k SEST radio telescope at La Silla, Chile SEST telescope. View from behind of the dish of the SwedishESO Submillimetre Telescope SEST at the European Southern Observatory ESO site at La Silla, Chile. The 15metre diameter dish of this radio telescope is used for observations at frequencies of 70365 gigahertz, corresponding to wavelengths of 0.8 to 42 millimetres. The parabolic surface of the dish is used to focus incoming electromagnetic radiation. Stock Photo - Afloimages
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SEST radio telescope at La Silla, Chile SEST telescope. View from behind of the dish of the Swedish ESO Submillimetre Telescope SEST at the European Southern Observatory ESO site at La Silla, Chile. The 15 metre diameter dish of this radio telescope is used for observations at frequencies of 70 365 gigahertz, corresponding to wavelengths of 0.8 to 42 millimetres. The parabolic surface of the dish is used to focus incoming electromagnetic radiation.
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SEST radio telescope at La Silla, Chile

SEST telescope. View from behind of the dish of the Swedish-ESO Submillimetre Telescope (SEST) at the European Southern Observatory (ESO) site at La Silla, Chile. The 15-metre diameter dish of this radio telescope is used for observations at frequencies of 70-365 gigahertz, corresponding to wavelengths of 0.8 to 42 millimetres. The parabolic surface of the dish is used to focus incoming electromagnetic radiation.

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