2017/05/31 by Byeonghee Yu, J. Colin Hill, Blake D. Sherwin · 51 citations
Physics and Astronomy · #Anisotropy #Astronomy #Astrophysics #COSMIC cancer database #Cosmic background radiation #Cosmic infrared background #Cosmic microwave background #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gravitational lens #Optics #Physics #Planck #Radio Astronomy Observations and Technology #Redshift #Sky #astro-ph.CO
paper · pdf · doi:10.1103/physrevd.96.123511
published in Physical review. D/Physical review. D. 96(12) (American Physical Society) · 10 pages, 7 figures, data products available at http://www.sns.ias.edu/~jch/delens/
arxiv created 2017/12/05 · openalex publication_date 2017/12/12 · arxiv updated 2017/12/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Delensing, the removal of the limiting lensing B-mode background, is crucial for the success of future cosmic microwave background (CMB) surveys in constraining inflationary gravitational waves (IGWs). In recent work, delensing with large-scale structure tracers has emerged as a promising method both for improving constraints on IGWs and for testing delensing methods for future use. However, the delensing fractions (i.e., the fraction of the lensing-B mode power removed) achieved by recent efforts have been only 20%--30%. In this work, we provide a detailed characterization of a full-sky, dust-cleaned cosmic infrared background (CIB) map for delensing and construct a further-improved delensing template by adding additional tracers to increase delensing performance. In particular, we build a multitracer delensing template by combining the dust-cleaned Planck CIB map with a reconstructed CMB lensing map from Planck and a galaxy number density map from the Wide-field Infrared Survey Explorer (WISE) satellite. For this combination, we calculate the relevant weightings by fitting smooth templates to measurements of all the cross-spectra and autospectra of these maps. On a large fraction of the sky (fsky=0.43), we demonstrate that our maps are capable of providing a delensing factor of 43\ifmmode±\else\textpm\fi1%; using a more restrictive mask (fsky=0.11), the delensing factor reaches 48\ifmmode±\else\textpm\fi1%. For low-noise surveys, our delensing maps, which cover much of the sky, can thus improve constraints on the tensor-to-scalar ratio (r) by nearly a factor of 2. The delensing tracer maps are made publicly available, and we encourage their use in ongoing and upcoming B-mode surveys.