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SANEPIC: A Map-Making Method for Timestream Data From Large Arrays

1 Pith paper cite this work. Polarity classification is still indexing.

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abstract

We describe a map-making method which we have developed for the Balloon-borne Large Aperture Submillimeter Telescope (BLAST) experiment, but which should have general application to data from other submillimeter arrays. Our method uses a Maximum Likelihood based approach, with several approximations, which allows images to be constructed using large amounts of data with fairly modest computer memory and processing requirements. This new approach, Signal And Noise Estimation Procedure Including Correlations (SANEPIC), builds upon several previous methods, but focuses specifically on the regime where there is a large number of detectors sampling the same map of the sky, and explicitly allowing for the the possibility of strong correlations between the detector timestreams. We provide real and simulated examples of how well this method performs compared with more simplistic map-makers based on filtering. We discuss two separate implementations of SANEPIC: a brute-force approach, in which the inverse pixel-pixel covariance matrix is computed; and an iterative approach, which is much more efficient for large maps. SANEPIC has been successfully used to produce maps using data from the 2005 BLAST flight.

fields

astro-ph.IM 1

years

2026 1

verdicts

UNVERDICTED 1

representative citing papers

Robust CMB polarisation mapmaking with a rotating half-wave plate

astro-ph.IM · 2026-06-30 · unverdicted · novelty 6.0

POMME is a new estimator that marginalizes signals varying slower than the HWP rotation timescale to produce unbiased CMB polarisation maps with near-optimal noise in the presence of strong contaminants.

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Showing 1 of 1 citing paper.

  • Robust CMB polarisation mapmaking with a rotating half-wave plate astro-ph.IM · 2026-06-30 · unverdicted · none · ref 12 · internal anchor

    POMME is a new estimator that marginalizes signals varying slower than the HWP rotation timescale to produce unbiased CMB polarisation maps with near-optimal noise in the presence of strong contaminants.