Impact of Simulation Box Size for Weak Lensing: Replication and Super-Sample Effects

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Main Authors: Tokiwa, Akira, Bayer, Adrian E., Armijo, Joaquin, Liu, Jia, Terasawa, Ryo, Thiele, Leander, Alvarez, Marcelo, Blot, Linda, Takada, Masahiro
Format: Preprint
Published: 2025
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author Tokiwa, Akira
Bayer, Adrian E.
Armijo, Joaquin
Liu, Jia
Terasawa, Ryo
Thiele, Leander
Alvarez, Marcelo
Blot, Linda
Takada, Masahiro
author_facet Tokiwa, Akira
Bayer, Adrian E.
Armijo, Joaquin
Liu, Jia
Terasawa, Ryo
Thiele, Leander
Alvarez, Marcelo
Blot, Linda
Takada, Masahiro
contents We quantify the bias caused by small simulation box size on weak lensing observables and covariances, considering both replication and super-sample effects for a range of higher-order statistics. Using two simulation suites -- one comprising large boxes ($3750\,h^{-1}{\rm Mpc}$) and another constructed by tiling small boxes ($625\,h^{-1}{\rm Mpc}$) -- we generate full-sky convergence maps and extract $10^\circ \times 10^\circ$ patches via a Fibonacci grid. We consider biases in the mean and covariance of the angular power spectrum, bispectrum (up to $\ell=3000$), PDF, peak/minima counts, and Minkowski functionals. By first identifying lines of sight that are impacted by replications, we find that replication causes a O$(10\%)$ bias in the PDF and Minkowski functionals, and a O$(1\%)$ bias in other summary statistics. Replication also causes a O$(10\%)$ bias in the covariances, increasing with source redshift and $\ell$, reaching $\sim25\%$ for $z_s=2.5$. We additionally show that replication leads to heavy biases (up to O$(100\%)$ at high redshift) when performing gnomonic projection on a patch that is centered along a direction of replication. We then identify the lines of sight that are minimally affected by replication, and use the corresponding patches to isolate and study super-sample effects, finding that, while the mean values agree to within $1\%$, the variances differ by O$(10\%)$ for $z_s\leq2.5$. We show that these effects remain in the presence of noise and smoothing scales typical of the DES, KiDS, HSC, LSST, Euclid, and Roman surveys. We also discuss how these effects scale as a function of box size. Our results highlight the importance of large simulation volumes for accurate lensing statistics and covariance estimation.
format Preprint
id arxiv_https___arxiv_org_abs_2511_20423
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Impact of Simulation Box Size for Weak Lensing: Replication and Super-Sample Effects
Tokiwa, Akira
Bayer, Adrian E.
Armijo, Joaquin
Liu, Jia
Terasawa, Ryo
Thiele, Leander
Alvarez, Marcelo
Blot, Linda
Takada, Masahiro
Cosmology and Nongalactic Astrophysics
We quantify the bias caused by small simulation box size on weak lensing observables and covariances, considering both replication and super-sample effects for a range of higher-order statistics. Using two simulation suites -- one comprising large boxes ($3750\,h^{-1}{\rm Mpc}$) and another constructed by tiling small boxes ($625\,h^{-1}{\rm Mpc}$) -- we generate full-sky convergence maps and extract $10^\circ \times 10^\circ$ patches via a Fibonacci grid. We consider biases in the mean and covariance of the angular power spectrum, bispectrum (up to $\ell=3000$), PDF, peak/minima counts, and Minkowski functionals. By first identifying lines of sight that are impacted by replications, we find that replication causes a O$(10\%)$ bias in the PDF and Minkowski functionals, and a O$(1\%)$ bias in other summary statistics. Replication also causes a O$(10\%)$ bias in the covariances, increasing with source redshift and $\ell$, reaching $\sim25\%$ for $z_s=2.5$. We additionally show that replication leads to heavy biases (up to O$(100\%)$ at high redshift) when performing gnomonic projection on a patch that is centered along a direction of replication. We then identify the lines of sight that are minimally affected by replication, and use the corresponding patches to isolate and study super-sample effects, finding that, while the mean values agree to within $1\%$, the variances differ by O$(10\%)$ for $z_s\leq2.5$. We show that these effects remain in the presence of noise and smoothing scales typical of the DES, KiDS, HSC, LSST, Euclid, and Roman surveys. We also discuss how these effects scale as a function of box size. Our results highlight the importance of large simulation volumes for accurate lensing statistics and covariance estimation.
title Impact of Simulation Box Size for Weak Lensing: Replication and Super-Sample Effects
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2511.20423