activity
20002005
most citedFirst Release of Gauss-Legendre Sky Pixelization (GLESP) software package for CMB analysis

3 citations · 6 across the 3 of their papers we have counts for

collaborators

7 papers

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…

astro-ph2000

Ultra - High Energy Cosmic Rays from decay of the Super Heavy Dark Matter Relics

A. G. Doroshkevich, P. D. Naselsky

In this paper we briefly discuss the problem of the origin of Ultra High Energy Cosmic Rays in the framework of Top-Down models. We show that, for high energy of decays and in a wi…