Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-25T17:40:00.611Z Has data issue: false hasContentIssue false
  • English
  • Français

PILOT – the Pathfinder for an International Large Optical Telescope

Published online by Cambridge University Press:  23 May 2007

N. Epchtein ,
M. Candidi ,
J.W.V. Storey ,
M.C.B. Ashley ,
M.G. Burton  and
J.S. Lawrence
J.W.V. Storey*
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
M.C.B. Ashley
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
M.G. Burton
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
J.S. Lawrence
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
*
[email protected]
Get access

Abstract

PILOT is proposed as a partnership between Australia and Europe todevelop a 2.4 m optical/infrared telescope for Dome C,Antarctica. Funding for a detailed designed study is being soughtfrom Australian sources, with a view to commencing construction inearly 2008. The current “strawman” design is for an f/10 dualNasmyth configuration with provision for both a silicon carbide fasttip-tilt secondary mirror for the thermal infrared, and an adaptivesecondary mirror to achieve diffraction-limited imaging atwavelengths as short as V-band.


Type
Research Article
Information
European Astronomical Society Publications Series , Volume 25: 1st ARENA Conference on "Large Astronomical Infrastructures at CONCORDIA, prospects and constraints for Antarctic Optical/IR Astronomy" , 2007 , pp. 255 - 259
Copyright
© EAS, EDP Sciences, 2007

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)