Cooling Improves Cosmic Microwave Background Map-making when Low-frequency Noise is Large
In the context of cosmic microwave background data analysis, we study the solution to the equation that transforms scanning data into a map. As originally suggested in “messenger” methods for solving linear systems, we split the noise covariance into uniform and nonuniform parts and adjust their rel...
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Veröffentlicht in: | The Astrophysical journal 2021-12, Vol.922 (2), p.97 |
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