1. Demonstration of Cosmic Microwave Background Delensing Using the Cosmic Infrared Background
- Author
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Anthony Challinor, Patricia Larsen, Daisy Mak, Blake D. Sherwin, Challinor, Anthony [0000-0003-3479-7823], and Apollo - University of Cambridge Repository
- Subjects
Physics ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,010308 nuclear & particles physics ,Cosmic microwave background ,Strong gravitational lensing ,General Physics and Astronomy ,Astronomy ,Spectral density ,FOS: Physical sciences ,Planck temperature ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,symbols.namesake ,Amplitude ,Gravitational lens ,Cosmic infrared background ,0103 physical sciences ,symbols ,astro-ph.CO ,Planck ,010303 astronomy & astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Delensing is an increasingly important technique to reverse the gravitational lensing of the cosmic microwave background (CMB) and thus reveal primordial signals the lensing may obscure. We present a first demonstration of delensing on Planck temperature maps using the cosmic infrared background (CIB). Reversing the lensing deflections in Planck CMB temperature maps using a linear combination of the 545 and 857GHz maps as a lensing tracer, we find that the lensing effects in the temperature power spectrum are reduced in a manner consistent with theoretical expectations. In particular, the characteristic sharpening of the acoustic peaks of the temperature power spectrum resulting from successful delensing is detected at a significance of 16$\rm{\sigma}$, with an amplitude of $A_{\rm{delens}} = 1.12 \pm 0.07$ relative to the expected value of unity. This first demonstration on data of CIB delensing, and of delensing techniques in general, is significant because lensing removal will soon be essential for achieving high-precision constraints on inflationary B-mode polarization., Comment: 6 pages, 5 figures, accepted for publication in PRL
- Published
- 2016