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20002008
most citedFirst Release of Gauss-Legendre Sky Pixelization (GLESP) software package for CMB analysis

3 citations · 7 across the 4 of their papers we have counts for

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8 papers · 1 filter

astro-ph20081 cited

Fast simulation of the whole-sky CMB map in the presence of primordial magnetic field

Pavel Naselsky, Jaiseung Kim

We present a novel method for generation of sets of the Cosmic Microwave Background (CMB) anisotropy maps, which reproduces the correlations associated with Alfvén turbulenc…

astro-ph20053 cited

First Release of Gauss-Legendre Sky Pixelization (GLESP) software package for CMB analysis

A. G. Doroshkevich, P. D. Naselsky, O. V. Verkhodanov +5

We report the release of the Gauss--Legendre Sky Pixelization (GLESP) software package version 1.0. In this report we present the main features and functions for processing and man…

astro-ph20033 cited

Phase analysis of the 1-year WMAP data and its application for the CMB foreground separation

Pavel D. Naselsky, Oleg V. Verkhodanov, Lung-Yih Chiang +1

We present a new method based on phase analysis for the Galaxy and foreground component separation from the cosmic microwave background (CMB) signal. This method is based on a prev…

astro-ph2002

Missing Parameters in the CMB Physics

Pavel D. Naselsky

The lecture is devoted to the comparison of a few models of cosmic recombination kinetics with recent CMB anisotropy data and to corresponding predictions for the upcoming PLANCK m…

astro-ph2001

Cosmic Microwave Background polarization and the ionization history of the Universe

Pavel Naselsky, Jens Schmalzing, Jesper Sommer-Larsen +1

We point out that polarization measurements as planned for the upcoming PLANCK mission can significantly enhance the accuracy of cosmic parameter estimation compared to the tempera…

astro-ph2000

Estimation of Signal and Noise Parameters from CMB Polarization Observations

P. Naselsky, D. Novikov, I. Novikov +1

We propose a technique for determination of the spectral parameters of the cosmological signal and pixel noise using observational data on CMB polarization without any additional a…