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Related papers: MOONS: The New Multi-Object Spectrograph for the V…

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VLTi Spectro-Imager (VSI) is a proposition for a second generation VLTI instrument which is aimed at providing the ESO community with the capability of performing image synthesis at milli-arcsecond angular resolution. VSI provides the VLTI…

Context:Optical interferometry is at a key development stage. ESO's VLTI has established a stable, robust infrastructure for long-baseline interferometry for general astronomical observers. The present second-generation instruments offer a…

Instrumentation and Methods for Astrophysics · Physics 2022-03-30 B. Lopez , S. Lagarde , R. G. Petrov , W. Jaffe , P. Antonelli , F. Allouche , P. Berio , A. Matter , A. Meilland , F. Millour , S. Robbe-Dubois , Th. Henning , G. Weigelt , A. Glindemann , T. Agocs , Ch. Bailet , U. Beckmann , F. Bettonvil , R. van Boekel , P. Bourget , Y. Bresson , P. Bristow , P. Cruzalèbes , E. Eldswijk , Y. Fanteï Caujolle , J. C. González Herrera , U. Graser , P. Guajardo , M. Heininger , K. -H. Hofmann , G. Kroes , W. Laun , M. Lehmitz , C. Leinert , K. Meisenheimer , S. Morel , U. Neumann , C. Paladini , I. Percheron , M. Riquelme , M. Schoeller , Ph. Stee , L. Venema , J. Woillez , G. Zins , P. Ábrahám , S. Abadie , R. Abuter , M. Accardo , T. Adler , J. Alonso , J. -C. Augereau , A. Böhm , G. Bazin , J. Beltran , A. Bensberg , W. Boland , R. Brast , L. Burtscher , R. Castillo , A. Chelli , C. Cid , J. -M. Clausse , C. Connot , R. D. Conzelmann , W. -C. Danchi , M. Delbo , J. Drevon , C. Dominik , A. van Duin , M. Ebert , F. Eisenhauer , S. Flament , R. Frahm , V. Gámez Rosas , A. Gabasch , A. Gallenne , E. Garces , P. Girard , A. Glazenborg , F. Y. J. Gonté , F. Guitton , M. de Haan , H. Hanenburg , X. Haubois , V. Hocdé , M. Hogerheijde , R. ter Horst , J. Hron , C. A. Hummel , N. Hubin , R. Huerta , J. Idserda , J. W. Isbell , D. Ives , G. Jakob , A. Jaskó , L. Jochum , L. Klarmann , R. Klein , J. Kragt , S. Kuindersma , E. Kokoulina , L. Labadie , S. Lacour , J. Leftley , R. Le Poole , J. -L. Lizon , M. Lopez , A. Mérand , A. Marcotto , N. Mauclert , T. Maurer , L. H. Mehrgan , J. Meisner , K. Meixner , M. Mellein , J. L. Menut , L. Mohr , L. Mosoni , R. Navarro , E. Nussbaum , L. Pallanca , E. Pantin , L. Pasquini , T. Phan Duc , J. -U. Pott , E. Pozna , A. Richichi , A. Ridinger , F. Rigal , Th. Rivinius , R. Roelfsema , R. -R. Rohloff , S. Rousseau , D. Salabert , D. Schertl , N. Schuhler , M. Schuil , K. Shabun , A. Soulain , C. Stephan , P. Toledo , K. Tristram , N. Tromp , F. Vakili , J. Varga , J. Vinther , L. B. F. M. Waters , M. Wittkowski , S. Wolf , F. Wrhel , G. Yoffe

The next generation of Extremely Large Telescopes (ELT), with diameters up to 39 meters, will start opera- tion in the next decade and promises new challenges in the development of instruments. The growing field of astrophotonics (the use…

Instrumentation and Methods for Astrophysics · Physics 2014-08-07 N. Blind , E. Le Coarer , P. Kern , J. Bland-Hawthorn

MUSE, a 2nd generation VLT instrument, will become the world's largest integral field spectrograph. It will be an AO assisted instrument which, in a single exposure, covers the wavelength range from 465 to 930 nm with an average resolution…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Peter M. Weilbacher , Joris Gerssen , Martin M. Roth , Petra Boehm , Arlette Pecontal-Rousset

4MOST (4m Multi Object Spectroscopic Telescope) is a spectroscopic facility that will be installed on ESO's VISTA around 2020. The science rationale of this facility are to be found in the ASTRONET Science Vision for European Astronomy (de…

Instrumentation and Methods for Astrophysics · Physics 2015-06-22 Eric Depagne , the 4MOST consortium

As telescope apertures increase, the challenge of scaling spectrographic astronomical instruments becomes acute. The next generation of extremely large telescopes (ELTs) strain the availability of glass blanks for optics and engineering to…

Instrumentation and Methods for Astrophysics · Physics 2014-08-21 Gary J. Hill

ESPRESSO is the new high-resolution spectrograph of ESO's Very-Large Telescope (VLT). It was designed for ultra-high radial-velocity precision and extreme spectral fidelity with the aim of performing exoplanet research and fundamental…

We describe updated scientific goals for the wide-field, millimeter-wave survey that will be produced by the Simons Observatory (SO). Significant upgrades to the 6-meter SO Large Aperture Telescope (LAT) are expected to be complete by 2028,…

Instrumentation and Methods for Astrophysics · Physics 2025-08-11 The Simons Observatory Collaboration , M. Abitbol , I. Abril-Cabezas , S. Adachi , P. Ade , A. E. Adler , P. Agrawal , J. Aguirre , Z. Ahmed , S. Aiola , T. Alford , A. Ali , D. Alonso , M. A. Alvarez , R. An , K. Arnold , P. Ashton , Z. Atkins , J. Austermann , S. Azzoni , C. Baccigalupi , A. Baleato Lizancos , D. Barron , P. Barry , J. Bartlett , N. Battaglia , R. Battye , E. Baxter , A. Bazarko , J. A. Beall , R. Bean , D. Beck , S. Beckman , J. Begin , A. Beheshti , B. Beringue , T. Bhandarkar , S. Bhimani , F. Bianchini , E. Biermann , S. Biquard , B. Bixler , S. Boada , D. Boettger , B. Bolliet , J. R. Bond , J. Borrill , J. Borrow , C. Braithwaite , T. L. R. Brien , M. L. Brown , S. M. Bruno , S. Bryan , R. Bustos , H. Cai , E. Calabrese , V. Calafut , F. M. Carl , A. Carones , J. Carron , A. Challinor , P. Chanial , N. Chen , K. Cheung , B. Chiang , Y. Chinone , J. Chluba , H. S. Cho , S. K. Choi , M. Chu , J. Clancy , S. E. Clark , P. Clarke , J. Cleary , D. L. Clements , J. Connors , C. Contaldi , G. Coppi , L. Corbett , N. F. Cothard , W. Coulton , K. D. Crowley , K. T. Crowley , A. Cukierman , J. M. D'Ewart , K. Dachlythra , R. Datta , S. Day-Weiss , T. de Haan , M. Devlin , L. Di Mascolo , S. Dicker , B. Dober , C. Doux , P. Dow , S. Doyle , C. J. Duell , S. M. Duff , A. J. Duivenvoorden , J. Dunkley , D. Dutcher , R. Dünner , M. Edenton , H. El Bouhargani , J. Errard , G. Fabbian , V. Fanfani , G. S. Farren , J. Fergusson , S. Ferraro , R. Flauger , A. Foster , K. Freese , J. C. Frisch , A. Frolov , G. Fuller , N. Galitzki , P. A. Gallardo , J. T. Galvez Ghersi , K. Ganga , J. Gao , X. Garrido , E. Gawiser , M. Gerbino , R. Gerras , S. Giardiello , A. Gill , V. Gilles , U. Giri , E. Gleave , V. Gluscevic , N. Goeckner-Wald , J. E. Golec , S. Gordon , M. Gralla , S. Gratton , D. Green , J. C. Groh , C. Groppi , Y. Guan , N. Gupta , J. E. Guðmundsson , S. Hagstotz , P. Hargrave , S. Haridas , K. Harrington , I. Harrison , M. Hasegawa , M. Hasselfield , V. Haynes , M. Hazumi , A. He , E. Healy , S. W. Henderson , B. S. Hensley , E. Hertig , C. Hervías-Caimapo , M. Higuchi , C. A. Hill , J. C. Hill , G. Hilton , M. Hilton , A. D. Hincks , G. Hinshaw , R. Hložek , A. Y. Q. Ho , S. Ho , S. P. Ho , T. D. Hoang , J. Hoh , E. Hornecker , A. L. Hornsby , S. C. Hotinli , Z. Huang , Z. B. Huber , J. Hubmayr , K. Huffenberger , J. P. Hughes , A. Idicherian Lonappan , M. Ikape , K. Irwin , J. Iuliano , A. H. Jaffe , B. Jain , H. T. Jense , O. Jeong , A. Johnson , B. R. Johnson , M. Johnson , M. Jones , B. Jost , D. Kaneko , E. D. Karpel , Y. Kasai , N. Katayama , B. Keating , B. Keller , R. Keskitalo , J. Kim , T. Kisner , K. Kiuchi , J. Klein , K. Knowles , A. M. Kofman , B. J. Koopman , A. Kosowsky , R. Kou , N. Krachmalnicoff , D. Kramer , A. Krishak , A. Krolewski , A. Kusaka , A. Kusiak , P. La Plante , A. La Posta , A. Laguë , J. Lashner , M. Lattanzi , A. Lee , E. Lee , J. Leech , C. Lessler , J. S. Leung , A. Lewis , Y. Li , Z. Li , M. Limon , L. Lin , M. Link , J. Liu , Y. Liu , J. Lonergan , T. Louis , T. Lucas , M. Ludlam , M. Lungu , M. Lyons , N. MacCrann , A. MacInnis , M. Madhavacheril , D. Mak , F. Maldonado , M. Mallaby-Kay , A. Manduca , A. Mangu , H. Mani , A. S. Maniyar , G. A. Marques , J. Mates , T. Matsumura , P. Mauskopf , A. May , N. McCallum , H. McCarrick , F. McCarthy , M. McCulloch , J. McMahon , P. D. Meerburg , Y. Mehta , J. Melin , J. Meyers , A. Middleton , A. Miller , M. Mirmelstein , K. Moodley , J. Moore , M. Morshed , T. Morton , E. Moser , T. Mroczkowski , M. Murata , M. Münchmeyer , S. Naess , H. Nakata , T. Namikawa , M. Nashimoto , F. Nati , P. Natoli , M. Negrello , S. K. Nerval , L. Newburgh , D. V. Nguyen , A. Nicola , M. D. Niemack , H. Nishino , Y. Nishinomiya , A. Orlando , J. Orlowski-Scherer , L. Pagano , L. A. Page , S. Pandey , A. Papageorgiou , I. Paraskevakos , B. Partridge , R. Patki , M. Peel , K. Perez Sarmiento , F. Perrotta , P. Phakathi , L. Piccirillo , E. Pierpaoli , T. Pinsonneault-Marotte , G. Pisano , D. Poletti , R. Puddu , G. Puglisi , F. J. Qu , M. J. Randall , C. Ranucci , C. Raum , R. Reeves , C. L. Reichardt , M. Remazeilles , Y. Rephaeli , D. Riechers , J. Robe , M. F. Robertson , N. Robertson , K. Rogers , F. Rojas , A. Romero , E. Rosenberg , A. Rotti , S. Rowe , A. Roy , S. Sadeh , N. Sailer , K. Sakaguri , T. Sakuma , Y. Sakurai , M. Salatino , G. H. Sanders , D. Sasaki , M. Sathyanarayana Rao , T. P. Satterthwaite , L. Saunders , L. Scalcinati , E. Schaan , B. Schmitt , M. Schmittfull , N. Sehgal , J. Seibert , Y. Seino , U. Seljak , S. Shaikh , E. Shaw , P. Shellard , B. Sherwin , M. Shimon , J. E. Shroyer , C. Sierra , J. Sievers , C. Sifón , P. Sikhosana , M. Silva-Feaver , S. M. Simon , A. Sinclair , K. Smith , W. Sohn , X. Song , R. F. Sonka , D. Spergel , J. Spisak , S. T. Staggs , G. Stein , J. R. Stevens , R. Stompor , E. Storer , R. Sudiwala , J. Sugiyama , K. M. Surrao , S. Sutariya , A. Suzuki , J. Suzuki , O. Tajima , S. Takakura , A. Takeuchi , I. Tansieri , A. C. Taylor , G. Teply , T. Terasaki , A. Thomas , D. B. Thomas , R. Thornton , H. Trac , T. Tsan , E. Tsang King Sang , C. Tucker , J. Ullom , L. Vacher , L. Vale , A. van Engelen , J. Van Lanen , J. van Marrewijk , D. D. Van Winkle , C. Vargas , E. M. Vavagiakis , I. Veenendaal , C. Vergès , M. Vissers , M. Viña , K. Wagoner , S. Walker , L. Walters , Y. Wang , B. Westbrook , J. Williams , P. Williams , H. Winch , E. J. Wollack , K. Wolz , J. Wong , Z. Xu , K. Yamada , E. Young , B. Yu , C. Yu , M. Zannoni , K. Zheng , N. Zhu , A. Zonca , I. Zubeldia

We discuss a cryogenic, multi-object near-infrared spectrometer as a second generation instrument for the VLT. The spectrometer combines 20 to 40 independent integral eld units (IFUs), which can be positioned by a cryogenic robot over the…

Astrophysics · Physics 2009-11-07 R. Genzel , R. Hofmann , D. Tomono , N. Thatte , F. Eisenhauer , M. Lehnert , M. Tecza , R. Bender

Since 2005 ESO has been working with its community and industry to develop an extremely large optical/infrared telescope. ESO's Extremely Large Telescope, or ELT for short, is a revolutionary ground-based telescope that will have a 39-metre…

Instrumentation and Methods for Astrophysics · Physics 2023-03-01 Paolo Padovani , Michele Cirasuolo , Remco van der Burg , Faustine Cantalloube , Elizabeth George , Markus Kasper , Kieran Leschinski , Carlos Martins , Julien Milli , Sabine Möhler , Mark Neeser , Benoit Neichel , Angel Otarola , Rubén Sánchez-Janssen , Benoit Serra , Alain Smette , Elena Valenti , Christophe Verinaud , Joël Vernet , Olivier Absil , Guido Agapito , Morten Andersen , Carmelo Arcidiacono , Matej Arko , Pierre Baudoz , Olivier Beltramo-Martin , Enrico Biancalani , Thomas Bierwirth , Leonard Burtscher , Giulia Carlà , Julio A. Castro-Almazán , Anne-Laure Cheffot , Lodovico Coccato , Carlos Correia , Romain Fetick , Giuliana Fiorentino , Thierry Fusco , Begoña García-Lorenzo , Nicola Gentile Fusillo , Oscar Gonzalez , Andrea Grazian , Marco Gullieuszik , Olivier Hainaut , Valentin Ivanov , Melanie Kaasinen , Darshan Kaddad , Tomasz Kamiński , Wolfgang Kausch , Florian Kerber , Stefan Kimeswenger , Rosita Kokotanekova , Arseniy Kuznetsov , Alexis Lau , Miska Le Louarn , Frédéric Lemmel , Jochen Liske , Gaspare Lo Curto , David Lucsanyi , Lars Lundin , Stefan Noll , Sylvain Oberti , James Osborn , Elena Masciadri , Dinko Milaković , Michael T. Murphy , Fernando Pedichini , Miguel Pereira Santaella , Roberto Piazzesi , Javier Piqueras López , Cédric Plantet , Thibaut Prod'homme , Norbert Przybilla , Mathieu Puech , Derryck T. Reid , Ansgar Reiners , Rutger Rijnenberg , Myriam Rodrigues , Fabio Rossi , Laurence Routledge , Hans Smit , Mathias Tecza , Niranjan Thatte , Roy van Boekel , Aprajita Verma , Arthur Vigan

This paper is a response to a call for white papers solicited by Gemini Observatory and its Science and Technology Advisory Committee, to help define the science case and requirements for a new Gemini instrument, envisaged to consist of a…

SOXS (Son Of X-Shooter) will be a spectrograph for the ESO NTT telescope capable to cover the optical and NIR bands, based on the heritage of the X-Shooter at the ESO-VLT. SOXS will be built and run by an international consortium, carrying…

VANDELS is a deep spectroscopic survey, performed with the VIMOS instrument at VLT, aimed at studying in detail the physical properties of high-redshift galaxies. VANDELS targeted about 2100 sources at 1<z<6.5 in the CANDELS Chandra…

Transmission spectroscopy facilitates the detection of molecules and/or clouds in the atmospheres of exoplanets. Such studies rely heavily on space-based or large ground-based observatories, as one needs to perform time- resolved, high…

We describe MIFS, a second generation integral-field spectrograph for the VLT, operating in the visible wavelength range. It combines a 1'x1' field of view with the improved spatial resolution provided by multi-conjugate adaptive optics and…

Fibre Multi-Object Spectrograph (FMOS) is the first near-infrared instrument with a wide field of view capable of acquiring spectra simultaneously from up to 400 objects. It has been developed as a common-use instrument for the F/2…

Dedicated to spectroscopic and imaging observations of the ultraviolet sky, the World Space Observatory for Ultraviolet Project is a Russia led international collaboration presently involving also China, Germany, Italy, Spain and Ukraine.…

Integral-field spectroscopy is the most effective method of exploiting the superb image quality of the ESO-VLT, allowing complex astrophysical processes to be probed on the angular scales currently accessible only for imaging data, but with…

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