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Astrometry is one of the main science case which drives the requirements of the next multiconjugate adaptive optics (MCAO) systems for future extremely large telescopes. The small diffraction limited point-spread function (PSF) and the high…

Instrumentation and Methods for Astrophysics · Physics 2019-05-09 M. Patti , C. Arcidiacono , M. Lombini , E. Diolaiti , F. Cortecchia

In the last few years, new Adaptive Optics [AO] techniques have emerged to answer new astronomical challenges: Ground-Layer AO [GLAO] and Multi-Conjugate AO [MCAO] to access a wider Field of View [FoV], Multi-Object AO [MOAO] for the…

Astrophysics · Physics 2009-11-11 B. Neichel , J-M. Conan , T. Fusco , E. Gendron , M. Puech , G. Rousset , F. Hammer

The SINFONI instrument for ESO's VLT combines integral field spectroscopy and adaptive optics (AO). We discuss detailed simulations of the adaptive optics module. These simulations are aimed at assessing the AO module performance,…

Astrophysics · Physics 2009-11-10 Anthony G A Brown , Enrico Fedrigo , Paul van der Werf

EAGLE 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.…

The MCAO Assisted Visible Imager and Spectrograph (MAVIS) is a new visible instrument for ESO Very Large Telescope (VLT). Its Adaptive Optics Module (AOM) must provide extreme adaptive optics correction level at low galactic latitude and…

Instrumentation and Methods for Astrophysics · Physics 2022-09-01 Guido Agapito , Daniele Vassallo , Cédric Plantet , Jesse Cranney , Hao Zhang , Valentina Viotto , Enrico Pinna , Francois Rigaut

This article reports on the results of simulations conducted to assess the performance of a modal Multi-Conjugate Adaptive Optics (MCAO) system on a 10m telescope with one Deformable Mirror (DM) conjugated to the telescope pupil and a…

Astrophysics · Physics 2009-11-07 B. Femenia , N. Devaney

The Multi-adaptive optics Imaging CamerA for Deep Observations (MICADO) will image a field of view of nearly 1 arcminute at the diffraction limit of the Extremely Large Telescope (ELT), making use of the adaptive optics correction provided…

METIS, the Mid-Infrared ELT Imager and Spectrograph, is one of the four first-generation ELT instruments scheduled to see first light in 2028. Its two main science modules are supported by an adaptive optics system featuring a pyramid…

Instrumentation and Methods for Astrophysics · Physics 2023-11-23 Markus Feldt , Horst Steuer , Carlos Correia , Andreas Obereder , Stefan Raffetseder , Thomas Bertram , Julia Shatokina , Faustine Cantalloube

Context: Current instrument developments at the largest telescopes worldwide have provisions for Multi-Conjugated Adaptive Optics (MCAO) modules. The large field of view and more uniform correction provided by these systems is not only…

Instrumentation and Methods for Astrophysics · Physics 2015-05-28 Eva Meyer , Martin Kuerster , Carmelo Arcidiacono , Roberto Ragazzoni , Hans-Walter Rix

Since the year 2000, adaptive optics (AO) has seen the emergence of a variety of new concepts addressing particular science needs; multiconjugate adaptive optics (MCAO) is one of them. By correcting the atmospheric turbulence in 3D using…

Instrumentation and Methods for Astrophysics · Physics 2020-03-09 Francois Rigaut , Benoit Neichel

MICADO is the adaptive optics imaging camera being studied for the E-ELT. Its design has been optimised for use with MCAO, but will have its own SCAO module for the initial operational phase; and in principle could also be used with GLAO or…

Instrumentation and Methods for Astrophysics · Physics 2015-05-14 R. Davies , the Micado team

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…

First multi-conjugate adaptive-optical (MCAO) systems are currently being installed on solar telescopes. The aim of these systems is to increase the corrected field-of-view with respect to conventional adaptive optics. However, this first…

Instrumentation and Methods for Astrophysics · Physics 2015-06-05 Aglae Kellerer

The Multiconjugate Adaptive optics Demonstrator (MAD) for ESO-Very Large Telescopes (VLT) will demonstrate on sky the MultiConjugate Adaptive Optics (MCAO) technique. In this paper the laboratory tests relative to the first preliminary…

Instrumentation and Methods for Astrophysics · Physics 2014-11-20 Carmelo Arcidiacono , Matteo Lombini , Emiliano Diolaiti , Jacopo Farinato , Roberto Ragazzoni

CANARY is the multi-object adaptive optics (MOAO) on-sky pathfinder developed in the perspective of Multi-Object Spectrograph on Extremely Large Telescopes~(ELTs). In 2013, CANARY was operated on-sky at the William Herschel telescope~(WHT),…

Instrumentation and Methods for Astrophysics · Physics 2017-02-01 O. A. Martin , É. Gendron. , G. Rousset , D. Gratadour , F. Vidal , T. J. Morris , A. G. Basden , R. M. Myers , C. M. Correia , D. Henry

The High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) is the visible and near-infrared (NIR), adaptive-optics-assisted, integral field spectrograph for ESO's Extremely Large Telescope (ELT).…

MICADO is a first light instrument for the Extremely Large Telescope (ELT), set to start operating later this decade. It will provide diffraction limited imaging, astrometry, high contrast imaging, and long slit spectroscopy at…

Instrumentation and Methods for Astrophysics · Physics 2024-08-30 E. Sturm , R. Davies , J. Alves , Y. Clénet , J. Kotilainen , A. Monna , H. Nicklas , J. -U. Pott , E. Tolstoy , B. Vulcani , J. Achren , S. Annadevara , H. Anwand-Heerwart , C. Arcidiacono , S. Barboza , L. Barl , P. Baudoz , R. Bender , N. Bezawada , F. Biondi , P. Bizenberger , A. Blin , A. Boné , P. Bonifacio , B. Borgo , J. van den Born , T. Buey , Y. Cao , F. Chapron , G. Chauvin , F. Chemla , K. Cloiseau , M. Cohen , C. Collin , O. Czoske , J. -O. Dette , M. Deysenroth , E. Dijkstra , S. Dreizler , O. Dupuis , G. van Egmond , F. Eisenhauer , E. Elswijk , A. Emslander , M. Fabricius , G. Fasola , F. Ferreira , N. M. Förster Schreiber , A. Fontana , J. Gaudemard , N. Gautherot , E. Gendron , C. Gennet , R. Genzel , L. Ghouchou , S. Gillessen , D. Gratadour , A. Grazian , F. Grupp , S. Guieu , M. Gullieuszik , M. de Haan , J. Hartke , M. Hartl , F. Haussmann , T. Helin , H. -J. Hess , R. Hofferbert , H. Huber , E. Huby , J. -M. Huet , D. Ives , A. Janssen , P. Jaufmann , T. Jilg , D. Jodlbauer , J. Jost , W. Kausch , H. Kellermann , F. Kerber , H. Kravcar , K. Kravchenko , C. Kulcsár , H. Kunkarayakti , P. Kunst , S. Kwast , F. Lang , J. Lange , V. Lapeyrere , B. Le Ruyet , K. Leschinski , H. Locatelli , D. Massari , S. Mattila , S. Mei , F. Merlin , E. Meyer , C. Michel , L. Mohr , M. Montargès , F. Müller , N. Münch , R. Navarro , U. Neumann , N. Neumayer , L. Neumeier , F. Pedichini , A. Pflüger , R. Piazzesi , L. Pinard , J. Porras , E. Portaluri , N. Przybilla , S. Rabien , J. Raffard , R. Raggazoni , R. Ramlau , J. Ramos , S. Ramsay , H. -F. Raynaud , P. Rhode , A. Richter , H. -W. Rix , M. Rodenhuis , R. -R. Rohloff , R. Romp , P. Rousselot , N. Sabha , B. Sassolas , J. Schlichter , M. Schuil , M. Schweitzer , U. Seemann , A. Sevin , M. Simioni , L. Spallek , A. Sönmez , J. Suuronen , S. Taburet , J. Thomas , E. Tisserand , P. Vaccari , E. Valenti , G. Verdoes Kleijn , M. Verdugo , F. Vidal , R. Wagner , M. Wegner , D. van Winden , J. Witschel , A. Zanella , W. Zeilinger , J. Ziegleder , B. Ziegler

In this paper, we present a first comparison of different Adaptive Optics (AO) concepts to reach a given scientific specification for 3D spectroscopy on Extremely Large Telescope (ELT). We consider that a range of 30%-50% of Ensquarred…

We discuss how to optimise the science output of the European Solar Telescope (EST), when used without the wide-field compensation for high-altitude seeing that the EST multi conjugate adaptive optics (MCAO) will offer. This will be the…

Instrumentation and Methods for Astrophysics · Physics 2026-05-05 G. B. Scharmer , M. G. Löfdahl , J. de la Cruz Rodríguez , B. Lindberg , H. Socas-Navarro , D. Kiselman , M. Rempel , J. Leenaarts

In order to increase the corrected field of view of an adaptive optics (AO) system, several deformable mirrors (DM) have to be placed in the conjugate planes of the dominant turbulent layers (multi-conjugate adaptive optics, MCAO [Beckers…

Astrophysics · Physics 2022-04-20 T. Berkefeld , A. Glindemann , S. Hippler