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Related papers: HIRES, the high-resolution spectrograph for the EL…

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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

HIRES, a high resolution spectrometer, is one of the first five instruments foreseen in the ESO roadmap for the E-ELT. This spectrograph should ideally provide full spectral coverage from the UV limit to 2.5 microns, with a resolving power…

Instrumentation and Methods for Astrophysics · Physics 2015-06-22 N. Sanna , E. Oliva , F. Massi , G. Cresci , L. Origlia

We proposed that the European ELT will be equipped with an ultra-high-precision polarimetric light feed as part of its high resolution optical and near-IR spectrograph HIRES. Such a feed is unique among the new ELTs and only possible in a…

Instrumentation and Methods for Astrophysics · Physics 2019-04-11 Klaus G. Strassmeier

A major endeavor of this decade is the direct characterization of young giant exoplanets at high spectral resolution to determine the composition of their atmosphere and infer their formation processes and evolution. Such a goal represents…

New generation exoplanet imagers on large ground-based telescopes are highly optimised for the detection of young giant exoplanets in the near-infrared, but they are intrinsically limited for their characterisation by the low spectral…

Exoplanet science is booming. In 20 years our knowledge has expanded considerably, from the first discovery of a Hot Jupiter, to the detection of a large population of Neptunes and super-Earths, to the first steps toward the…

Atmospheric composition provides essential markers of the most fundamental properties of giant exoplanets, such as their formation mechanism or internal structure. New-generation exoplanet imagers, like VLT/SPHERE or Gemini/GPI, have been…

Instrumentation and Methods for Astrophysics · Physics 2018-06-29 A. Vigan , G. P. P. L. Otten , E. Muslimov , K. Dohlen , M. W. Phillips , U. Seemann , J. -L. Beuzit , R. Dorn , M. Kasper , D. Mouillet , I. Baraffe , A. Reiners

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 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, 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…

Building on the experience of the high-resolution community with the suite of VLT high-resolution spectrographs, which has been tremendously successful, we outline here the (science) case for a high-fidelity, high-resolution spectrograph…

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…

In 2006 ESO Council authorized a Phase B study of a European AO-telescope with a 42 m segmented primary with a 5-mirror design, the E-ELT. Several reports and working groups have already presented science cases for an E-ELT, specifically…

Astrophysics of Galaxies · Physics 2015-05-18 Nils Ryde

IRIS (InfraRed Imaging Spectrograph) is a first light near-infrared diffraction limited imager and integral field spectrograph being designed for the future Thirty Meter Telescope (TMT). IRIS is optimized to perform astronomical studies…

We present the science drivers for the Far-Infrared Enhanced Survey Spectrometer (FIRESS), one of two science instrument on the PRobe Infrared Mission for Astrophysics (PRIMA). FIRESS is designed to meet science objectives in the areas of…

The Infra-Red Imaging Spectrograph (IRIS) is one of the three first light instruments for the Thirty Meter Telescope (TMT) and is the only one to directly sample the diffraction limit. The instrument consists of a parallel imager and…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 Anna M. Moore , Brian J. Bauman , Elizabeth J. Barton , David Crampton , Alex Delacroix , James E. Larkin , Luc Simard , Ryuji Suzuki , Shelley A. Wright

The HERMES high-resolution spectrograph project aims at exploiting the specific potential of small but flexible telescopes in observational astrophysics. The optimised optical design of the spectrograph is based on the well-proven concept…

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