The impact of Galactic synchrotron emission on CMB anisotropy measurements

2007/12/18 by L. La Porta, C. Burigana, W. Reich +1 · 50 citations
Physics and Astronomy · #Anisotropy #Astronomy #Astrophysics #Context (archaeology) #Cosmic microwave background #Cosmic ray #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Geology #Limiting #Optics #Physics #Radio Astronomy Observations and Technology #Synchrotron #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078435

published in Astronomy and Astrophysics 479(3), 641-654 (EDP Sciences) · 15 pages, 20 figures, Astronomy & Astrophysics, accepted

openalex publication_date 2007/12/18 · arxiv created 2008/01/03 · arxiv updated 2009/12/01 · openalex created_date 2022/10/03 · openalex updated_date 2026/07/31

Abstract

Context. Galactic foreground emission fluctuations are a limiting factor for precise cosmic microwave background (CMB) anisotropy measurements.

Citations

• Observational constraints on the cosmological evolution of dual-population radio sources
• First‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Foreground Emission
• The large-scale clustering of radio sources
• A Full‐Sky Hα Template for Microwave Foreground Prediction
• Full sky study of diffuse Galactic emission at decimeter wavelenghts
• Three‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Temperature Analysis
• Cosmic-Ray Propagation and Interactions in the Galaxy
• Extragalactic source counts and contributions to the anisotropies of the cosmic microwave background: predictions for the Planck Surveyor mission
• Particle Physics Models of Inflation and the Cosmological Density Perturbation
• Three‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Implications for Cosmology
• A determination of the spectra of Galactic components observed by the Wilkinson Microwave Anisotropy Probe

Cited by

• ALL-SKY INTERFEROMETRY WITH SPHERICAL HARMONIC TRANSIT TELESCOPES