High Galactic latitude polarized emission at 1.4 GHz and implications for cosmic microwave background observations

Monthly Notices of the Royal Astronomical Society

Volumn 358, Issue 1, 2005, Pages 1-12

  Carretti, E ^a   Bernardi, G ^a   Sault, R J ^b   Cortiglioni, S ^a   Poppi, S ^c  

^a OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b CSIRO   (Australia)

^c CNR   (Italy)

Author keywords

Cosmic microwave background; Diffuse radiation; Polarization; Radiation mechanisms: non thermal; Radio continuum: ISM

Indexed keywords

COSMOLOGY; INTERFEROMETERS; MICROWAVES; POWER SPECTRUM; SURVEYS;

ANGULAR SCALE; AUSTRALIA; COSMIC MICROWAVES BACKGROUND; DIFFUSE RADIATION; FARADAY ROTATION EFFECT; GALACTIC LATITUDE; POLARIZED EMISSIONS; POWER-SPECTRA; RADIATION MECHANISMS: NONTHERMAL; RADIO CONTINUUM: ISM;

POLARIZATION;

EID: 15544382218     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08761.x     Document Type: Article

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