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Scanning and Mapping Strategies for CMB Experiments

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TLDR
A time-ordered method for map-making with one-horned experiments that has reasonable memory and CPU needs but can handle complex COBE-like scans paths and 1/f noise is given.
Abstract
CMB anisotropy experiments seeking to make maps with more pixels than the 6144 pixels used by the COBE DMR need to address the practical issues of the computer time and storage required to make maps. A simple, repetitive scan pattern reduces these requirements but leaves the experiment vulnerable to systematic errors and striping in the maps. In this paper I give a time-ordered method for map-making with one-horned experiments that has reasonable memory and CPU needs but can handle complex COBE-like scans paths and 1/f noise.

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Cosmic confusion: degeneracies among cosmological parameters derived from measurements of microwave background anisotropies

TL;DR: In this article, the authors analyse degeneracies among cosmological parameters to illustrate some of the limitations inherent in CMB parameter estimation and show that small correlated errors in estimates of the CMB power spectrum at levels well below the cosmic variance limits (caused, for example, by Galactic foregrounds or scanning errors).
Posted Content

CMB-S4 Science Case, Reference Design, and Project Plan

Kevork N. Abazajian, +224 more
TL;DR: In this article, the authors present the science case, reference design, and project plan for the Stage-4 ground-based cosmic microwave background experiment CMB-S4, as well as the experimental data.
Journal ArticleDOI

Overview of the atacama cosmology telescope: receiver, instrumentation, and telescope systems

TL;DR: The Atacama Cosmology Telescope as discussed by the authors was designed to measure small-scale anisotropies in the cosmic microwave background and detect galaxy clusters through the Sunyaev-Zel'dovich effect.
Journal ArticleDOI

Foregrounds and CMB experiments: I. Semi-analytical estimates of contamination

TL;DR: In this article, an indicator of the accuracy of the separation of the CMB anisotropies from those induced by foregrounds is presented, based on a generalisation of the Wiener filtering method to multi-frequency, multi-resolution data.
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