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Welcome to the biennial report of the Isaac Newton Group of Telescopes for
the years 2004 and 2005. The dynamics and excitement of astronomy have certainly
been felt at the observatory during the last two years. As you can read in this
report many scientific highlights passed the scene and important technical advances
were made. This report provides an overview of the main events and summarizes
the financial status and scientific output of the telescopes. The successes
and achievements over the period covered by this report have only been possible
thanks to the continued quality efforts of ING staff, who have shown a high
level of commitment and professionalism through uncertain and sometimes difficult
times.
It is now some thirty years ago that La Palma was being explored as a potential
location for a new observatory in the Northern hemisphere. That choice has most
certainly paid off in scientific terms. The site testing equipment in those
days was not so sophisticated to today’s standards and the circumstances
under which the work was conducted were rather primitive. The pictures below
(courtesy of site tester Thomas Gough) give an impression of the situation.
Although the observatory is now well established, characterization of the observing
site continues and is even stepping up pace with the advent of adaptive optics,
the construction of very large telescopes such as the 10m GTC, and the possibility
of construction of a future Extremely Large Telescope. In the early days analysis
of star trails and of sparse meteorological measurements were the basis for
initiating the observatory; now we possess an arsenal of additional tool such
as DIMM, MASS, SLODAR, and remote sensing to help us decide on the quality of
the atmosphere. But what remains the same is the finding that La Palma is one
of the very best observing sites in the World.
The reporting years saw also intense activity on growing European collaboration
between observatories in which ING was strongly involved. Under the umbrella
of OPTICON a large programme to promote trans-national access to telescopes
was initiated. The demand for observing programmes for the ING telescopes was
so large that limits had to be imposed to prevent the scheme from running out
of resources. European collaboration, not only for the construction of future
large facilities, but also for existing observatories will be beneficial to
European astronomy at large. ING hopes to play a key role in this as well.