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Proceedings Paper

The GIANO-TNG spectrometer
Author(s): E. Oliva; L. Origlia; C. Baffa; C. Biliotti; P. Bruno; F. D'Amato; C. Del Vecchio; G. Falcini; S. Gennari; F. Ghinassi; E. Giani; M. Gonzalez; F. Leone; M. Lolli; M. Lodi; R. Maiolino; F. Mannucci; G. Marcucci; I. Mochi; P. Montegriffo; E. Rossetti; S. Scuderi; M. Sozzi
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Paper Abstract

GIANO is an infrared (0.9-2.5 μm cross-dispersed echelle spectrometer designed to achieve high resolution, high throughput, wide band coverage and very high stability for accurate radial velocity measurements. It also includes polarimetric capabilities and a low resolution mode with RS ~ 400 and complete 0.75-2.5 μm coverage. This makes it a very versatile, common user instrument which will be permanently mounted and available on the Nasmyth-B foci of the Telescopio Nazionale Galileo (TNG) located at Roque de Los Muchachos Observatory (ORM), La Palma, Spain. The project is fast-track and relies on well known, relatively standard technologies. It has been recognized as one of the top priority instrumental projects of INAF (the Italian National Institute of Astronomy) and received its first financing for the phase-A study in October 2003. Integration in the laboratory is planned to start before the end of 2006, commissioning at the telescope is foreseen within 2007 and scientific operations in 2008. One of the most important scientific goals is the search for rocky planets with habitable conditions around low-mass stars. If completed on time, GIANO will be the first and only IR instrument operating worldwide providing the combination of efficiency, spectral resolution, wavelength coverage and stability necessary for this type of research. With its unique combination of high and low resolution modes, GIANO will also be a very flexible common-user instrument ideal e.g. for quantitative spectroscopy of brown dwarfs, stars and stellar clusters as well as for the determination of the spectral energy distribution of faint/red objects such as high redshift galaxies. The expected limiting magnitudes are such that GIANO will be able to deliver good quality HR spectra of any 2MASS object and LR spectra of any object detected in the UKIDSS large area survey.

Paper Details

Date Published: 28 June 2006
PDF: 10 pages
Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 626919 (28 June 2006); doi: 10.1117/12.670006
Show Author Affiliations
E. Oliva, INAF, Osservatorio di Arcetri (Italy)
Telescopio Nazionale Galileo (Spain)
L. Origlia, INAF, Osservatorio di Bologna (Italy)
C. Baffa, INAF, Osservatorio di Arcetri (Italy)
C. Biliotti, INAF, Osservatorio di Arcetri (Italy)
P. Bruno, INAF, Osservatorio di Catania (Italy)
F. D'Amato, CNR, Istituto Nazionale di Ottica Applicata (Italy)
C. Del Vecchio, INAF, Osservatorio di Arcetri (Italy)
G. Falcini, INAF, Osservatorio di Arcetri (Italy)
S. Gennari, INAF, Osservatorio di Arcetri (Italy)
F. Ghinassi, Telescopio Nazionale Galileo (Spain)
E. Giani, INAF, Osservatorio di Arcetri (Italy)
M. Gonzalez, Telescopio Nazionale Galileo (Spain)
F. Leone, INAF, Osservatorio di Catania (Italy)
M. Lolli, INAF, Osservatorio di Bologna (Italy)
M. Lodi, Telescopio Nazionale Galileo (Spain)
R. Maiolino, INAF, Osservatorio di Arcetri (Italy)
F. Mannucci, INAF, Osservatorio di Arcetri (Italy)
G. Marcucci, Univ. di Firenze (Italy)
I. Mochi, INAF, Osservatorio di Arcetri (Italy)
P. Montegriffo, INAF, Osservatorio di Bologna (Italy)
E. Rossetti, INAF, Osservatorio di Bologna (Italy)
S. Scuderi, INAF, Osservatorio di Catania (Italy)
M. Sozzi, INAF, Istituto di Radioastronomia (Italy)


Published in SPIE Proceedings Vol. 6269:
Ground-based and Airborne Instrumentation for Astronomy
Ian S. McLean; Masanori Iye, Editor(s)

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