TY  -  
T1  - Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization 
SN  -  /  
UR  - http://hdl.handle.net/10138/233356 
T3  -  
A1  - Ade, P. A. R.; Keihanen, E.; Kurki-Suonio, H.; Suur-Uski, A. -S.; Valiviita, J.; Planck Collaboration 
A2  -  
PB  -  
Y1  - 2015 
LA  - eng 
AB  - Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We use these data to characterize the frequency dependence of dust emission. We make use of the Planck 353 GHz I, Q, and U Stokes maps as dust templates, and cross-correlate them with the Planck and WMAP data at 12 frequencies from 23 to 353 GHz, over circular patches with 10 degrees radius. The cross-correlation analysis is performed for both intensity and polarization data in a ... 
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SP  -  
OP  -  
KW  - polarization; ISM: general; Galaxy: general; radiation mechanisms: general; submillimeter: ISM; infrared: ISM; MICROWAVE-ANISOTROPY-PROBE; H-ALPHA EMISSION; DMR SKY MAPS; SPINNING DUST; WMAP OBSERVATIONS; INTERSTELLAR DUST; SUBMILLIMETER POLARIZATION; MAGNETIC NANOPARTICLES; COMPONENT SEPARATION; FOREGROUND EMISSION; 115 Astronomy, Space science 
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ER  -