| Monday 26th June | ||
| Invited talks | ||
| chair: Benoit Neichel | ||
| 9:00 | Adaptive Optics Program at TMT | Corinne Boyer |
| 9:30 | GMT AO system design and status | Antonin Bouchez |
| ELT science with AO | ||
| 10:00 | A Review of Visible Light AO Systems and Science on ELTs | Laird Close |
| 10:20 | Science Development for IRIS (Infrared Imaging Spectrograph) on TMT | Shelley Wright |
| 10:40 | Testing Theories of Gravity at the Galactic Center with ELTs | Tuan Do |
| 11:00 | Coffee break | |
| chair: Mitchell Troy | ||
| 11:30 | AO4ELT meets the Solar System: The coming interplay between adaptive optics on ELT, space telescopes, and spacecraft missions | Albert R. Conrad |
| AO pathfinders and new concepts | ||
| 11:50 | AOF – first on-sky performance of the GALACSI GLAO mode (or how to close 10 loops in less than 5 minutes) | Johann Kolb |
| 12:10 | A Visible MCAO system for VLT-UT4 telescope | S. Esposito |
| 12:30 | Commissioning Natural-Guide-Star MCAO with LINC-NIRVANA on LBT | Tom Herbst |
| 12:50 | Keck Planet Imager and Characterizer (KPIC) | Dimitri Mawet |
| 13:10 | Getting ready for GeMS 2.0: A workhorse AO facility | Gaetano Sivo |
| 13:30 | Lunch | |
| AO reconstruction and control | ||
| chair: Jean-Pierre Veran | ||
| 14:50 | Point source sensitivity, Pupil alignment, calibration and control for TMT-NFIRAOS-IRIS | Glen Herriot |
| 15:10 | Non-common Path Aberrations measurement using the NWIWM method | Luis Fernando Rodríguez Ramos |
| 15:30 | Understanding the Vibration Environment for LBT/AO | Pedro Escarate |
| 15:50 | Disturbance Feedforward Control for Vibration Suppression in Adaptive Optics of Large Telescopes | Martin Glück |
| 16:10 | Coffee break | |
| Post-processing of AO data | ||
| chair: Jose Marino | ||
| 16:30 | Point spread function reconstruction for tomographic adaptive optics systems | O. Beltramo-Martin |
| 16:50 | PSF reconstruction and deconvolution for extremely large telescopes | Roland Wagner |
| 17:10 | Scientific impact of PSF knowledge in AO assisted Integral Field Spectroscopy | Niranjan Thatte |
| 17:30 | Data processing on simulated data for SHARK-NIR | Elena Carolo |
| 18:00 | Poster session 1 |
Poster session 1
Current designs of ELT AO systems
| GMTIFS: The Giant Magellan Telescope integral fields spectrograph and imager [P1001] | Brady Espeland |
| Design and expected performance of the GMT's GLAO and phasing sensors [P1002] | Brian McLeod |
| High contrast imaging performance of E-ELT/METIS [P1003] | Brunella Carlomagno |
| Status of the SCAO design of METIS and end-to-end simulation performances [P1004] | Cantalloube Faustine |
| Design study and first performance simulation of the E-ELT/MICADO focal plane coronagraphs [P1005] | Elsa Huby |
| NFIRAOS [P1006] | Glen Herriot, |
| Towards a Stray Light Analysis of the E-ELT [P1007] | Holzlöhner, R. |
| The Infrared Imaging Spectrograph (IRIS) for TMT: Instrument Overview [P1008] | James Larkin |
| Preparation of AITV phase for EELT MOSAIC [P1009] | K. El Hadi |
| Thirty Meter Telescope Adaptive Optics System Error Budgets and Requirements Traceability [P1010] | Kayla Hardie |
| TMT Laser Guide Star Facility Design Update [P1011] | M. Trubey |
| Exploring MAORY performances through tolerance analysis [P1012] | Mauro Patti |
| E-ELT Pre-Focal Station NGS Sensor Arm [P1013] | Paolo La Penna |
| Instrument requirements for precision relative astrometry using TMT/IRIS [P1014] | Ryuji Suzuki |
| A Laser Guide Star WFS design for HARMONI [P1015] | Benoit Neichel |
| Laser guide star optimized wavefront sensor system for the Thirty Meter Telescope [P1016] | Sean Adkins |
AO pathfinders and new concepts
| ERIS, first generation becoming second generation, or re-vitalising an AO instrument [P1017] | Angela Cortes |
| Alignment and preliminary outcomes of an ELT-size instrument to a very large telescope: LINC-NIRVANA at LBT [P1018] | Bergomi Maria |
| Demonstration of hybrid stellar/laser AO wavefront sensing techniques to extend the brightness limit of high-contrast exoplanet AO systems [P1019] | Christoph Baranec |
| A virtual coronagraphic test bench for SHARK-NIR, the second-generation high contrast imager for the Large Binocular Telescope [P1020] | Daniele Vassallo |
| Improved Adaptive Optics Operations at the Large Binocular Telescope Observatory [P1021] | Gregory E. Taylor |
| P-REx: the AO fed Piston Reconstruction Experiment [P1022] | J.-U. Pott |
| SHARK-NIR, the coronagraphic camera for LBT, moving toward construction [P1023] | Jacopo Farinato |
| High Contrast Spectroscopy Testbed for Segmented Telescopes [P1024] | Jacques-Robert Delorme |
| From MagAO-X to GMagAO-X: How the GMT could characterize Proxima b at 4-mirror first light [P1025] | Jared R. Males |
| iLocater: Adaptic optics fed precision spectroscopy for exoplanet science [P1026] | Jonathan Crass |
| AO Systems, Instrumentation, and Capabilities at the LBT - Leading the way for the ELTs [P1027] | Julian Christou |
| SCExAO: lessons learned for a future TMT instrument [P1028] | Julien Lozi |
| Aperture Partitioning for Bispectrum Speckle Imaging [P1029] | Lauren H. Schatz |
| AO development of the DAG 4 m telescope [P1030] | Laurent Jolissaint |
| GTC Adaptive Optics integration progress and Laser Guide Star analysis [P1031] | M. Reyes García-Talavera |
| Complementary Technologies to Adaptive Optics - a System View [P1032] | Matthew Maniscalco |
| EXTREME HIGH CONTRAST IMAGING OF EXOPLANETS WITH OFF-AXIS TELESCOPES: TECHNOLOGY INCUBATION FOR THE NEXT DECADE [P1033] | Maud Langlois |
| Hoverboards: smart focal plane positioners for adaptive optics [P1034] | Michael Goodwin |
| Keck Segment Surface Artifacts: Impacts on Segment Phasing and Image Quality [P1035] | Mitchell Troy |
| NIRPS: an AO-assisted fibre-fed spectrograph. The effect of Adaptive Optics on the fiber modal noise and how to kill it [P1036] | N. Blind |
| Pioneering high contrast science instruments for planet characterization on ELTs [P1037] | Nemanja Jovanovic |
| Enhanced Speckle Nulling Using Single-Mode Fiber Injection and Super-Nyquist Techniques [P1038] | Nikita Klimovich |
| Performance assessment of Adaptive Optics techniques on FSO communications through the atmosphere [P1039] | Noelia Martínez Rey |
| GALACSI on the mountain – first on-sky stand-alone results [P1040] | Paolo La Penna |
| Status and performance of the THD bench in multi-deformable mirror configuration [P1041] | Pierre Baudoz |
| Closed-loop atmospheric dispersion compensation: on-sky demonstration of sub-milliarcsecond residual dispersion across H band [P1042] | Prashant Pathak |
| Hierarchichal-segmented AO in order to attain wide field compensation in the visible on an 8m class telescope [P1043] | Ragazzoni R. |
| A new EU Horizon 2020 OPTICON network to study novel AO (and AO-related) methods and technologies for the E-ELT [P1044] | Richard Myers |
| Commissioning LINC-NIRVANA on LBT [P1045] | Rosalie C. McGurk |
| A solution to the MCAO partial illumination issue [P1046] | Rosalie McGurk |
| GIRMOS - an Gemini MOAO spectrograph and pathfinder for TMT [P1047] | S. Chapman |
| The LSST Real-Time Active Optics System [P1048] | Sandrine Thomas |
| A testing facility for AO on-sky demonstrations at the Copernico’s Telescope within the ADONI framework [P1049] | Simonetta Chinellato |
| The integration of the operational AO software into the LBTO [P1050] | Xianyu Zhang |
| ULTIMATE-Subaru: Wide-field Near-infrared Surveyor with GLAO at Subaru telescope [P1051] | Yosuke Minowa |
Modelling and numerical simulations
| The GreenFlash Real-time Simulator [P1052] | Andrew P Reeves |
| Status of the MAORY numerical simulation tool [P1053] | Carmelo Arcidiacono |
| End-to-end simulations of a near-infrared pyramid sensor on Keck II [P1054] | Cedric Plantet |
| Simulating the Performance of Pyramid Wavefront Sensors on Extended Objects and Broadband Sensing [P1055] | Etsuko Mieda |
| MICADO SCAO numerical simulations [P1056] | Fabrice Vidal |
| ROKET: erROr breaKdown Estimation Tool for adaptive optics systems [P1057] | Florian Ferreira |
| Comparison of layer compression methods and joint optimization [P1058] | Andreas Obereder |
| Analyzing the Operational Behavior of NFIRAOS LGS MCAO Acquisition on the Thirty Meter Telescope using SysML [P1059] | Gelys Trancho |
| Simulations of a novel laser guide star: Projected pupil plane pattern (PPPP) [P1060] | Huizhe Yang |
| The CAOS Problem-Solving Environment: tools for AO numerical modeling and post-AO deconvolution [P1061] | M. Carbillet |
| Python based AOTools - There is a better way [P1062] | Matthew J Townson |
| Latest AO simulation results for the E-ELT [P1063] | Miska Le Louarn |
| Integrated Modeling and Adaptive Optics [P1064] | R. CONAN |
| Analyzing the Operational Behavior of the Alignment and Phasing System of the Thirty Meter Telescope using SysML [P1065] | Sebastian J. I. Herzig |
| Performance of TMT's NFIROAS on Maunakea versus La Palma [P1066] | Tony Travouillon |
| GMCAO simulation tool development [P1067] | Valentina Viotto |
| Tuesday 27th June | ||
| Invited talks | ||
| chair: Antonin Bouchez | ||
| 8:50 | E-ELT design and status | Michele Cirasuolo |
| Current designs of E-ELT AO systems | ||
| 9:20 | Wide-field Adaptive Optics for MOSAIC, the multiple object spectrograph for the E-ELT | Tim Morris |
| 9:40 | The METIS Laser Tomographic AO system | Remko Stuik |
| 10:00 | On the road to the Preliminary Design Review of the MAORY adaptive optics module for E-ELT | Emiliano Diolaiti |
| 10:20 | Towards an overall astrometric error budget with MICADO-MCAO | Gabriele Rodeghiero |
| 10:40 | The Adaptive Optics modes for HARMONI – From Classical to Laser Assisted Tomographic AO | Benoit Neichel |
| 11:00 | Coffee break | |
| Wavefront correction | ||
| chair: Norbert Hubin | ||
| 11:30 | The E-ELT M4, on its way to become reality | Elise Vernet |
| 11:50 | SWAP DM: preliminary design and schematics of a deformable mirror (DM) for extreme adaptive optics | Teresa Kopf |
| 12:10 | Technology and control for extremely accurate and stable open-loop deformable mirrors | Urban Bitenc |
| 12:30 | MEMS Deformable Mirrors for ELTs | Paul Bierden |
| 12:50 | Segmented deformable mirrors for Ground layer Adaptive Optics | Edward Kibblewhite |
| 13:10 | Next generation of piezo deformable mirrors | Hubert Pages |
| 13:30 | Lunch | |
| ELT science with AO | ||
| chair: Corinne Boyer | ||
| 14:50 | High angular resolution at GTC: Science capabilities of FRIDA+GTCAO | Almudena Prieto |
| 15:10 | Prospects of Deep Field Surveys with Global-MCAO on an ELT | Elisa Portaluri |
| 15:30 | What do we really know about extrasolar planets? | Katie M. Morzinski |
| AO pathfinders and new concepts | ||
| 15:50 | SCExAO as a prototyping platform available to the ELT extreme-AO community | Olivier Guyon |
| 16:10 | Coffee break | |
| chair: Thierry Fusco | ||
| 16:30 | Which strategy for AO at LBTO in the 10+ years to come | Christian Veillet |
| 16:50 | GRAAL on-sky performance with the AOF | J. Paufique |
| 17:10 | ARGOS Imaging and Spectroscopy Performance at the LBT | S. Rabien |
| 17:30 | Never enough resolution: boost it with KERNEL interferometry | F. Martinache |
| 18:00 | Poster session 2 |
Poster session 2
Wavefront correction
| Next Generation Adaptive Optics on the TMT: A Low-Voltage ASIC Driver for MEMS Deformable Mirrors [P2001] | Colin Ross |
| GMT M2 units positioners system design and analysis [P2002] | Daniele Gallieni |
| Deformable mirror characterisation from ambient down to -40C [P2003] | Francois Rigaut |
| The challenge of MOEMS Deformable Mirrors tested in cryo for future AO systems [P2004] | Frederic Zamkotsian |
| The LBT Adaptive Secondary Thin Shells [P2005] | G. Brusa |
| Re-commissioning of the VLT/UT4 telescope after the Deformable Secondary Mirror instalation [P2006] | Hibon Pascale |
| XAO for the E-ELT and CHARA upgrade: Two examples of deformable mirror optimization [P2007] | Julien Charton |
| Multiphysiscs dynamic simulation of the E-ELT M4 adaptive mirror during earthquake [P2008] | Mauro Manetti |
| Direct expansion gas cooling technology applied to the E-ELT M4 adaptive mirror [P2009] | R. Biasi |
| Optical calibration of the E-ELT adaptive mirror M4: testing protocol and assessment of the measurement accuracy [P2010] | Giorgio Pariani |
| Optical calibration of the E-ELT adaptive mirror M4: Strategy for optical measurement error estimation [P2011] | Giorgio Pariani |
| Optical calibration of the E-ELT adaptive mirror M4: design, alignment and verification of the interferometric test tower [P2012] | Giorgio Pariani |
| ESO’s Deformable Mirrors development program [P2013] | Stefan Stroebele |
Wavefront sensing
| Using unmanned aerial vehicles for AO tip-tilt measurement [P2014] | Alastair Basden |
| Roof- and Pyramid Wavefront Sensing with Extended Sources [P2015] | Brent Ellerbroek |
| Numerical Evaluation of Pyramid Type Sensors for Extreme Adaptive Optics for the European Extremely Large Telescope [P2016] | Byron Engler |
| The TP3-WFS: a new guy in town [P2017] | Carlos Colodro Conde |
| Acquisiton with the TMT IRIS On-Instrument Wavefront Sensor System [P2018] | David Andersen |
| Recovering pyramid WS gain in non-common path aberration correction mode via deformable lens [P2019] | Demetrio Magrin |
| Phasing the GMT with a next generation e-APD dispersed fringe sensor: design and on-sky prototyping [P2020] | Derek Kopon |
| On-sky performance of the QACITS pointing control technique with the Keck/NIRC2 vortex coronagraph [P2021] | Elsa Huby |
| Current status and implementation of pyramid truth wavefront sensor on NFIROAS simulation bench at NRC-Herzberg [P2022] | Etsuko Mieda |
| SHARK-VIS the LBT high contrast imager at visible wavelengths [P2023] | F. Pedichini |
| SPOOF: Spot Packing Optimisation on Optical Frames [P2024] | Francois Rigaut |
| Final performance of NGS2 at Factory Acceptance Tests [P2025] | Francois Rigaut |
| On-sky performance demonstration of the near infrared SAPHIRA e-APD array and new developments of e-APD technology [P2026] | Gert Finger |
| Shack-Hartmann wavefront sensor sensitivity loss factor estimation in partial correction regime [P2027] | Carmelo Arcidiacono |
| The use of an axicon beam-shaping element in non-modulated pyramid wavefront sensors [P2028] | Denis Brousseau |
| New wave front sensor for adaptive optics and cophasing of segmented mirrors [P2029] | José Manuel Rodríguez-Ramos |
| Comparison of different wavefront sensing methods for phase discontinuity measurement [P2030] | K. El Hadi |
| Focal plane complex wavefront sensing with coronagraphic phase diversity on the THD2 bench [P2031] | L. M. Mugnier |
| Post-coronagraphic wavefront sensing for segmented pupils [P2032] | Lucie Leboulleux |
| Development & Verification of the non-Linear Curvature Wavefront Sensor [P2033] | Mala Mateen |
| Binary Adaptive Optics [P2034] | Manuel P. Cagigal |
| Design and status of the NGS WFS of MAORY [P2035] | Marco Bonaglia |
| Update AO Detector Developments at ESO [P2036] | Mark Downing |
| Utility of Photon-Counting, Energy-Resolving Detectors in Wavefront Sensing [P2037] | Michael P. Fitzgerald |
| Automatic determination of noises and gains of wavefront sensors on CANARY data [P2038] | Michel Tallon |
| A low-cost, very high-order Shack-Hartmann sensor for testing TMT deformable mirrors [P2039] | Mojtaba Taheri |
| Optical design, simulation and laboratory characterisation of CAWS: the Calibration and Alignment Wavefront Sensor for High-order adaptive optics [P2040] | Nicolas Dubost |
| The Plenoptic Camera as wavefront sensor for the VTT Solar Telescope [P2041] | Noelia Martínez Rey |
| Achromatic double-roof prism wavefront sensor: a cheaper alternative to the double-pyramid? [P2042] | Olivier Lardière |
| Scintillation and ELTs [P2043] | Ollie Farley |
| Wavefront sensing detectors: 2 decades of technological progress [P2044] | Philippe Feautrier |
| Self-Coherent Camera At The Palomar Observatory [P2045] | Raphaël Galicher |
| Speckle Statistics in Extreme Adaptive Optics Near-Infrared Images [P2046] | Sean B. Goebel |
| Wavefront sensing for a future HabEx space telescope [P2047] | Stefan Martin |
| Spatial Filtering of a Pyramid Wavefront Sensor on the High Order Testbench [P2048] | Tyler Banas |
| Dispersed fringe sensor for phasing the multi-aperture optical telescope [P2049] | Shengqian Wang |
| A Holographic Diffuser Generalised Optical Differentiation Wavefront Sensor [P2062] | Luca Marafatto |
ELT science with AO
| Multi-Conjugate Adaptive Optics (MCAO) images of the molecular hydrogen in the planetary nebula NGC 2346, obtained with GSAOI [P2050] | Arturo Manchado |
| Searching for Habitable Exoplanets in the Alpha Centauri Star System with the 10-micron TIKI Camera [P2051] | Christian Marois |
| Observing exoplanets with high dispersion coronagraphy. I. The scientific potential of current and next-generation large ground-based telescopes [P2052] | Dimitri Mawet |
| AO science operations review: from the VLT to ELTs [P2053] | Julien Girard |
| Looking for low-mass planets in Alpha Centauri with the VLT [P2054] | Markus Kasper |
| Developing post-coronagraphic, high-resolution spectroscopy for terrestrial planet characterization on ELTs [P2055] | Nemanja Jovanovic |
| QSO host galaxy and environments in the ELT era [P2056] | Simona Paiano |
| The driving science for TMT’s AO systems [P2057] | Warren Skidmore |
Solar AO
| Monte-Carlo modelling of solar adaptive optics systems [P2058] | Alastair Basden |
| Adaptive optics for high precision polarimetry [P2059] | Marco Stangalini |
| THEMIS solar adaptive optics: Laboratory integration and validations status before commissioning [P2060] | Maud Langlois |
| Blur: Solar Multi-Conjugate Adaptive Optics Simulations [P2061] | Jose Marino |
| Thursday 29th June | ||
| Laser guide star systems | ||
| chair: Celine d'Orgeville | ||
| 9:00 | Laser Workshop review | Céline D'Orgeville |
| 9:20 | Terrestrial combination of multiple sodium guidestar laser beams for increased on-sky brightness | Dr. Robert Johnson |
| 9:40 | First on-sky results of the CANARY experiment with an ELT-elongated sodium LGS | Lisa Bardou |
| 10:00 | The Horizontal Structure Function of the Sodium Centroid in the upper Mesosphere | Thomas Pfrommer |
| 10:20 | Laser Guide Star return flux at Cerro Paranal and at the Canary Islands | Domenico Bonaccini Calia |
| 10:40 | LGS spot truncation mitigation in ELTs: optimizing the pixel usage | Leonardo Blanco |
| 11:00 | Coffee break | |
| Wavefront sensing | ||
| chair: Simone Esposito | ||
| 11:30 | Infrared detectors for wavefront sensing | JL Gach |
| 11:50 | Microwave Kinetic Inductance Detectors for High Contrast Imaging | Benjamin A. Mazin |
| 12:10 | e2v sensors for adaptive optics wavefront sensing | Paul Jorden |
| AO pathfinders and new concepts | ||
| 12:30 | Three years of SPHERE operation at the VLT: status, future prospects and lessons learned for ELT instrumentation | Jean-Luc Beuzit |
| 12:50 | `imaka - a wide-field GLAO demonstrator for Maunakea | Jessica Lu |
| 13:10 | Riding the waves with AOLI: presentation, commissioning and AIV innovations | Sergio Velasco |
| 13:30 | Lunch | |
| AO reconstruction and control | ||
| chair: Yutaka Hayano | ||
| 14:50 | Towards minimum-variance control of ELTs AO systems | Caroline Kulcsár |
| 15:10 | Tomographic errors for wide field AO systems on E-ELTs ? impact on telescope design and ultimate performances | T. Fusco |
| 15:30 | On the optimality of wavefront reconstructors from gradients at the ELT scale | Clémentine Béchet |
| 15:50 | On-sky testing of algorithms for extended LGS spots | Alastair Basden |
| 16:10 | Coffee break | |
| chair: Caroline Kulcsar | ||
| 16:30 | Mitigate the impact of ELT architecture on AO performance: learn from todays?s telescopes to characterize and prevent the low-wind | M. N'Diaye |
| 16:50 | Closed-loop Estimation of the AO Interaction Matrix with Minimal Perturbation | Niek Doelman |
| 17:10 | Green Flash: Exploiting future and emerging computing technologies for AO RTC at ELT scale | Damien Gratadour |
| 17:30 | GENDER IN AO DISCUSSION | |
| 18:00 | Poster session 3 | |
| 20:30 | Conference dinner |
Poster session 3
Laser guide star systems
| Canary Phase D: On Sky Testing of the European ELT LGS AO Configuration [P3001] | Andrew P Reeves |
| Semiconductor Guidestar Laser for Astronomy, Space, and Laser Communications [P3002] | Celine d'Orgeville |
| Experiments at the WHT on LGS-AO with Pyramid WFS and pulsed lasers [P3003] | Domenico Bonaccini Calia |
| Tracking the sodium layer altitude with GeMS in the era of NGS2 [P3004] | Eduardo Marin |
| predicting the photon returns from the sodium layer using a pulsed laser format [P3005] | Edward Kibblewhite |
| Aircraft safety and operational efficiency during LGS operations at the Large Binocular Telescope Observatory [P3006] | Gustavo Rahmer |
| Trade-off evaluation of the alternatives for GTC Laser Guide Star (LGS) System [P3007] | J. Sánchez-Capuchino |
| Modeling the response of mesospheric sodium to pulsed-laser excitation [P3008] | Joschua A. Hellemeier |
| Laser Guide Star Objective of MAORY [P3009] | Matteo Lombini |
| LGS AO error budget analysis using Keck II AO telemetry data [P3010] | Matthias Schoeck |
| Ingot Laser Guide Stars WaveFront Sensing [P3011] | Ragazzoni R. |
| Development of extreme narrow band filter for LGS daytime use [P3012] | Yutaka Hayano |
Site testing and characterization
| Water vapor forecast for LBTI (LBTO) and VISIR (VLT) [P3013] | Alessio Turchi |
| Turbulence Profiling at Cerro Las Campanas Using a Laser Scintillometer [P3014] | Antonin H. Bouchez |
| CATS : a new station for a complete characterization of atmospheric turbulence [P3015] | Aziz ZIAD |
| The Generalized FASS (Full Aperture Seeing Sensor): filling the lower altitudes of the Cn2 profile [P3016] | Clémentine Béchet |
| Quantitative characterisation of sky conditions on Paranal with the microwave radiometer LHATPRO – perspectives toward science operations of the E-ELT [P3017] | Florian Kerber |
| Photometry and Spectrum measurements of the Laser Guide Star beam emission at Observatorio del Roque de Los Muchachos with the Gran Telescopio CANARIAS [P3018] | G. Lombardi |
| Stereo-SCIDAR at ESO: One year of results [P3019] | James Osborn |
| Evaluation of statistical turbulence models for use in the Distributed Kalman Filter [P3020] | Jesse Cranney |
| Determining ground layer turbulence statistics using a SLODAR-type method [P3021] | Jonatan Lehtonen |
| Coherence time ($tau_0$) at Roque de los Muchachos Observatory (Canary Islands) [P3022] | Julio Castro-Almazan |
| The Canarian Observatories G-SCIDAR turbulence profile database (CanSciDat): data release [P3023] | Julio Castro-Almazan |
| Estimation of daytime vertical turbulence profile at Obervatorio del Teide from the radiosonde database [P3024] | Luzma Montoya |
| Sodium Layer Statistics from the Canary High-Resolution Sodium Profiler [P3025] | Matthew J Townson |
| Atmospheric coherence time and turbulence altitude information from the SHIMM seeing monitor [P3026] | Saavidra Perera |
| Nowcasting and forecasting of the surface layer of turbulence at Paranal Observatory [P3027] | Timothy Butterley |
| Site characterization at Mount Stromlo Observatory: the first results [P3028] | Visa Korkiakoski |
| Turbulence profiling simulation for tomographic AO systems in ELTs [P3029] | Yoshito Ono |
AO reconstruction and control
| New adaptive optics Tomographic Pupil Image reconstructor based on convolutional neural networks [P3030] | Carlos Gonzalez Gutiérrez |
| Low-order mode estimation in LTAO systems from natural guide stars [P3031] | Carlos M. Correia |
| The measurement of the Interaction Matrices for the LINC-NIRVANA MCAO [P3032] | Carmelo Arcidiacono |
| Fourier reconstruction for future adaptive optics systems [P3033] | Charlotte Z Bond |
| Optimising the performance of a Pyramid WFS: tracking the optical gain [P3034] | Charlotte Z Bond |
| RTC strategies for Harmoni SCAO and LTAO modes [P3035] | Cyril Petit |
| ELT-scale real-time control on Intel Xeon Phi and many core CPUs [P3036] | David Jenkins |
| A generic and scalable heterogeneous architecture for real-time computing and performances measurements in AO [P3037] | denis perret |
| Optical design and wavefront control for vortex coronagraphs on large segmented aperture telescopes [P3038] | Garreth Ruane |
| Preliminary performance results of the "Weighted Fourier Phase Slope" centroiding method for Shack Hartmann wavefront sensors obtained with the OOMAO simulator [P3039] | Haresh M. Chulani |
| Bumpless SPHERE LQG tip/tilt control with the control switching adaptor [P3040] | Henri-François Raynaud |
| Two novel algorithms for wavefront reconstruction from pyramid sensor data: Convolution with Linearized Inverse Filter and Pyramid Fourier Transform Reconstructor [P3041] | Iuliia Shatokhina |
| ADRC: a strategy to deal with adaptive optics feedback control [P3042] | Luis F. Rodríguez-Ramos |
| Time performance setup for the GTCAO real-time control host [P3043] | José Marco de la Rosa |
| GTC AO Mechanisms Software Control [P3044] | Josefina Rosich |
| A GPU based RTC for E-ELT Adaptive optics: RTC prototype [P3045] | Julien Bernard |
| Performance of the extreme-AO instrument SPHERE and dependence on the atmospheric conditions [P3046] | Julien Milli |
| Wind Predictive Wavefront Control [P3047] | Tom Herbst |
| Distributed Kalman filter implementation issues for ELT AO control [P3048] | Léonard Prengère |
| Real time controller based on FPGA and DSP for solar AO system and solar MCAO prototype [P3049] | Youming Guo |
| Performance of AO predictive control in the presence of non-stationary turbulence [P3050] | Maaike van Kooten |
| The ARGOS vibration compensation system [P3051] | Matthias Rosensteiner |
| Real-time Shack-Hartmann wavefront sensor reference scaling compensates for beacon size and shape [P3052] | Michael J. Steinbock |
| Feedback control baseline strategies for GTC adaptive optics with NGS [P3053] | Miguel Núñez |
| Efficient supervision strategy for tomographic AO systems on E-ELT [P3054] | N. Doucet |
| FPGA based microserver for high performance real-time computing in Adaptive Optics [P3055] | R. Biasi |
| Reconstruction Methods for Adaptive Optics [P3056] | Ronny Ramlau |
| Wavefront Reconstruction from Pyramid Sensor Measurements based on the Inversion of the Finite Hilbert Transform [P3057] | Victoria Hutterer |
| Modal Control Gains Optimization for the Pyramid Wavefront Sensor: Numerical Simulations and Optical Bench Validation [P3058] | Vincent Deo |
| Efficient tomographic wave-front reconstruction with Toeplitz matrix structure for LTAO systems in ELTs [P3059] | Yoshito Ono |
Post-processing of AO data
| Correction of distortion for Wide Field Adaptive Optics images [P3060] | Anaïs Bernard |
| PSF reconstruction for integral field spectrograph [P3061] | Anna Ciurlo |
| Processing multispectral high-contrast images: MEDUSAE, an inverse problem approach [P3062] | Cantalloube Faustine |
| PSF reconstruction via full turbulence estimation and telescope end-to-end simulation [P3063] | Clémentine Béchet |
| Accurate uncertainty estimation in crowded fields observed with AO [P3064] | E. Gallego-Cano |
| Processing diffraction-limited images through innovative Super-Resolution techniques [P3065] | Sergio Velasco |
| Post-coronagraphic PSF sharpening with the vortex coronagraph [P3066] | Gilles Orban de Xivry |
| Point spread function reconstruction analysis, modelling, simulations, and tests on the HeNOS bench at NRC-Herzberg [P3067] | Luc Gilles |
| Point Spread Function Determination at W. M. Keck Observatory: Science Verification and Facility Development [P3068] | Sam Ragland |
The schedule of the programme can be downloaded here.
