k SEST radio telescope at La Silla, Chile SEST telescope. Dish of the SwedishESO Sub millimetre Telescope SEST at the European Southern Observatory ESO site at La Silla, Chile, during twilight. 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 reflect focus incoming electromagnetic radiation onto the receiving antenna above its centre. Stock Photo - Afloimages
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SEST radio telescope at La Silla, Chile SEST telescope. Dish of the Swedish ESO Sub millimetre Telescope SEST at the European Southern Observatory ESO site at La Silla, Chile, during twilight. 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 reflect focus incoming electromagnetic radiation onto the receiving antenna above its centre.
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SEST radio telescope at La Silla, Chile

SEST telescope. Dish of the Swedish-ESO Sub- millimetre Telescope (SEST) at the European Southern Observatory (ESO) site at La Silla, Chile, during twilight. 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 reflect & focus incoming electromagnetic radiation onto the receiving antenna above its centre.

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