Delensing CMB <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>B</mml:mi> </mml:mrow> </mml:math> -modes using galaxy surveys: The effect of galaxy bias and matter clustering nonlinearities

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Journal
Physical review. D/Physical review. D.
Published
2025-12-01
DOI
https://doi.org/10.1103/krp5-rq56
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
0.00
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article

Delensing CMB <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>B</mml:mi> </mml:mrow> </mml:math> -modes using galaxy surveys: The effect of galaxy bias and matter clustering nonlinearities

Karl J. Friston
Physical review. D/Physical review. D.
Galaxies: Formation, Evolution, Phenomena
article

Delensing CMB <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>B</mml:mi> </mml:mrow> </mml:math> -modes using galaxy surveys: The effect of galaxy bias and matter clustering nonlinearities

Karl J. Friston
article en

Abstract

No abstract available for this paper.
Physical review. D/Physical review. D.Vol. 112(12)
Berkeley College (US), Lawrence Berkeley National Laboratory (US), University of California System (US), Instituto de Física de Cantabria (ES), University of California, Berkeley (US)
Openalex Percentile: Top 73%
Galaxies: Formation, Evolution, Phenomena
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Delensing CMB <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>B</mml:mi> </mml:mrow> </mml:math> -modes using galaxy surveys: The effect of galaxy bias and matter clustering nonlinearities — Karl J. Friston · Physical review. D/Physical review. D. (2025) | TGRS Research Map | TGRS