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Dust Polarization From Starlight Data
Pablo Fosalba, Alex Lazarian, Simon Prunet +1
We present a statistical analysis of the interstellar medium (ISM) polarization from the largest compilation available of starlight data, which comprises ~ 5500 stars. The measured…
Polarized Microwave Emission from Dust
A. Lazarian, S. Prunet
Polarized emission from dust is an important foreground that can hinder the progress in polarized CMB studies unless carefully accounted for. We discuss potential difficulties asso…
Fast Clustering Analysis of Inhomogeneous Megapixel CMB maps
I. Szapudi, S. Prunet, S. Colombi
Szapudi et al (2001) introduced the method of estimating angular power spectrum of the CMB sky via heuristically weighted correlation functions. Part of the new technique is that a…
MASTER of the CMB Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex CMB Data Sets
E. Hivon, K. M. Gorski, C. B. Netterfield +3
We describe a fast and accurate method for estimation of the cosmic microwave background (CMB) anisotropy angular power spectrum --- Monte Carlo Apodised Spherical Transform Estima…
Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
P. de Bernardis, P. A. R. Ade, J. J. Bock +32
Three peaks and two dips have been detected in the power spectrum of the cosmic microwave background from the BOOMERANG experiment, at and $\ell \sim 420,…
Statistical Properties of Galactic Starlight Polarization
Pablo Fosalba, Alex Lazarian, Simon Prunet +1
We present a statistical analysis of Galactic interstellar polarization from the largest compilation available of starlight data. The data comprises ~ 9300 stars of which we have s…