Separation of anomalous and synchrotron emissions using WMAP polarization data

Astronomy and Astrophysics

Volumn 490, Issue 3, 2008, Pages 1093-1102

  Miville Deschenes M A ^a,b   Ysard, N ^a   Lavabre, A ^a   Ponthieu, N ^a   MacIas Perez J F ^c   Aumont, J ^c,d   Bernard, J P ^d  

^a UNIVERSITÉ PARIS SUD   (France)

^b UNIVERSITY OF TORONTO   (Canada)

^c UNIVERSITÉ JOSEPH FOURIER GRENOBLE 1   (France)

^d IRAP   (France)

Author keywords

Dust, extinction; ISM: magnetic fields; Polarization; Radio continuum: ISM; Turbulence

Indexed keywords

COSMOLOGY; DUST; ELECTROMAGNETIC WAVES; EMISSION SPECTROSCOPY; ISOMERS; MAGNETIC FIELD MEASUREMENT; MAGNETIC FIELDS; MAGNETIC MATERIALS; MAGNETISM; OPTICAL WAVEGUIDES; POLARIZATION; POWER SPECTRUM; SEPARATION; SIGNAL TO NOISE RATIO; SYNCHROTRON RADIATION; SYNCHROTRONS; TURBULENCE;

A MAGNETIC FIELDS; CLASSICAL MODELS; COMPONENT SEPARATIONS; DUST EMISSIONS; DUST MODELS; DUST, EXTINCTION; GALACTIC MAGNETIC FIELDS; INTENSITY DATUM; INTERSTELLAR MEDIUMS; ISM: MAGNETIC FIELDS; JOINT ANALYSES; LARGE-SCALE; MEAN-VALUE; MICROWAVE EMISSIONS; PITCH ANGLES; PLANCK MISSIONS; POLARIZATION DATUM; POWER LAW SPECTRUMS; RADIO CONTINUUM: ISM; SIGNAL-TO-NOISE RATIOS; SPATIAL VARIATIONS; SPECTRAL INDICES; SPIRAL MODELS; STANDARD DEVIATIONS; SYNCHROTRON EMISSIONS;

MATHEMATICAL MODELS;

EID: 54949107039     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809484     Document Type: Article

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