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The millimetre and submillimetre spectral region (300 to 3000 Ilm
or 1000 to 100 GHz) was until recently one of the few spectral
regimes not fully opened up for astronomical studies. Thanks both
to improvements in detectors and receivers and to the construction
of large telescopes at high altitude sites this situation is
improving very rapidly. Three major telescopes have been built
recently and are coming into operation during 1987 and 1988, namely
the 15m James Clerk Maxwell Telescope (JCMT) and the lOAm Caltech
Submillimetre Observatory (CSO) telescope, both located on Mauna
Kea, Hawaii, and the 15 m Swedish -ESO telescope (SEST) in Chile.
Because a very wide range of astronomical problems can be tackled
with these major new facilities there is a great deal of interest
from the many potential new users anxious to become familiar with
this rapidly developing field. During 1986 it became clear to
British and Dutch astronomers involved in planning the
commissioning and operation of the JCMT, that a summer school in
this field would greatly benefit the potential and actual JCMT user
community. With financial support from the SERC and supplemented by
a grant from the ZWO, the Summer School on 'Millimetre and
Submillimetre Astronomy' was held at Stirling University from June
21 to 27, 1987.
The millimetre and submillimetre spectral region (300 to 3000 Ilm
or 1000 to 100 GHz) was until recently one of the few spectral
regimes not fully opened up for astronomical studies. Thanks both
to improvements in detectors and receivers and to the construction
of large telescopes at high altitude sites this situation is
improving very rapidly. Three major telescopes have been built
recently and are coming into operation during 1987 and 1988, namely
the 15m James Clerk Maxwell Telescope (JCMT) and the lOAm Caltech
Submillimetre Observatory (CSO) telescope, both located on Mauna
Kea, Hawaii, and the 15 m Swedish -ESO telescope (SEST) in Chile.
Because a very wide range of astronomical problems can be tackled
with these major new facilities there is a great deal of interest
from the many potential new users anxious to become familiar with
this rapidly developing field. During 1986 it became clear to
British and Dutch astronomers involved in planning the
commissioning and operation of the JCMT, that a summer school in
this field would greatly benefit the potential and actual JCMT user
community. With financial support from the SERC and supplemented by
a grant from the ZWO, the Summer School on 'Millimetre and
Submillimetre Astronomy' was held at Stirling University from June
21 to 27, 1987.
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