TL;DR
NaMaster is a comprehensive software package that unifies and validates pseudo-$C_ll$ estimators for angular power spectra, accommodating complex systematics, contaminant deprojection, and $E/B$ purification for cosmological data analysis.
Contribution
The paper introduces NaMaster, the first unified, validated software framework for computing angular cross-power spectra with advanced systematic handling and purification features.
Findings
NaMaster accurately recovers input spectra in complex simulated scenarios.
The software handles spin-0 and spin-2 fields on the sphere and flat-sky.
NaMaster is validated against realistic cosmological observation simulations.
Abstract
The pseudo- is an algorithm for estimating the angular power and cross-power spectra that is very fast and, in realistic cases, also nearly optimal. The algorithm can be extended to deal with contaminant deprojection and purification, and can therefore be applied in a wide variety of scenarios of interest for current and future cosmological observations. This paper presents NaMaster, a public, validated, accurate and easy-to-use software package that, for the first time, provides a unified framework to compute angular cross-power spectra of any pair of spin-0 or spin-2 fields, contaminated by an arbitrary number of linear systematics and requiring - or -mode purification, both on the sphere or in the flat-sky approximation. We describe the mathematical background of the estimator, including all the features above, and its software implementation in NaMaster. We…
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