann tomographic wavefront reconstruction using LGS: analysis of spot elongation and fratricide effect 05010
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The CAFADIS camera: a new tomographic wavefront sensor for Adaptive Optics 05011
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The TMT/NFIRAOS LGS wavefront sensing demonstration bench 05012
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Concept Study of On-Instrument Wavefront Sensors (OIWFS) for the TMT IRIS Science Instrument 05013
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Detectors for LGS WF sensing on an ELT: characteristics, special features, limitations, technology 05014
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Anisoplanatism effects in Shack-Hartmann Wave Front Sensing with Laser Guide Stars on the ELTs 05015
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Characterization and mitigation of Laser–Guide–Star–induced aberrations 05016
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Pyramid wave-front sensing with a laser guide star for an ELT 05017
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Focal-plane wavefront sensing for segmented telescope 05018
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A Direct Measurement of Atmospheric Dispersion in N-band Spectra: Implications for Mid-IR Systems on ELTs 05019
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A prototype of the Laser Guide Stars wavefront sensor for the E-ELT multi-conjugate adaptive optics module 05020
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Modeling the Chromatic Correction Error in Adaptive Optics: Application to the Case of Mid-Infrared Observations in Dry to Wet Atmospheric Conditions 05021
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Deformable mirrors
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Voice-coil technology for the E-ELT M4 Adaptive Unit 06002
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MEMS deformable mirrors in astronomical adaptive optics 06003
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Recent Progress on Correcting Components (useful for ELTs) at CILAS 06004
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Electromagnetic DM technology meets future AO demands 06005
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Adaptive Optics for ELTs with Low-Cost and Lightweight Segmented Deformable Mirrors 06006
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A 1-metre Ni coated CFRP demonstrator for large deformable mirrors 06007
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Deformable mirror fitting error by correcting the segmented wavefronts 06008
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Characterisation of the influence function non-additivities for a 1024-actuator MEMS deformable mirror 06009
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Real-time control
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Tomography reconstruction using the Learn and Apply algorithm 07001
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Atmospheric tomography with separate minimum variance laser and natural guide star mode control 07002
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Adapting optimal LQG methods to ELT-sized AO systems 07003
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Sparse prediction of turbulence in time and space 07004
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Fourier transform-wavefront reconstruction for the pyramid wavefront sensor 07005
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An FPGA Based Computing Platform for Adaptive Optics Control 07006
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FPGA-based real time processing of the Plenoptic Wavefront Sensor 07007
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Toward an optimal control for wide field of view AO on ELT 07008
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An optimized calibration strategy for high order adaptive optics systems : the Slope-Oriented Hadamard Actuation 07009
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Implementation of a waveform recovery algorithm on FPGAs using a zonal method (Hudgin) 07010
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Pathfinders
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A Sample of GeMS Calibrations and Control Schemes 08001
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Solar Multi-Conjugate Adaptive Optics at the Dunn Solar Telescope 08002
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CANARY: The NGS/LGS MOAO demonstrator for EAGLE 08003
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Experimental results of tomographic reconstruction on ONERA laboratory MCAO bench 08004
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Laboratory Experiments of Laser Tomographic Adaptive Optics at Visible Wavelengths on a 10-meter Telescope 08005
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Segment phasing experiments on the High Order Test bench 08006
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Post processing
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Determination of astrometry and photometry of faint companions in the presence of residual speckle noise 09001
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Suppressing stellar residual light on extremely large telescopes by aperture modulation 09002
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Use of AO PSF models for the Study of Resolved Stellar Populations 09003
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Reconstruction of the point spread function for the ground layer adaptive optics system ARGOS 09004
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Optimal Method for Exoplanet Detection by Spectral and Angular Differential Imaging 09005
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Statistics of undevelop ed speckles in partially polarized light 09006
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Acknowledgements 00002
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