Fig. I.2: The Calar Alto observatory, a view from the north towards the telescope domes.
From left to right: the 2.2-metre telescope, the Spanish 1.5-metre telescope, the 1.2-metre telescope, the Schmidt reflector and the 43-metre high dome of the 3.5-metre telescope. In the background can be seen the Almeria coast.
  I General
ved in cooperation with the Carl Zeiss company at Oberkochen and other companies. In this way, a large number of companies have acquired know-how which has helped them to secure leading positions on the world market.
Between 1975 and 1984, the 1.2-metre reflector financed by the Deutsche Forschungsgemeinschaft/ German Research Association as well as the 2.2-metre and 3.5-metre telescopes started operation on Calar Alto (Figure I.2). The 80-centimetre Schmidt telescope was transferred from the Hamburg Observatory. There is also a Spanish 1.5-metre telescope on the site which does not belong to the DSAZ: the Observatorio Nacional de Madrid is in charge of this instrument. The original plans to construct a southern observatory on the Gamsberg in Namibia could not be implemented for political reasons. The 2.2-metre telescope which was intended for this purpose has been loaned to the European Southern Observatory for 25 years. Since 1984, it has been in operation on La Silla Mountain in Chile, where 25% of its observation time is available to the astronomers of the MPIA.
One aspect of the MPIA’s present task is the operation of the Calar Alto Observatory. This includes the constant optimisation of the telescopes’ capabilities: now that the ALFA adaptive optical system has been commissioned, the 3.5-metre telescope is once again at the forefront of technological development (Chapter II.1).
Other aspects include the development of new measuring instruments in Heidelberg, the preparation of observation programmes and the evaluation of the data obtained from the telescopes. A substantial part of the Institute’s work is devoted to building new instruments for the telescopes (Chapter III). The MPIA is equipped with ultra-modern precision mechanics and electronics workshops for this purpose. The Calar Alto Observatory provides the MPIA with one of the two European observatories with the highest performance. Research concentrates on the »classical« visible region of the spectrum and on the infrared region.
In addition to these tasks, the MPIA has been engaged in extra-terrestrial research ever since it was established. This was associated with an early start on infrared astronomy which has played a particularly important part in the Institute’s later development as a whole. Nowadays, the MPIA has a substantial involvement in the ISO project (Infrared Space Observatory, Figure I.3) of the


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