Paper
15 July 2010 HARMONI: a single-field wide-band integral-field spectrograph for the European ELT
Niranjan Thatte, Mathias Tecza, Fraser Clarke, Roger L. Davies, Alban Remillieux, Roland Bacon, David Lunney, Santiago Arribas, Evencio Mediavilla, Fernando Gago, Naidu Bezawada, Pierre Ferruit, Ana Fragoso, David Freeman, Javier Fuentes, Thierry Fusco, Angus Gallie, Adolfo Garcia, Timothy Goodsall, Felix Gracia, Aurelien Jarno, Johan Kosmalski, James Lynn, Stuart McLay, David Montgomery, Arlette Pecontal, Hermine Schnetler, Harry Smith, Dario Sosa, Giuseppina Battaglia, Neil Bowles, Luis Colina, Eric Emsellem, Ana Garcia-Perez, Szymon Gladysz, Isobel Hook, Patrick Irwin, Matt Jarvis, Robert Kennicutt, Andrew Levan, Andy Longmore, John Magorrian, Mark McCaughrean, Livia Origlia, Rafael Rebolo, Dimitra Rigopoulou, Sean Ryan, Mark Swinbank, Nial Tanvir, Eline Tolstoy, Aprajita Verma
Author Affiliations +
Abstract
We 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[1].
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Niranjan Thatte, Mathias Tecza, Fraser Clarke, Roger L. Davies, Alban Remillieux, Roland Bacon, David Lunney, Santiago Arribas, Evencio Mediavilla, Fernando Gago, Naidu Bezawada, Pierre Ferruit, Ana Fragoso, David Freeman, Javier Fuentes, Thierry Fusco, Angus Gallie, Adolfo Garcia, Timothy Goodsall, Felix Gracia, Aurelien Jarno, Johan Kosmalski, James Lynn, Stuart McLay, David Montgomery, Arlette Pecontal, Hermine Schnetler, Harry Smith, Dario Sosa, Giuseppina Battaglia, Neil Bowles, Luis Colina, Eric Emsellem, Ana Garcia-Perez, Szymon Gladysz, Isobel Hook, Patrick Irwin, Matt Jarvis, Robert Kennicutt, Andrew Levan, Andy Longmore, John Magorrian, Mark McCaughrean, Livia Origlia, Rafael Rebolo, Dimitra Rigopoulou, Sean Ryan, Mark Swinbank, Nial Tanvir, Eline Tolstoy, and Aprajita Verma "HARMONI: a single-field wide-band integral-field spectrograph for the European ELT", Proc. SPIE 7735, Ground-based and Airborne Instrumentation for Astronomy III, 77352I (15 July 2010); https://doi.org/10.1117/12.857445
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Cited by 13 scholarly publications.
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KEYWORDS
Spectrographs

Sensors

Galactic astronomy

Telescopes

Calibration

Stars

Visible radiation

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