Prospects for polarized foreground removal (2009)
- Authors:
- Autor USP: MAGALHAES, ANTONIO MARIO - IAG
- Unidade: IAG
- Subjects: SATÉLITES ARTIFICIAIS; GALÁXIA (VIA LÁCTEA)
- Language: Inglês
- Imprenta:
- Publisher: American Institute of Physics
- Publisher place: College Park
- Date published: 2009
- Source:
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ABNT
DUNKLEY, J e MAGALHÃES, Antônio Mário. Prospects for polarized foreground removal. 2009, Anais.. College Park: American Institute of Physics, 2009. . Acesso em: 05 mar. 2026. -
APA
Dunkley, J., & Magalhães, A. M. (2009). Prospects for polarized foreground removal. In CMB Polarization Workshop: Theory and Foregrounds : CMBPol Mission Concept Study: Batavia, IL, 23-26 June 2008. College Park: American Institute of Physics. -
NLM
Dunkley J, Magalhães AM. Prospects for polarized foreground removal. CMB Polarization Workshop: Theory and Foregrounds : CMBPol Mission Concept Study: Batavia, IL, 23-26 June 2008. 2009 ;[citado 2026 mar. 05 ] -
Vancouver
Dunkley J, Magalhães AM. Prospects for polarized foreground removal. CMB Polarization Workshop: Theory and Foregrounds : CMBPol Mission Concept Study: Batavia, IL, 23-26 June 2008. 2009 ;[citado 2026 mar. 05 ] - The interstellar magnetic field close to the sun. II
- Understanding the links among magnetic fields, filament, the bipolar bubble, and star formation in RCW57A using NIR polarimetry
- Whence the interstellar magnetic field shaping the heliosphere?
- Polarização em estrelas wolf-rayet binárias: simulações com o método de Monte Carlo
- Evidence for an interstellar dust filament in the outer heliosheath
- Connecting the interstellar magnetic field at the heliosphere to the Loop I superbubble
- Magnetic field structure of the small magellanic cloud
- Dust in a hostile environment: interstellar dust in the line of sight to hd 62542
- Blobs in Wolf-Rayet winds: random photometric and polarimetric variability
- Estrutura do campo magnético da pequena nuvem de Magalhães
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