ABSTRACT A new class of telescope is being built with primary mirrors as large as 8.4 meters in diameter and as fast as f/i . Fabricating the secondary mirrors for these telescopes has presented tough challenges because of their large sizes, up to 1.7 meter diameter; their aspheric departure of more than 300 microns; the required figure accuracy of a few tens of nanometers; and the fact that they are typically convex and difficult to measure. We have developed tools and techniques to meet these demands to produce secondary mirrors efficiently and accurately. A dedicated facility was constructed in the Mirror Lab that integrates a 1 .8-m stressed-lap polishing machine with interferometric and mechanical measuring systems. This paper presents...
The Giant Magellan Telescope (GMT) primary mirror consists of seven 8.4 m light-weight honeycomb mir...
ABSTRACT We present a plan for making the optics of a 21 m telescope that builds on advances in mirr...
The two 911mm-diameter adaptive secondary (AS) mirrors for the Large Binocular telescope (LBT) are c...
Modern large telescopes such as TAO, LSST, TMT and EELT require 0.9m-4m monolithic convex secondary ...
The pursuit of economical fabrication of large (8 m) fast ( < f/2), astronomical optics has led t...
This thesis demonstrates the possibility of manufacturing larger mirrors from nickel coated aluminiu...
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....
The Richard F. Carts Mirror Lab at the University of Arizona continues the production of 8.4 m light...
Large convex aspheres are notoriously difficult to fabricate because of the tremendous cost and diff...
Research has been carried out on three major difficulties in designing efficient and economic telesc...
The Richard F. Caris Mirror Lab at the University of Arizona continues production of 8.4 m lightweig...
Classical fabrication methods alone do not enable manufacturing of large flat mirrors that are much ...
QC 351 A7 no. 79In this report we describe the work carried out under contract F19628-72-C-0047 enti...
We are developing technologies in processing and metrology to fabricate a 1.4-meter aperture, aspher...
The Giant Magellan Telescope (GMT) primary mirror consists of seven 8.4 m light-weight honeycomb mir...
ABSTRACT We present a plan for making the optics of a 21 m telescope that builds on advances in mirr...
The two 911mm-diameter adaptive secondary (AS) mirrors for the Large Binocular telescope (LBT) are c...
Modern large telescopes such as TAO, LSST, TMT and EELT require 0.9m-4m monolithic convex secondary ...
The pursuit of economical fabrication of large (8 m) fast ( < f/2), astronomical optics has led t...
This thesis demonstrates the possibility of manufacturing larger mirrors from nickel coated aluminiu...
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....
The Richard F. Carts Mirror Lab at the University of Arizona continues the production of 8.4 m light...
Large convex aspheres are notoriously difficult to fabricate because of the tremendous cost and diff...
Research has been carried out on three major difficulties in designing efficient and economic telesc...
The Richard F. Caris Mirror Lab at the University of Arizona continues production of 8.4 m lightweig...
Classical fabrication methods alone do not enable manufacturing of large flat mirrors that are much ...
QC 351 A7 no. 79In this report we describe the work carried out under contract F19628-72-C-0047 enti...
We are developing technologies in processing and metrology to fabricate a 1.4-meter aperture, aspher...
The Giant Magellan Telescope (GMT) primary mirror consists of seven 8.4 m light-weight honeycomb mir...
ABSTRACT We present a plan for making the optics of a 21 m telescope that builds on advances in mirr...
The two 911mm-diameter adaptive secondary (AS) mirrors for the Large Binocular telescope (LBT) are c...