Bibcode
Thatte, Niranjan A.; Tecza, Mathias; Freeman, David; Gallie, Angus M.; Montgomery, David; Clarke, Fraser; Fragoso-López, A. B.; Fuentes, F. J.; Gago, F.; Garcia, Adolfo; Gracia, F.; Kosmalski, Johan; Lynn, James; Sosa, D.; Arribas, Santiago; Bacon, Roland; Davies, Roger L.; Fusco, Thierry; Lunney, David; Mediavilla, E.; Remillieux, Alban; Schnetler, Hermine
Referencia bibliográfica
Ground-based and Airborne Instrumentation for Astronomy IV. Proceedings of the SPIE, Volume 8446, id. 84461L-84461L-10 (2012).
Fecha de publicación:
9
2012
Número de citas
7
Número de citas referidas
0
Descripción
HARMONI is a visible and near-IR integral field spectrograph, providing
the E-ELT's spectroscopic capability at first light. It obtains
simultaneous spectra of 32000 spaxels, at a range of resolving powers
from R~4000 to R~20000, covering the wavelength range from 0.47 to 2.45
μm. The 256 × 128 spaxel field of view has four different plate
scales, with the coarsest scale (40 mas) providing a 5″ ×
10″ FoV, while the finest scale is a factor of 10 finer (4mas). We
describe the opto-mechanical design of HARMONI, prior to the start of
preliminary design, including the main subsystems - namely the image
de-rotator, the scale-changing optics, the splitting and slicing optics,
and the spectrographs. We also present the secondary guiding system, the
pupil imaging optics, the field and pupil stops, the natural guide star
wavefront sensor, and the calibration unit.