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Efficient GLS map-making and assessment of $1/f$ noise impact for future CMB satellite missions
Time-correlated $1/f$ noise is a major source of large-scale contamination in measurements of the polarized cosmic microwave background (CMB) that can limit sensitivity to primordial $B$ modes. Generalized least-squares (GLS) map-making is optimal for stationary Gaussian noise when its covariance is
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