MILLIMETER WAVE
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Last Modified: Wednesday, 17-October-02 10:05 AM EDT


This material is based on work supported by the National Science Foundation under Grants AST-9532046 and AST-9725951.

Any opinions, findings and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect those of the National Science Foundation.

System Performance

  • The SEQUOIA array is competitive with wideband SIS receivers, and much simpler to use.
  • The receiver is cooled by a single 3.5W (at 18K) refrigerator.
  • SEQUOIA's spectral line baseline stability is excellent. Gain fluctuations are large (0.2%) but highly correlated across a wide band.
  • System reliability has been excellent in the first three years of operation.
Noise temperature per pixel per frequency
Noise temperature per pixel per frequency




View of the front end of the receiver


That concludes the SEQUOIA tour. Please come again!

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