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Related papers: The Mid-infrared E-ELT Imager and Spectrograph (ME…

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METIS, the Mid-infrared ELT Imager and Spectrograph (formerly called MIDIR), is a proposed instrument for the European Extremely Large Telescope (E-ELT), currently undergoing a phase-A study. The study is carried out within the framework of…

The Mid-infrared ELT Imager and Spectrograph (METIS) is a first-generation instrument for the Extremely Large Telescope (ELT), Europe's next-generation 39 m ground-based telescope for optical and infrared wavelengths. METIS will offer…

The Mid-infrared ELT Imager and Spectrograph (METIS) will provide the Extremely Large Telescope (ELT) with a unique window to the thermal- and mid-infrared (3 - 13 microns). Its single-conjugate adaptive optics (SCAO) system will enable…

The Mid-infrared ELT Imager and Spectrograph (METIS) is one of the first-generation scientific instruments for the ELT, built under the supervision of ESO by a consortium of research institutes across and beyond Europe. Designed to cover…

We present results of performance modelling for METIS, the Mid-infrared European Extremely Large Telescope (E-ELT) Imager and Spectrograph. Designed by a consortium of NOVA (Netherlands), UK Astronomy Technology Centre (UK), MPIA Heidelberg…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 Sarah Kendrew , Laurent Jolissaint , Bernhard Brandl , Rainer Lenzen , Eric Pantin , Alistair Glasse , Joris Blommaert , Lars Venema , Ralf Siebenmorgen , Frank Molster

METIS is a mid-infrared instrument proposed for the European Extremely Large Telescope (E-ELT). It is designed to provide imaging and spectroscopic capabilities in the 3 - 14 micron region up to a spectral resolution of 100000. One of the…

The ELT is a 39m large, ground-based optical and near- to mid-infrared telescope under construction in the Chilean Atacama desert. Operation is planned to start around the middle of the next decade. All first light instruments will come…

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

METIS is one of the three first-light instruments planned for the ELT, mainly dedicated to high contrast imaging in the mid-infrared. On the SPHERE high-contrast instrument currently installed at the VLT, we observe that one of the main…

MIDIR is the proposed thermal/mid-IR imager and spectrograph for the European Extremely Large Telescope (E-ELT). It will cover the wavelength range of 3 to at least 20 microns. Designed for diffraction-limited performance over the entire…

Astrophysics · Physics 2009-11-13 S. Kendrew , B. Brandl , R. Lenzen , L. Venema , H. U. Käufl , G. Finger , A. Glasse , R. Stuik

We quantify the scientific potential for exoplanet imaging with the Mid-infrared E-ELT Imager and Spectrograph (METIS) foreseen as one of the instruments of the European Extremely Large Telescope (E-ELT). We focus on two main science cases:…

Instrumentation and Methods for Astrophysics · Physics 2015-06-19 Sascha P. Quanz , Ian Crossfield , Michael R. Meyer , Eva Schmalzl , Jenny Held

Metis is the first solar coronagraph designed for a space mission capable of performing simultaneous imaging of the off-limb solar corona in both visible and UV light. The observations obtained with Metis aboard the Solar Orbiter ESA-NASA…

Solar and Stellar Astrophysics · Physics 2019-11-20 Ester Antonucci , Marco Romoli , Vincenzo Andretta , Silvano Fineschi , Petr Heinzel , J. Daniel Moses , Giampiero Naletto , Gianalfredo Nicolini , Daniele Spadaro , Luca Teriaca , Arkadiusz Berlicki , Gerardo Capobianco , Giuseppe Crescenzio , Vania Da Deppo , Mauro Focardi , Fabio Frassetto , Klaus Heerlein , Federico Landini , Enrico Magli , Andrea Marco Malvezzi , Giuseppe Massone , Radek Melich , Piergiorgio Nicolosi , Giancarlo Noci , Maurizio Pancrazzi , Maria G. Pelizzo , Luca Poletto , Clementina Sasso , Udo Schühle , Sami K. Solanki , Leonard Strachan , Roberto Susino , Giuseppe Tondello , Michela Uslenghi , Joachim Woch , Lucia Abbo , Alessandro Bemporad , Marta Casti , Sergio Dolei , Catia Grimani , Mauro Messerotti , Marco Ricci , Thomas Straus , Daniele Telloni , Paola Zuppella , Frederic Auchère , Roberto Bruno , Angela Ciaravella , Alain J. Corso , Miguel Alvarez Copano , Regina Aznar Cuadrado , Raffaella D'Amicis , Reiner Enge , Alessio Gravina , Sonja Jejčič , Philippe Lamy , Alessandro Lanzafame , Thimo Meierdierks , Ioanna Papagiannaki , Hardi Peter , German Fernandez Rico , Mewael Giday Sertsu , Jan Staub , Kanaris Tsinganos , Marco Velli , Rita Ventura , Enrico Verroi , Jean-Claude Vial , Sebastien Vives , Antonio Volpicelli , Stephan Werner , Andreas Zerr , Barbara Negri , Marco Castronuovo , Alessandro Gabrielli , Roberto Bertacin , Rita Carpentiero , Silvia Natalucci , Filippo Marliani , Marco Cesa , Philippe Laget , Danilo Morea , Stefano Pieraccini , Paolo Radaelli , Paolo Sandri , Paolo Sarra , Stefano Cesare , Felice Del Forno , Ernesto Massa , Mauro Montabone , Sergio Mottini , Daniele Quattropani , Tiziano Schillaci , Roberto Boccardo , Rosario Brando , Arianna Pandi , Cristian Baietto , Riccardo Bertone , Alberto Alvarez-Herrero , Pilar García Parejo , María Cebollero , Mauro Amoruso , Vito Centonze

We investigate the detectability of extended mid-infrared (MIR) emission associated with FU-Ori type objects (FUors) using the METIS coronagraphs on the 39-m Extremely Large Telescope (ELT). The imaging simulations were made for three…

Instrumentation and Methods for Astrophysics · Physics 2025-03-11 Michihiro Takami , Gilles Otten , Olivier Absil , Christian Delacroix , Jennifer L. Karr , Shiang-Yu Wang

The Enhanced Resolution Imager and Spectrograph (ERIS) is the new near-infrared instrument at the VLT-UT4. ERIS replaces and extends the observational capabilities formerly provided by SINFONI and NACO: integral field spectroscopy at 1 -…

The workhorse instruments of the 8-10m class observatories have become their multi-object spectrographs (MOS), providing comprehensive follow-up to both ground-based and space-borne imaging. With the advent of deeper imaging surveys from,…

The first generation of ELT instruments includes an optical-infrared high-resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion Echelle Spectrograph). ANDES consists of three fibre-fed…

Instrumentation and Methods for Astrophysics · Physics 2024-07-23 A. Marconi , M. Abreu , V. Adibekyan , V. Alberti , S. Albrecht , J. Alcaniz , M. Aliverti , C. Allende Prieto , J. D. Alvarado Gómez , C. S. Alves , P. J. Amado , M. Amate , M. I. Andersen , S. Antoniucci , E. Artigau , C. Bailet , C. Baker , V. Baldini , A. Balestra , S. A. Barnes , F. Baron , S. C. C. Barros , S. M. Bauer , M. Beaulieu , O. Bellido-Tirado , B. Benneke , T. Bensby , E. A. Bergin , P. Berio , K. Biazzo , L. Bigot , A. Bik , J. L. Birkby , N. Blind , O. Boebion , I. Boisse , E. Bolmont , J. S. Bolton , M. Bonaglia , X. Bonfils , L. Bonhomme , F. Borsa , J. -C. Bouret , A. Brandeker , W. Brandner , C. H. Broeg , M. Brogi , D. Brousseau , A. Brucalassi , J. Brynnel , L. A. Buchhave , D. F. Buscher , L. Cabona , A. Cabral , G. Calderone , R. Calvo-Ortega , F. Cantalloube , B. L. Canto Martins , L. Carbonaro , Y. Caujolle , G. Chauvin , B. Chazelas , A. -L. Cheffot , Y. S. Cheng , A. Chiavassa , L. Christensen , R. Cirami , M. Cirasuolo , N. J. Cook , R. J. Cooke , I. Coretti , S. Covino , N. Cowan , G. Cresci , S. Cristiani , V. Cunha Parro , G. Cupani , V. D'Odorico , K. Dadi , I. de Castro Leão , A. De Cia , J. R. De Medeiros , F. Debras , M. Debus , A. Delorme , O. Demangeon , F. Derie , M. Dessauges-Zavadsky , P. Di Marcantonio , S. Di Stefano , F. Dionies , A. Domiciano de Souza , R. Doyon , J. Dunn , S. Egner , D. Ehrenreich , J. P. Faria , D. Ferruzzi , C. Feruglio , M. Fisher , A. Fontana , B. S. Frank , C. Fuesslein , M. Fumagalli , T. Fusco , J. Fynbo , O. Gabella , W. Gaessler , E. Gallo , X. Gao , L. Genolet , M. Genoni , P. Giacobbe , E. Giro , R. S. Goncalves , O. A. Gonzalez , J. I. González Hernández , C. Gouvret , F. Gracia Temich , M. G. Haehnelt , C. Haniff , A. Hatzes , R. Helled , H. J. Hoeijmakers , I. Hughes , P. Huke , Y. Ivanisenko , A. S. Järvinen , S. P. Järvinen , A. Kaminski , J. Kern , J. Knoche , A. Kordt , H. Korhonen , A. J. Korn , D. Kouach , G. Kowzan , L. Kreidberg , M. Landoni , A. A. Lanotte , A. Lavail , B. Lavie , D. Lee , M. Lehmitz , J. Li , W. Li , J. Liske , C. Lovis , S. Lucatello , D. Lunney , M. J. MacIntosh , N. Madhusudhan , L. Magrini , R. Maiolino , J. Maldonado , L. Malo , A. W. S. Man , T. Marquart , C. M. J. Marques , E. L. Marques , P. Martinez , A. Martins , C. J. A. P. Martins , J. H. C. Martins , P. Maslowski , C. A. Mason , E. Mason , R. A. McCracken , M. A. F. Melo e Sousa , P. Mergo , G. Micela , D. Milaković , P. Molliere , M. A. Monteiro , D. Montgomery , C. Mordasini , J. Morin , A. Mucciarelli , M. T. Murphy , M. N'Diaye , N. Nardetto , B. Neichel , N. Neri , A. T. Niedzielski , E. Niemczura , B. Nisini , L. Nortmann , P. Noterdaeme , N. J. Nunes , L. Oggioni , F. Olchewsky , E. Oliva , H. Onel , L. Origlia , G. Ostlin , N. N. -Q. Ouellette , E. Palle , P. Papaderos , G. Pariani , L. Pasquini , J. Peñate Castro , F. Pepe , C. Peroux , L. Perreault Levasseur , S. Perruchot , P. Petit , O. Pfuhl , L. Pino , J. Piqueras , N. Piskunov , A. Pollo , K. Poppenhaeger , M. Porru , J. Puschnig , A. Quirrenbach , E. Rauscher , R. Rebolo , E. M. A. Redaelli , S. Reffert , D. T. Reid , A. Reiners , P. Richter , M. Riva , S. Rivoire , C. Rodriguez-López , I. U. Roederer , D. Romano , M. Roth , S. Rousseau , J. Rowe , A. Saccardi , S. Salvadori , N. Sanna , N. C. Santos , P. Santos Diaz , J. Sanz-Forcada , M. Sarajlic , J. -F. Sauvage , D. Savio , A Scaudo , S. Schäfer , R. P. Schiavon , T. M. Schmidt , C. Selmi , R. Simoes , A. Simonnin , S. Sivanandam , M. Sordet , R. Sordo , F. Sortino , D. Sosnowska , S. G. Sousa , A. Spang , R. Spiga , E. Stempels , J. R. Y. Stevenson , K. G. Strassmeier , A. Suárez Mascareño , A. Sulich , X. Sun , N. R. Tanvir , F. Tenegi-Sangines , S. Thibault , S. J. Thompson , P. Tisserand , A. Tozzi , M. Turbet , J. -P. Veran , P. Vallee , I. Vanni , R. Varas , A. Vega-Moreno , K. A. Venn , A. Verma , J. Vernet , M. Viel , G. Wade , C. Waring , M. Weber , J. Weder , B. Wehbe , J. Weingrill , M. Woche , M. Xompero , E. Zackrisson , A. Zanutta , M. R. Zapatero Osorio , M. Zechmeister , J. Zimara

Non-common path quasi-static and differential aberrations are one of the big hurdles of direct imaging for current and future high-contrast imaging instruments. They increase speckle and photon noise thus reducing the achievable contrast…

Instrumentation and Methods for Astrophysics · Physics 2024-07-22 Gilles Orban de Xivry , Olivier Absil , Christian Delacroix , Prashant Pathak , Maxime Quesnel , Thomas Bertram

IRIS is a near-infrared (0.84 to 2.4 microns) integral field spectrograph and wide-field imager being developed for first light with the Thirty Meter (TMT). It mounts to the advanced optics (AO) system NFIRAOS and has integrated…

Adaptive Optics at mid-IR wavelengths has long been seen as either not necessary or easy. The impact of atmospheric turbulence on the performance of 8-10 meter class telescopes in the mid-IR is relatively small compared to other performance…

Instrumentation and Methods for Astrophysics · Physics 2015-05-14 R. Stuik , L. Jolissaint , S. Kendrew , S. Hippler , B. Brandl , L. Venema
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