Paper
28 September 2004 A wide-field telescope for MACHO searching at Dome C
Author Affiliations +
Abstract
Wide-Field imaging at visible wavelengths with seeing of the order of 0.1-0.2arcsec is believed to be possible from the high Antarctic plateau site of Dome-C by the removal of ground layer effects only. We present a proposal for a 2m-class telescope specifically designed for the science case of short duration (~10s or greater) microlensing events in the crowded central regions of Galactic Globular Clusters and nearby galaxies where the achievement of a spatial resolution of the order of a fraction of arcsec is essential. The philosophy behind the telescope proposal is discussed in detail. It is emphasized that this is a project with a specific unique science goal in mind and not a large scale facility instrument. A preliminary design for the optics, ground layer removal using a deformable secondary and "static" wavefront sensor and telescope structure is presented. In particular, it is shown that substantial simplification in the design can be achieved by having a specific science goal in mind, so reducing the complexity and increasing reliability. Transport and logistics for the successful deployment and operation of the telescope at the Dome-C site are discussed.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Roberto Ragazzoni, Giuseppe Bono, Piero Salinari, Carmelo Arcidiacono, Maurizio Busso, Emiliano Diolaiti, Jacopo Farinato, Anna Moore, Armando Riccardi, Marco Roncatelli, Giorgio Sartori, Roberto Soci, Gino Tosti, and Elise Vernet "A wide-field telescope for MACHO searching at Dome C", Proc. SPIE 5489, Ground-based Telescopes, (28 September 2004); https://doi.org/10.1117/12.552057
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Mirrors

Turbulence

Adaptive optics

Wavefront sensors

Optical instrument design

Stars

RELATED CONTENT

First light of the LINC-NIRVANA Pathfinder experiment
Proceedings of SPIE (July 21 2014)
Preparing for the phase B of the E ELT MCAO...
Proceedings of SPIE (August 07 2014)
Optical Design Of The Hipparcos Telescope
Proceedings of SPIE (October 31 1986)
EAGLE an MOAO fed multi IFU working in the...
Proceedings of SPIE (September 17 2009)

Back to Top