A model of diffuse Galactic radio emission from 10 MHz to 100 GHz

Monthly Notices of the Royal Astronomical Society

Volumn 388, Issue 1, 2008, Pages 247-260

  de Oliveira Costa, Angélica ^a   Tegmark, Max ^a   Gaensler, B M ^b   Jonas, Justin ^c   Landecker, T L ^d   Reich, Patricia ^e  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF SYDNEY   (Australia)

^c RHODES UNIVERSITY   (South Africa)

^d NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Astronomical data bases: miscellaneous; Diffuse radiation; ISM: structure; Methods: data analysis; Radio continuum: ISM

Indexed keywords

COSMOLOGY; OPTICAL CHARACTER RECOGNITION; PRINCIPAL COMPONENT ANALYSIS;

100 GHZ; ASTRONOMICAL DATA BASE: MISCELLANEOUS; COSMIC MICROWAVE BACKGROUND EXPERIMENTS; COSMOLOGICAL MEASUREMENTS; DIFFUSE RADIATION; GALACTIC RADIO EMISSIONS; HIGH REDSHIFT UNIVERSE; ISM: STRUCTURE; METHODS. DATA ANALYSIS; RADIO CONTINUUM: ISM;

SURVEYS;

EID: 56349130235     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13376.x     Document Type: Article

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