| Issue |
EAS Publications Series
Volume 40, 2010
3rd ARENA Conference: An Astronomical Observatory at CONCORDIA (Dome C, Antarctica)
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|---|---|---|
| Page(s) | 183 - 186 | |
| DOI | https://doi.org/10.1051/eas/1040025 | |
| Published online | 23 December 2009 | |
L. Spinoglio and N. Epchtein (eds)
EAS Publications Series, 40 (2010) 183-186
Infrared instruments for a 2.5 m telescope at Dome C
1
Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Madrid, Spain
2
Laboratorio de Astrofísica Estelar y Exoplanetas, CAB-INTA, Madrid, Spain
3
FRACTAL SLNE, Las Rozas de Madrid, Spain
4
Departamento de Física Teórica y del Cosmos, Universidad de Granada, Spain
5
Istituto di Astrofisica Spaziale e Fisica Cosmica, Roma, Italy
We have carried out a conceptual design study for a near-infrared (NIR) wide-field camera and a mid-infrared (MIR) camera-spectrograph for a 2.5 m telescope at Dome C. The main scientific drivers are the characterisation of young embedded objects, the evolution of crystalline silicates in circumstellar disks and the observation of exoplanet secondary transits. Both instrument exploit the unique features of Dome C: improved infrared transmission, reduced sky background, superb seeing, low temperature, and increased atmospheric stability. The NIR camera covers the wavelength range 0.8–5.5 μm and is optimized for the Kdark and L bands. The MIR instrument is sensitive in the range 7–40 μm with a possible extension to the sub-mm. It is optimized for the Q window, including the Q+ extended portion (25–40 μm) only observable from the Antarctic Plateau.
© EAS, EDP Sciences, 2010