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The Atacama Pathfinder Experiment (APEX)
Since 2005 the Atacama Pathfinder Experiment 12 meter telescope (APEX) in the Chilean Atacama desert
observes the Southern Sky at submillimeter wavelength. APEX is a joint project of the MPIfR,
ESO and
the Swedish
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The Effelsberg 100m-Radio
Telescope
The telescope is located only some dozen kilometers far from our institute
in Bad Münstereifel-Effelsberg and therefore can be considered
as a major workhorse.
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The IRAM 30m-Millimeter Telescope at Pico Veleta
The 30m-telescope near Granada, Spain, is operated by
IRAM.
For many years we supplied a series of Max-Planck-Bolometer (MAMBO)
Arrays operated at this telescope.
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The IRAM Interferometer at Plateau de Bure
The interferometer nearby Grenoble, France is operated by
IRAM.
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Submillimeter Array
The interferometer on top of Mauna Kea, Hawaii, is a joint venture between the
Smithsonian Astrophysical Observatory and
Academia Sinica Institute of Astronomy and Astrophysics.
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Caltech Submillimeter Observatory
This telescope at Mauna Kea, Hawaii is operated by the
Caltech Submillimeter Wave Astronomy Group.
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Very Large Array
This interferometer nearby Socorro, New Mexico is operated by
NRAO.
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Very Long Baseline Array
This interferometer consists of ten radio antennas spread across the United States and its territories. It is operated by
NRAO.
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European VLBI Network
This organization coordinates VLBI observations involving European telescopes.
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MERLIN
MERLIN, operated by Jodrell Bank Observatory, is the Multi-Element Radio
Linked Interferometer Network, an array of radio telescopes distributed
around Great Britain.
It operates at frequencies ranging from 151 MHz to 24 GHz.
At 5GHz, the resolution of MERLIN is better than 50 milliarcseconds,
somewhat greater than that of the Hubble Space Telescope.
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