Dust distribution during reionization

2007/05/31 by E. Elfgren, Erik Elfgren, F.–X. Désert +3
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #COSMIC cancer database #Context (archaeology) #Cosmic microwave background #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Galaxy #Geography #Optics #Physics #Redshift #Reionization #Stars #astro-ph

paper · pdf · doi:10.1051/0004-6361:20053151

published as Astron.Astrophys.476:1145-1150,2007 · 6 pages, 6 figures; Typos fixed. Clarifications in the abstract, sections 2 and 4.1 and fig 6

arxiv created 2007/10/22 · openalex publication_date 2007/10/23 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. The dust produced by the first generation of stars will be a foreground to cosmic microwave background.

Citations

• Using SCUBA to place upper limits on arcsecond-scale cosmic microwave background anisotropies at 850 m
• GALICS- I. A hybrid N-body/semi-analytic model of hierarchical galaxy formation
• The Implications of Wilkinson Microwave Anisotropy Probe Observations for Population III Star Formation Processes
• Neutrino masses and the number of neutrino species from WMAP and 2dFGRS
• First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic Results
• First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters