We are developing technologies in processing and metrology to fabricate a 1.4-meter aperture, aspherical surface Aluminium prototype mirror for Cherenkov Telescope Array. The aim is to fast process these large aperture mirrors at low cost. The technical development will ensure the high specifications on the surface quality. Different metrology methods including Swinging Arm Profilometry (SAP) and phase measuring deflectomtry (PMD) are being developed. Recent results have shown very promising progress on these developments. We have excellent record in transferring our research results into industry. These cutting-edge technologies will be transferred to our industry partner to explore further developments
The Cherenkov Telescope Array (CTA) is the next generation very high-energy gamma-ray observatory, w...
The Cherenkov Telescope Array (CTA) is the next generation very high-energy gamma-ray observatory, w...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...
Modern large telescopes such as TAO, LSST, TMT and EELT require 0.9m-4m monolithic convex secondary ...
This thesis demonstrates the possibility of manufacturing larger mirrors from nickel coated aluminiu...
The effective utilization of synchrotron radiation (SR) from high-brightness sources requires the us...
The "Large Active Mirrors in Aluminium", or L.A.M.A. project is intended as a metallic alt...
The next generation of ground-based extremely large telescopes of 30 m to 100 m aperture calls for t...
For extremely large telescopes, there is strong need for thin deformable mirrors in the 3-4 m class....
For extremely large telescopes, there is strong need for thin deformable mirrors in the 3-4 m class....
Research has been carried out on three major difficulties in designing efficient and economic telesc...
The telescopes of the Cherenkov Telescope Array (CTA) will have segmented mirrors, with mirror facet...
The telescopes of the Cherenkov Telescope Array (CTA) will have segmented mirrors, with mirror facet...
ABSTRACT A new class of telescope is being built with primary mirrors as large as 8.4 meters in diam...
The development of lightweight glass mirrors manufactured via cold-slumping technique for Imaging At...
The Cherenkov Telescope Array (CTA) is the next generation very high-energy gamma-ray observatory, w...
The Cherenkov Telescope Array (CTA) is the next generation very high-energy gamma-ray observatory, w...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...
Modern large telescopes such as TAO, LSST, TMT and EELT require 0.9m-4m monolithic convex secondary ...
This thesis demonstrates the possibility of manufacturing larger mirrors from nickel coated aluminiu...
The effective utilization of synchrotron radiation (SR) from high-brightness sources requires the us...
The "Large Active Mirrors in Aluminium", or L.A.M.A. project is intended as a metallic alt...
The next generation of ground-based extremely large telescopes of 30 m to 100 m aperture calls for t...
For extremely large telescopes, there is strong need for thin deformable mirrors in the 3-4 m class....
For extremely large telescopes, there is strong need for thin deformable mirrors in the 3-4 m class....
Research has been carried out on three major difficulties in designing efficient and economic telesc...
The telescopes of the Cherenkov Telescope Array (CTA) will have segmented mirrors, with mirror facet...
The telescopes of the Cherenkov Telescope Array (CTA) will have segmented mirrors, with mirror facet...
ABSTRACT A new class of telescope is being built with primary mirrors as large as 8.4 meters in diam...
The development of lightweight glass mirrors manufactured via cold-slumping technique for Imaging At...
The Cherenkov Telescope Array (CTA) is the next generation very high-energy gamma-ray observatory, w...
The Cherenkov Telescope Array (CTA) is the next generation very high-energy gamma-ray observatory, w...
The next generation of imaging atmospheric Cherenkov telescopes will require the production of thous...