Abstract
The University College London Echelle Spectrograph (UCLES) was commissioned in June 1988 at the Anglo-Australian Telescope (AAT). The main characteristics of this novel instrument are summarized. The use of ray tracing techniques not only for the optical design, but for alignment and calibration, is described. This has been very successful also for the control of UCLES. The results obtained during laboratory tests and during the first observing sessions at the AAT are presented, together with a description of future implementations.
Original language | English |
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Title of host publication | Instrumentation in Astronomy VII |
Subtitle of host publication | SPIE astronomical telescopes and instrumentation for the 21st century |
Editors | David L. Crawford |
Pages | 562-576 |
Number of pages | 15 |
Volume | 1235 |
DOIs | |
Publication status | Published - 1 Jul 1990 |
Externally published | Yes |
Event | SPIE Astronomical Telescopes and Instrumentation for the 21st Century - Tucson, United States Duration: 11 Feb 1990 → 16 Feb 1990 Conference number: 7 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
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Publisher | SPIE |
Volume | 1235 |
ISSN (Print) | 0277-786X |
Conference
Conference | SPIE Astronomical Telescopes and Instrumentation for the 21st Century |
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Country/Territory | United States |
City | Tucson |
Period | 11/02/90 → 16/02/90 |