Erratum: Baryonic effects on CMB lensing and neutrino mass constraints (Physical Review D (2020) 101 (063534) DOI: 10.1103/PhysRevD.101.063534)

Eegene Chung; Simon Foreman; Alexander Van Engelen

doi:10.1103/PhysRevD.102.109903

Erratum: Baryonic effects on CMB lensing and neutrino mass constraints (Physical Review D (2020) 101 (063534) DOI: 10.1103/PhysRevD.101.063534)

Eegene Chung, Simon Foreman, Alexander Van Engelen

Earth and Space Exploration, School of (SESE)

Research output: Contribution to journal › Comment/debate › peer-review

2 Scopus citations

Abstract

The Clkk curves displayed in Fig. 1 were computed using Eq. (1), with the form of Pm(k,z) given by Eq. (3). Our numerical implementation of this computation contained an error that affected these curves and the other results derived from them. In addition, there was a separate error that only affected the matter power spectra from the IllustrisTNG300 simulation and the associated Clkk computation1.

Original language	English (US)
Article number	109903
Journal	Physical Review D
Volume	102
Issue number	10
DOIs	https://doi.org/10.1103/PhysRevD.102.109903
State	Published - Nov 25 2020

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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abstract = "The Clkk curves displayed in Fig. 1 were computed using Eq. (1), with the form of Pm(k,z) given by Eq. (3). Our numerical implementation of this computation contained an error that affected these curves and the other results derived from them. In addition, there was a separate error that only affected the matter power spectra from the IllustrisTNG300 simulation and the associated Clkk computation1.",

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AU - Foreman, Simon

AU - Van Engelen, Alexander

PY - 2020/11/25

Y1 - 2020/11/25

N2 - The Clkk curves displayed in Fig. 1 were computed using Eq. (1), with the form of Pm(k,z) given by Eq. (3). Our numerical implementation of this computation contained an error that affected these curves and the other results derived from them. In addition, there was a separate error that only affected the matter power spectra from the IllustrisTNG300 simulation and the associated Clkk computation1.

AB - The Clkk curves displayed in Fig. 1 were computed using Eq. (1), with the form of Pm(k,z) given by Eq. (3). Our numerical implementation of this computation contained an error that affected these curves and the other results derived from them. In addition, there was a separate error that only affected the matter power spectra from the IllustrisTNG300 simulation and the associated Clkk computation1.

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Erratum: Baryonic effects on CMB lensing and neutrino mass constraints (Physical Review D (2020) 101 (063534) DOI: 10.1103/PhysRevD.101.063534)

Abstract

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