| Project
Goal |
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| Characterize
the South Pole as a |
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| Submillimeter-wave
Astronomical Site |
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| – | Opacity as a
function of frequency and time |
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| – | Sky noise |
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| – | Atmospheric
Modeling to understand opacity and |
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| sky noise |
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| – | Precipitable
Water Vapor (PWV) as an input to |
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| models |
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| – | Comparison with
other sites |
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