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Three-reflections telescope proposalas flat-field anastigmat for wide field observations at Dome C

Published online by Cambridge University Press:  05 January 2006

M. Ferrari
Affiliation:
Observatoire Astronomique de Marseille Provence, LAM - 2, place Leverrier, 13248 Marseille Cedex 4, France
G. Lemaître
Affiliation:
Observatoire Astronomique de Marseille Provence, LAM - 2, place Leverrier, 13248 Marseille Cedex 4, France
R. Viotti
Affiliation:
Istituto di Astrofisica Spaziale e Fisica Cosmica, via Fosso del Cavaliere 100, 00133 Roma, Italy
C. La Padula
Affiliation:
Istituto di Astrofisica Spaziale e Fisica Cosmica, via Fosso del Cavaliere 100, 00133 Roma, Italy
G. Comte
Affiliation:
Observatoire Astronomique de Marseille Provence, LAM - 2, place Leverrier, 13248 Marseille Cedex 4, France
M. Blanc
Affiliation:
Observatoire Astronomique de Marseille Provence, LAM - 2, place Leverrier, 13248 Marseille Cedex 4, France
M. Boer
Affiliation:
Observatoire Astronomique de Marseille Provence, OHP, 04870 St. Michel l'Observatoire, France
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Abstract

It is now evident that the exceptional seeing at Dome C willallow, in the next years, to pursue astronomical programs withconditions better than at any other observatory in the world, andvery close to space experiments.Considering a new type of wide-field telescope, particularastronomical programs could be well optimized for observations atDome C such as surveys for the discovery and follow up ofnear-Earth asteroids, search for extra-solar planets using transitor micro-lensing events, and stellar luminosity variations.We propose to build a 1.5–2 m class three-reflections telescope, with1–1.5 degree FOV, four times shorter than an equivalent Schmidttelescope, and providing a flat field without requiring atriplet- or quadruplet-lens corrector since its design isanastigmatic.We present the preliminary optical tests of such designs:MINITRUST 1 and 2 are two 45 cm identical prototypes based inFrance and Italy, and manufactured using active optics techniques.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2005

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