Instruments and methods of investigation

Sky pixelization for the analysis of extended emission

 a,  b
a Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Zelenchukskiy Region, Karachai-Cherkessian Republic, Russian Federation
b Astro Space Centre, Lebedev Physical Institute, Russian Academy of Sciences, ul. Profsoyuznaya 84/32, Moscow, 117997, Russian Federation

Spherical pixelization schemes are reviewed for analyzing extended emission, and in particular for investigating the cosmic microwave background. Problems with implementing different schemes are considered. The nonhierarchical Gauss — Legendre sky pixelization (GLESP) approach is discussed in detail.

Fulltext is available at IOP
PACS: 95.75.−z, 95.85.Bh, 98.80.−k, 98.80.Es (all)
DOI: 10.3367/UFNe.0183.201308c.0849
Citation: Verkhodanov O V, Doroshkevich A G "Sky pixelization for the analysis of extended emission" Phys. Usp. 56 801–812 (2013)
BibTexBibNote ® (generic) BibNote ® (RIS)MedlineRefWorks
TI Sky pixelization for the analysis of extended emission
AU Verkhodanov, O. V.
AU Doroshkevich, A. G.
PB Physics-Uspekhi
PY 2013
JO Physics-Uspekhi
JF Physics-Uspekhi
JA Phys. Usp.
VL 56
IS 8
SP 801-812

Received: 14th, June 2012, revised: 18th, July 2012, 27th, July 2012

Оригинал: Верходанов О В, Дорошкевич А Г «Системы пикселизации неба для анализа протяжённого излучения» УФН 183 849–862 (2013); DOI: 10.3367/UFNr.0183.201308c.0849

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