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The COSETI Observatory

  • The Electromagnetic Spectrum.

    • The “Optical” spectrum regime covers the range of wavelengths from 10-3 m
      (far-infrared) to 10-8 m
      (ultra-violet).

  • SETI “Magic Optical Wavelengths”.

    • Carbon Dioxide CO2
      (10.6 microns).

    NGC5850

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