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Adaptive optics (AO) instruments for the future extremely large telescopes (ELTs) are characterized by advanced optical systems with diffraction-limited optical quality. Low geometric distortion is also crucial for high accuracy astrometric…

Instrumentation and Methods for Astrophysics · Physics 2019-04-02 Mauro Patti , Matteo Lombini , Edoardo Maria Alberto Redaelli , Emiliano Diolaiti

Ground-based telescopes have been playing a leading role in exoplanet direct imaging science and technological development for the past two decades and will continue to have an indispensable role for the next decade and beyond. Extreme…

Rather than using an adaptive optics (AO) system to correct a telescope s entire pupil, it can instead be used to more finely correct a smaller sub-aperture. Indeed, existing AO systems can be used to correct a sub-aperture 1/3 to 1/2 the…

Astrophysics · Physics 2009-11-13 E. Serabyn , K. Wallace , M. Troy , B. Mennesson , P. Haguenauer , R. Gappinger , R. Burruss

Adaptive optics (AO) systems and image reconstruction algorithms are indispensable tools when it comes to high-precision astrometry. In this paper, we analyze the potential of combining both techniques, i.e. by applying image reconstruction…

Instrumentation and Methods for Astrophysics · Physics 2019-03-13 Felix Bosco , Jörg-Uwe Pott , Rainer Schödel

Many adaptive optics systems operate by measuring the distortion of the wavefront in one wavelength range and performing the scientific observations in a second, different wavelength range. One common technique is to measure wavefront…

Astrophysics · Physics 2009-11-07 Henry G. Roe

Ground-based adaptive optics (AO) in the infrared has made exceptional advances in approaching space-like image quality at higher collecting area. Optical-wavelength applications are now also growing in scope. We therefore provide here a…

Instrumentation and Methods for Astrophysics · Physics 2009-09-25 Matt Mountain , Roeland van der Marel , Remi Soummer , Anton Koekemoer , Harry Ferguson , Marc Postman , Donald T. Gavel , Olivier Guyon , Douglas Simons , Wesley A. Traub

Autonomous highway driving, especially for long-haul heavy trucks, requires detecting objects at long ranges beyond 500 meters to satisfy braking distance requirements at high speeds. At long distances, vehicles and other critical objects…

Computer Vision and Pattern Recognition · Computer Science 2026-04-09 Parker Ewen , Dmitriy Rivkin , Mario Bijelic , Felix Heide

Performances of an adaptive optics (AO) system are directly linked with the quality of its alignment. During the instrument calibration, having open loop fast tools with a large capture range are necessary to quickly assess the system…

We briefly discuss the past, present, and future state of astronomical science with laser guide star adaptive optics (LGS AO). We present a tabulation of refereed science papers from LGS AO, amounting to a total of 23 publications as of May…

Astrophysics · Physics 2009-11-11 Michael C. Liu

We report on the first observation of cosmologically distant field galaxies with an high order Adaptive Optics (AO) system on an 8-10 meter class telescope. Two galaxies were observed at 1.6 microns at an angular resolution as high as 50…

Adaptive optics (AO) is a powerful image correction technique with proven benefits for many life-science microscopy methods. However, the complexity of adding a reflective wavefront modulator and a wavefront sensor into already complicated…

GRAVITY+ improves by orders of magnitude the sensitivity, sky-coverage and contrast of the Very Large Telescope Interferometer (VLTI). A central part of this project is the development of Gravity Plus Adaptive Optics (GPAO), a dedicated…

Instrumentation and Methods for Astrophysics · Physics 2026-03-11 GRAVITY+ Collaboration , : , F. Allouche , C. Bailet , M. Benisty , A. Berdeu , J. -P. Berger , P. Berio , A. Bigioli , C. Blanchard , O. Boebion , H. Bonnet , G. Bourdarot , P. Bourget , W. Brandner , J. Brulé , P. Burgos , M. Carbillet , C. Correia , B. Courtney Barrer , S. Curaba , R. Davies , D. Defrère , A. Delboulbé , F. Delplancke , R. Dembet , A. Drescher , N. Dubost , A. Eckart , C. Édouard , F. Eisenhauer , L. Esteras Otal , M. Fabricius , H. Feuchtgruber , P. Fédou , G. Finger , N. M. Förster Schreiber , R. Frahm , E. Garcia , P. Garcia , R. Garcia Lopez , R. Genzel , J. P. Gil , S. Gillessen , T. Gomes , F. Gonté , V. Gopinath , C. Gouvret , J. Graf , P. Guajardo , S. Guieu , W. Hackenberg , M. Hartl , X. Haubois , F. Haußmann , T. Henning , P. Hibon , S. Hönig , M. Horrobin , M. Houllé , N. Hubin , I. Ibn Taieb , L. Jochum , L. Jocou , A. Jost , J. Kammerer , L. Karl , A. Kaufer , P. Kern , P. Kervella , J. Kolb , H. Korhonen , L. Kreidberg , P. Krempl , S. Lacour , S. Lagarde , O. Lai , V. Lapeyrère , R. Laugier , V. Leal , J. -B. Le Bouquin , J. Leftley , P. Léna , B. Lopez , D. Lutz , Y. Magnard , F. Mang , A. Marcotto , D. Maurel , A. Mérand , F. Millour , M. Montarges , N. More , N. Morujão , T. Moulin , H. Nowacki , M. Nowak , S. Oberti , T. Ott , L. Pallanca , F. Patru , T. Paumard , K. Perraut , G. Perrin , P. O. Petrucci , R. Petrov , O. Pfuhl , N. Pourré , S. Rabien , C. Rau , M. Riquelme , S. Robbe-Dubois , S. Rochat , M. Salman , J. Sánchez-Bermúdez , J. Schubert , J. Scigliuto , P. Shchekaturov , N. Schuhler , J. Shangguan , T. Shimizu , S. Scheithauer , C. Soenke , F. Soulez , E. Stadler , J. Stadler , C. Straubmeier , E. Sturm , M. Subroweit , C. Sykes , L. J. Tacconi , K. R. W. Tristram , S. Uysal , S. von Fellenberg , F. Widmann , E. Wieprecht , E. Wiezorrek , J. Woillez , S. Yazici , G. Zins

The highest resolution images ever taken in the visible were obtained by combining Lucky Imaging and low order adaptive optics. This paper describes a new instrument to be deployed on the WHT 4.2m and GTC 10.4 m telescopes on La Palma, with…

The Adaptive Optics Lucky Imager (AOLI) is a new instrument designed to combine adaptive optics (AO) and lucky imaging (LI) techniques to deliver high spatial resolution in the visible, 20 mas, from ground-based telescopes. Here we present…

In order to avoid collisions with space debris, the near Earth orbit must be continuously scanned by either ground- or spaced-based facilities. For the low Earth orbit, radar telescopes are the workhorse for this task, especially due to…

Instrumentation and Methods for Astrophysics · Physics 2015-01-26 Daniel Hampf , Paul Wagner , Wolfgang Riede

The WHT is unusually well-placed for exploitation of adaptive-optics (AO) technology. The site seeing is excellent (median 0.7 arcsec), dome seeing is negligible, and preliminary studies indicate that most of the atmospheric seeing…

Astrophysics · Physics 2009-11-06 C. R. Benn

Twenty multiple stellar systems with solar-type primaries were observed at high angular resolution using the PALM-3000 adaptive optics system at the 5 m Hale telescope. The goal was to complement the knowledge of hierarchical multiplicity…

Solar and Stellar Astrophysics · Physics 2015-10-07 Lewis C. Roberts, , Andrei Tokovinin , Brian D. Mason , William I. Hartkopf , Reed L. Riddle

We conducted a survey of nearby binary systems composed of main sequence stars of spectral types F and G in order to improve our understanding of the hierarchical nature of multiple star systems. Using Robo-AO, the first robotic adaptive…

Non-line-of-sight (NLOS) imaging of objects not visible to either the camera or illumination source is a challenging task with vital applications including surveillance and robotics. Recent NLOS reconstruction advances have been achieved…

Image and Video Processing · Electrical Eng. & Systems 2019-07-30 Sreenithy Chandran , Suren Jayasuriya

A ground-layer adaptive optics system (GLAO) uses a single adaptive mirror to partially correct the wavefront for atmospheric and telescope aberrations over a wide field of view. Instead of reaching diffraction limit on a narrow field, the…

Instrumentation and Methods for Astrophysics · Physics 2017-06-02 Donald Gavel
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