The Simons Observatory: Design, Optimization, and Performance of Low-Frequency Detectors
The Simons Observatory (SO) is a cosmic microwave background (CMB) experiment located in the Atacama Desert in Chile that will make precise temperature and polarization measurements over six spectral bands ranging from 27 to 285 GHz. Three small aperture telescopes (SATs) and one large aperture tele...
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Veröffentlicht in: | Journal of low temperature physics 2025-01, Vol.218 (1), p.21-28 |
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Hauptverfasser: | , , , , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
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