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Submillimetre astronomy or
submillimeter astronomy (see
spelling differences) is the
branch of
observational astronomy that is
conducted at submillimetre...
- The
Submillimeter Array (SMA)
consists of
eight 6-meter (20 ft)
diameter radio telescopes arranged as an
interferometer for
submillimeter wavelength observations...
- one of the world's
premier observatories for optical, infrared, and
submillimeter astronomy, and in 2009 was the
largest measured by
light gathering power...
- The
Caltech Submillimeter Observatory (CSO) was a 10.4-meter (34 ft)
diameter submillimeter wavelength telescope situated alongside the 15-meter (49 ft)...
- The
Atacama Large Millimeter/
submillimeter Array (ALMA) is an
astronomical interferometer of 66
radio telescopes in the
Atacama Desert of
northern Chile...
- The
Submillimeter Telescope (SMT),
formerly known as the
Heinrich Hertz Submillimeter Telescope, is a
submillimeter wavelength radio telescope located...
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Submillimeter Wave
Astronomy Satellite (SWAS, also
Explorer 74 and SMEX-3) is a NASA
submillimetre astronomy satellite, and is the
fourth spacecraft in...
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around 1
millimeter and
proceeds into
shorter wavelengths, it is
sometimes known as the
submillimeter band, and its
radiation as
submillimeter waves, especially...
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telescope is
designed for
observations in the microwave,
millimeter-wave, and
submillimeter-wave
regions of the
electromagnetic spectrum, with the particular...
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objects visible in far-infrared
radiation (extending from 30 μm
towards submillimeter wavelengths around 450 μm). In the far-infrared,
stars are not especially...
