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Integral field spectrographs are an important technology for exoplanet imaging, due to their ability to take spectra in a high-contrast environment, and improve planet detection sensitivity through spectral differential imaging. ALES is the…

The integral field spectrograph configuration of the LMIRCam science camera within the Large Binocular Telescope Interferometer (LBTI) facilitates 2 to 5 $\mu$m spectroscopy of directly imaged gas-giant exoplanets. The mode, dubbed ALES,…

Instrumentation and Methods for Astrophysics · Physics 2018-08-09 Jordan M. Stone , Andrew J. Skemer , Philip Hinz , Zack Briesemeister , Travis Barman , Charles E. Woodward , Mike Skrutskie , Jarron Leisenring

We present the data reduction pipeline, MEAD, for Arizona Lenslets for Exoplanet Spectroscopy (ALES), the first thermal infrared integral field spectrograph designed for high-contrast imaging. ALES is an upgrade of LMIRCam, the $1-5\,\mu$m…

SCALES (Slicer Combined with an Array of Lenslets for Exoplanet Spectroscopy) is a 2 to 5 micron high-contrast lenslet-based Integral Field Spectrograph (IFS) designed to characterize exoplanets and their atmospheres. Like other…

Instrumentation and Methods for Astrophysics · Physics 2022-08-25 Deno Stelter , Andrew J. Skemer , Renate Kupke , Cyril Bourgenot , Raquel A. Martinez , Stephanie E. Sallum

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 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

SCALES (Santa Cruz Array of Lenslets for Exoplanet Spectroscopy) is a 2-5 micron high-contrast lenslet integral-field spectrograph (IFS) driven by exoplanet characterization science requirements and will operate at W. M. Keck Observatory.…

The next generation ground-based extremely large telescopes (ELTs) present incredible opportunities to discover and characterize diverse planetary systems, even potentially habitable worlds. Adaptive-optics assisted thermal-IR (3-14 micron)…

METIS will be among the first generation of scientific instruments on the E-ELT. Focusing on highest angular resolution and high spectral resolution, METIS will provide diffraction limited imaging and coronagraphy from 3-14um over an…

SCALES (Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy) is a 2 - 5 micron high-contrast lenslet-based integral field spectrograph (IFS) designed to characterize exoplanets and their atmospheres. The SCALES…

The Large Binocular Telescope Interferometer (LBTI) is a strategic instrument of the LBT designed for high-sensitivity, high-contrast, and high-resolution infrared (1.5-13 $\mu$m) imaging of nearby planetary systems. To carry out a wide…

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 ISS (Integral-field Spectrograph System) has been designed as part of the EAGLE Phase A Instrument Study for the E-ELT. It consists of two input channels of 1.65x1.65 arcsec field-of-view, each reconfigured spatially by an image-slicing…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 P. R. Hastings , B. Stobie , S. Vives , P. Vola , M. Wells , C. J. Evans

The Large Binocular Telescope Interferometer is a NASA-funded nulling and imaging instrument designed to coherently combine the two 8.4-m primary mirrors of the LBT for high-sensitivity, high-contrast, and high-resolution infrared imaging…

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…

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…

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…

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