А. G. Doroshkevich

6 ta ish

Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, 125047 Moscow, Russia

1. Statistical characteristics of large scale structure

   M. Demiański, А. G. Doroshkevich

   MaqolaGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics20041 iqtibos

   ABIABI:AkademIndex/openalex/2004.article.000048

2. Geometrical methods of analysis of polarization of CMB

   A. D. Dolgov, А. G. Doroshkevich, D. Novikov +1

   MaqolaCosmology and Gravitation TheoriesAstronomical and Astrophysical Transactions20000 iqtibos

   ABIABI:AkademIndex/openalex/2000.article.000035

3. Ultra - High Energy Cosmic Rays from decay of the Super Heavy Dark\n Matter Relics

   А. G. Doroshkevich, Pavel Naselsky, P. D. Naselsky

   PreprintAstrophysics and Cosmic PhenomenaarXiv (Cornell University)20000 iqtibos

   ABIABI:AkademIndex/openalex/2000.preprint.000003

4. Phase cross-correlation of the WMAP ILC map and foregrounds

   P. D. Naselsky, А. G. Doroshkevich, О. В. Верходанов

   PreprintNeutrino Physics ResearchCERN Document Server (European Organization for Nuclear Research)20030 iqtibos

   ABIABI:AkademIndex/openalex/2003.preprint.000001

5. Physical state of the intergalactic medium at redshifts<i>z</i>= 2-4

   M. Demiański, А. G. Doroshkevich

   MaqolaGalaxies: Formation, Evolution, PhenomenaMonthly Notices of the Royal Astronomical Society20040 iqtibos

   ABIABI:AkademIndex/openalex/2004.article.000137

6. Minimal Spanning Tree Technique

   А. G. Doroshkevich

   BobComputational Physics and Python Applications20060 iqtibos

   ABIABI:AkademIndex/openalex/2006.chapter.000022