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Related papers: GRAVITY+ Wavefront Sensors: High-Contrast, Laser G…

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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

GRAVITY is a second generation instrument for the VLT Interferometer, designed to enhance the near-infrared astrometric and spectro-imaging capabilities of VLTI. Combining beams from four telescopes, GRAVITY will provide an astrometric…

In the context of the GRAVITY+ upgrade, the adaptive optics (AO) systems of the GRAVITY interferometer are undergoing a major lifting. The current CILAS deformable mirrors (DM, 90 actuators) will be replaced by ALPAO kilo-DMs (43x43, 1432…

This article describes the operation of the near-infrared wavefront sensing based Adaptive Optics (AO) system CIAO. The Coud\'e Infrared Adaptive Optics (CIAO) system is a central auxiliary component of the Very Large Telescope (VLT)…

The GRAVITY instrument has been revolutionary for near-infrared interferometry by pushing sensitivity and precision to previously unknown limits. With the upgrade of GRAVITY and the Very Large Telescope Interferometer (VLTI) in GRAVITY+,…

Instrumentation and Methods for Astrophysics · Physics 2023-07-12 GRAVITY+ Collaboration , : , Roberto Abuter , Patricio Alarcon , Fatme Allouche , Antonio Amorim , Christophe Bailet , Helen Bedigan , Anthony Berdeu , Jean-Philippe Berger , Philippe Berio , Azzurra Bigioli , Richard Blaho , Olivier Boebion , Marie-Lena Bolzer , Henri Bonnet , Guillaume Bourdarot , Pierre Bourget , Wolfgang Brandner , Cesar Cardenas , Ralf Conzelmann , Mauro Comin , Yann Clénet , Benjamin Courtney-Barrer , Yigit Dallilar , Ric Davies , Denis Defrère , Alain Delboulbé , Françoise Delplancke-Ströbele , Roderick Dembet , Tim de Zeeuw , Antonia Drescher , Andreas Eckart , Clemence Édouard , Frank Eisenhauer , Maximilian Fabricius , Helmut Feuchtgruber , Gert Finger , Natascha M. Förster Schreiber , Eloy Fuenteseca , Enrique Garcia , Paulo Garcia , Feng Gao , Eric Gendron , Reinhard Genzel , Juan Pablo Gil , Stefan Gillessen , Tiago Gomes , Frédéric Gonté , Carole Gouvret , Patricia Guajardo , Ivan Guidolin , Sylvain Guieu , Ronald Guzmann , Wolfgang Hackenberg , Nicolas Haddad , Michael Hartl , Xavier Haubois , Frank Haußmann , Gernot Heißel , Thomas Henning , Stefan Hippler , Sebastian Hönig , Matthew Horrobin , Norbert Hubin , Estelle Jacqmart , Laurent Jocou , Andreas Kaufer , Pierre Kervella , Jean-Paul Kirchbauer , Johan Kolb , Heidi Korhonen , Laura Kreidberg , Peter Krempl , Sylvestre Lacour , Stephane Lagarde , Olivier Lai , Vincent Lapeyrère , Romain Laugier , Jean-Baptiste Le Bouquin , James Leftley , Pierre Léna , Steffan Lewis , Dieter Lutz , Yves Magnard , Felix Mang , Aurelie Marcotto , Didier Maurel , Antoine Mérand , Florentin Millour , Nikhil More , Hugo Nowack , Matthias Nowak , Sylvain Oberti , Francisco Olivares , Thomas Ott , Laurent Pallanca , Thibaut Paumard , Karine Perraut , Guy Perrin , Romain Petrov , Oliver Pfuhl , Nicolas Pourré , Sebastian Rabien , Christian Rau , Miguel Riquelme , Sylvie Robbe-Dubois , Sylvain Rochat , Muhammad Salman , Malte Scherbarth , Markus Schöller , Joseph Schubert , Nicolas Schuhler , Jinyi Shangguan , Pavel Shchekaturov , Taro Shimizu , Silvia Scheithauer , Arnaud Sevin , Christian Soenke , Ferreol Soulez , Alain Spang , Eric Stadler , Christian Straubmeier , Eckhard Sturm , Calvin Sykes , Linda Tacconi , Helmut Tischer , Konrad Tristram , Frédéric Vincent , Sebastiano von Fellenberg , Sinem Uysal , Felix Widmann , Ekkehard Wieprecht , Erich Wiezorrek , Julien Woillez , Şenol Yazıcı , Gérard Zins

We present the proposal for the infrared adaptive optics (AO) assisted, two-object, high-throughput, multiple-beam-combiner GRAVITY for the VLTI. This instrument will be optimized for phase-referenced interferometric imaging and…

Astrophysics · Physics 2007-05-23 F. Eisenhauer , G. Perrin , S. Rabien , A. Eckart , P. Lena , R. Genzel , R. Abuter , T. Paumard , W. Brandner

Context. The GRAVITY+ upgrade implies a complete renewal of its adaptive optics (AO) systems. Its complex design, featuring moving components between the deformable mirrors and the wavefront sensors, requires the monitoring and…

Full sky coverage Adaptive Optics on Extremely Large Telescopes requires the adoption of several Laser Guide Stars as references.With such large apertures, the apparent elongation of the beacons is absolutely significant.With few…

We present the adaptive optics assisted, near-infrared VLTI instrument - GRAVITY - for precision narrow-angle astrometry and interferometric phase referenced imaging of faint objects. Precision astrometry and phase-referenced…

HARMONI is a visible and near-infrared integral field spectrograph equipped with two complementary adaptive optics systems, fully integrated within the instrument. A Single Conjugate AO (SCAO) system offers high performance for a limited…

In the last decade, the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the European Virgo observatory have opened a new observational window on the universe. These cavity-enhanced laser interferometers sense spacetime…

GRAVITY is an adaptive optics assisted Beam Combiner for the second generation VLTI instrumentation. The instrument will provide high-precision narrow-angle astrometry and phase-referenced interferometric imaging in the astronomical K-band…

Observational tests of ground layer wavefront recovery have been made in open loop using a constellation of four natural guide stars at the 1.55 m Kuiper telescope in Arizona. Such tests explore the effectiveness of wide-field seeing…

Astrophysics · Physics 2011-02-11 Christoph Baranec , Michael Lloyd-Hart , N. Mark Milton

GRAVITY+ is the upgrade of GRAVITY and the Very Large Telescope Interferometer (VLTI) with wide-separation fringe tracking, new adaptive optics, and laser guide stars on all four 8~m Unit Telescopes (UTs), for ever fainter, all-sky, high…

Instrumentation and Methods for Astrophysics · Physics 2022-09-14 GRAVITY+ Collaboration , : , R. Abuter , F. Allouche , A. Amorim , C. Bailet , M. Bauböck , J. -P. Berger , P. Berio , A. Bigioli , O. Boebion , M. L. Bolzer , H. Bonnet , G. Bourdarot , P. Bourget , W. Brandner , Y. Clénet , B. Courtney-Barrer , Y. Dallilar , R. Davies , D. Defrère , A. Delboulbé , F. Delplancke , R. Dembet , P. T. de Zeeuw , A. Drescher , A. Eckart , C. Édouard , F. Eisenhauer , M. Fabricius , H. Feuchtgruber , G. Finger , N. M. Förster Schreiber , E. Garcia , P. Garcia , F. Gao , E. Gendron , R. Genzel , J. P. Gil , S. Gillessen , T. Gomes , F. Gonté , C. Gouvret , P. Guajardo , S. Guieu , M. Hartl , X. Haubois , F. Haußmann , G. Heißel , Th. Henning , S. Hippler , S. Hönig , M. Horrobin , N. Hubin , E. Jacqmart , L. Jochum , L. Jocou , A. Kaufer , P. Kervella , H. Korhonen , L. Kreidberg , S. Lacour , S. Lagarde , O. Lai , V. Lapeyrère , R. Laugier , J. -B. Le Bouquin , J. Leftley , P. Léna , D. Lutz , F. Mang , A. Marcotto , D. Maurel , A. Mérand , F. Millour , N. More , H. Nowacki , M. Nowak , S. Oberti , T. Ott , L. Pallanca , T. Paumard , K. Perraut , G. Perrin , R. Petrov , O. Pfuhl , N. Pourré , S. Rabien , C. Rau , S. Robbe-Dubois , S. Rochat , M. Salman , M. Schöller , J. Schubert , N. Schuhler , J. Shangguan , T. Shimizu , S. Scheithauer , A. Sevin , F. Soulez , A. Spang , E. Stadler , J. Stadler , C. Straubmeier , E. Sturm , L. J. Tacconi , K. R. W. Tristram , F. Vincent , S. von Fellenberg , S. Uysal , F. Widmann , E. Wieprecht , E. Wiezorrek , J. Woillez , S. Yazici , A. Young , G. Zins

The upgrade of the VLTI infrastructure for the 2nd generation instruments is now complete with the transformation of the laboratory, and installation of star separators on both the 1.8-m Auxiliary Telescopes (ATs) and the 8-m Unit…

The Max-Planck institutes for astronomy (MPIA) and for extraterrestrial physics (MPE) run an adaptive optics (AO) system with a laser guide star at the 3.5 m telescope on Calar Alto, Spain. This system, called ALFA, produces now scientific…

Instrumentation and Methods for Astrophysics · Physics 2016-07-20 Markus Kasper , Douglas Looze , Stefan Hippler , Ric Davies , Andreas Glindemann

MAORY is the adaptive optics module for ELT providing two gravity invariant ports with the same optical quality for two different client instruments. It enable high angular resolution observations in the near infrared over a large field of…

The very large telescope (VLT) interferometer (VLTI) in its current operating state is equipped with high-order adaptive optics (MACAO) working in the visible spectrum. A low-order near-infrared wavefront sensor (IRIS) is available to…

Future large space telescopes will be equipped with adaptive optics (AO) to overcome wavefront aberrations and achieve high contrast for imaging faint astronomical objects, such as earth-like exoplanets and debris disks. In contrast to AO…

Instrumentation and Methods for Astrophysics · Physics 2020-01-07 He Sun , N. Jeremy Kasdin , Robert Vanderbei
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