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Título

HARMONI: a single-field wide-band integral-field spectrograph for the European ELT

AutorThatte, Niranjan A.; Tecza, Matthias; Clarke, Fraser; Davies, Roger L.; Remillieux, Alban; Bacon, Roland M.; Lunney, David; Arribas-Mocoroa, Santiago CSIC ORCID ; Mediavilla, E.; Gago, Fernando; Bezawada, Naidu; Ferruit, P.; Fragoso, Ana; Freeman, David; Fuentes, Javier; Fusco, Thierry; Gallie, Angus M.; Garcia, Adolfo; Goodsall, Timothy; Gracia, Felix; Jarno, Aurélien; Kosmalski, Johan; Lynn, James D.; McLay, Stuart; Montgomery, David M.; Pécontal-Rousset, Arlette; Schnetler, Hermine; Smith, Harry; Sosa, Dario; Battaglia, Giuseppina; Bowles, Neil; Colina, Luis CSIC ORCID; Emsellem, Eric; Garcia-Perez, Ana; Hook, Isobel; Irwin, Patrick; Jarvis, Matt J.; Kennicutt, Robert; Levan, Andrew; Longmore, Andy; Magorrian, John; McCaughrean, Mark; Origlia, Livia; Rebolo López, Rafael CSIC ORCID; Rigopoulou, Dimitra; Ryan, Sean; Swinbank, Mark; Tanvir, Nial; Tolstoy, Eline; Verma, Aprajita CSIC
Palabras claveIntegral field
Spectrograph
Diffraction-limited
Near-infrared
Image slicer
Cryogenics
ELT
Fecha de publicación2010
EditorSociety of Photo-Optical Instrumentation Engineers
CitaciónGround-based and Airborne Instrumentation for Astronomy III 7735: 77352I (2010)
ResumenWe describe the results of a Phase A study for a single field, wide band, near-infrared integral field spectrograph for the European Extremely Large Telescope (E-ELT). HARMONI, the High Angular Resolution Monolithic Optical & Nearinfrared Integral field spectrograph, provides the E-ELT’s core spectroscopic requirement. It is a work-horse instrument, with four different spatial scales, ranging from seeing to diffraction-limited, and spectral resolving powers of 4000, 10000 & 20000 covering the 0.47 to 2.45 μm wavelength range. It is optimally suited to carry out a wide range of observing programs, focusing on detailed, spatially resolved studies of extended objects to unravel their morphology, kinematics and chemical composition, whilst also enabling ultra-sensitive observations of point sources. We present a synopsis of the key science cases motivating the instrument, the top level specifications, a description of the opto-mechanical concept, operation and calibration plan, and image quality and throughput budgets. Issues of expected performance, complementarity and synergies, as well as simulated observations are presented elsewhere in these proceedings
DescripciónTrabajo presentado en SPIE Astronomical Telescopes, celebrado en San Diego (California), del 15 de junio al 2 de julio de 2010
Versión del editorhttp://dx.doi.org/10.1117/12.857445
URIhttp://hdl.handle.net/10261/200555
DOI10.1117/12.857445
ISBN0277-786X
E-ISSN1996-756X
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