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Description of UKIRT
The Infrared Flux Collector, as it was originally called, was proposed
by
Prof. Jim Ring of Imperial College, London and Gordon Carpenter of the
Royal Observatory, Edinburgh. It was built between 1975 and 1978. It is
a
classical Cassegrain telescope with a primary mirror which is about
half
as
thick as those of conventional telescopes of its era. The design is
derived
from that of the 1.5m IR Flux Collector (now the Carlos Sanchez
Telescope)
in Tenerife, and was originally conceived as an inexpensive "light
bucket"
with very relaxed specifications.
The mechanical structure of UKIRT was designed and built by Dunford
Hadfields of Sheffield, UK, and the optics (originally providing f/9
Cassegrain and f/19 coude foci) were manufactured by the now-defunct
firm
of Grubb Parsons & Co. of Newcastle-upon-Tyne, UK, who pioneered
the
figuring of large thin mirrors in the process.
The telescope was officially opened in October 1979. Since then it
has
been steadily improved; by the early '80s it was performing several
times
better than its specifications required. After a programme of upgrades
carried out between 1990 and 1998 it is currently delivering what is
believed to be the best imaging performance of any ground-based
telescope.
Thanks to this and to a state-of-the-art instrument suite UKIRT is
currently one of the most scientifically productive telescopes in the
world, producing over 80 scientific papers per year.
UKIRT currently operates at f/36.4; details of its optical system
are listed elsewhere.
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