The Accuracy of Weak Lensing Simulations
arXiv:1910.10625 · doi:10.1093/mnras/staa281
Abstract
We investigate the accuracy of weak lensing simulations by comparing the results of five independently developed lensing simulation codes run on the same input -body simulation. Our comparison focuses on the lensing convergence maps produced by the codes, and in particular on the corresponding PDFs, power spectra and peak counts. We find that the convergence power spectra of the lensing codes agree to out to scales . For lensing peak counts, the agreement is better than for peaks with signal-to-noise . We also discuss the systematic errors due to the Born approximation, line-of-sight discretization, particle noise and smoothing. The lensing codes tested deal in markedly different ways with these effects, but they nonetheless display a satisfactory level of agreement. Our results thus suggest that systematic errors due to the operation of existing lensing codes should be small. Moreover their impact on the convergence power spectra for a lensing simulation can be predicted given its numerical details, which may then serve as a validation test.
arXiv comment16 pages, 10 figures; comments welcomed! In v2: minor clarifications added; matches version published in MNRAS
References in corpus (112)
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Efficient Computation of CMB anisotropies in closed FRW models
- Weak Gravitational Lensing
- Stable clustering, the halo model and nonlinear cosmological power spectra
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- An All-Sky Analysis of Polarization in the Microwave Background
- Revising the Halofit Model for the Nonlinear Matter Power Spectrum
- Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
- KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
- Statistics of Cosmic Microwave Background Polarization
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
- Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
- Cosmology with cosmic shear observations: a review
- The Aquila comparison Project: The Effects of Feedback and Numerical Methods on Simulations of Galaxy Formation
- Weak Lensing of the CMB: A Harmonic Approach
- Haloes gone MAD: The Halo-Finder Comparison Project
- Weak lensing for precision cosmology
- Compound gravitational lensing as a probe of dark matter substructure within galaxy halos
- Reconstruction of lensing from the cosmic microwave background polarization
- KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data
- Transients from Initial Conditions: A Perturbative Analysis
- Ray-tracing through the Millennium Simulation: Born corrections and lens-lens coupling in cosmic shear and galaxy-galaxy lensing
- Ray Tracing Simulations of Weak Lensing by Large-Scale Structure
- Quantifying the effect of baryon physics on weak lensing tomography
- Quantitative Interpretation of Quasar Microlensing Light Curves
- Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
- The Frontier Fields Lens Modeling Comparison Project
- PINOCCHIO: pinpointing orbit-crossing collapsed hierarchical objects in a linear density field
- The Aspen--Amsterdam Void Finder Comparison Project
- The MICE Grand Challenge Lightcone Simulation III: Galaxy lensing mocks from all-sky lensing maps
- SubHaloes going Notts: The SubHalo-Finder Comparison Project
- Cosmology with the shear-peak statistics
- Improving lognormal models for cosmological fields
- Matter power spectrum and the challenge of percent accuracy
- Rejuvenating the matter power spectrum: restoring information with a logarithmic density mapping
- Cosmology Constraints from the Weak Lensing Peak Counts and the Power Spectrum in CFHTLenS
- A New Algorithm for Computing Statistics of Weak Lensing by Large-Scale Structure
- Weak lensing analysis in three dimensions
- The onion universe: all sky lightcone simulations in spherical shells
- Strong lensing optical depths in a \LambdaCDM universe
- Modified Gravity N-body Code Comparison Project
- Precision calculations of the cosmic shear power spectrum projection
- Second Order Corrections to Weak Lensing by Large-Scale Structure
- How well can cold-dark-matter substructures account for the observed radio flux-ratio anomalies?
- Modelling the line-of-sight contribution in substructure lensing
- Sussing Merger Trees: The Merger Trees Comparison Project
- Simulating weak lensing by large scale structure
- Weak lensing power spectra for precision cosmology: Multiple-deflection, reduced shear and lensing bias corrections
- Modeling baryonic physics in future weak lensing surveys
- Effects of Dark Matter Substructures on Gravitational Lensing: Results from the Aquarius Simulations
- Impact of post-Born lensing on the CMB
- KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics-I: Inference from Analytical Prediction of High Signal-to-Noise Ratio Convergence Peaks
- Strong lensing optical depths in a LCDM universe II: the influence of the stellar mass in galaxies
- The mass-Peak Patch algorithm for fast generation of deep all-sky dark matter halo catalogues and its N-Body validation
- Effects of cluster galaxies on arc statistics
- The impact of gas physics on strong cluster lensing
- Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
- Comparing approximate methods for mock catalogues and covariance matrices I: correlation function
- Constraining Gravity Theory Using Weak Lensing Peak Statistics from the Canada-France-Hawaii-Telescope Lensing Survey
- nIFTy Cosmology: Galaxy/halo mock catalogue comparison project on clustering statistics
- Numerical study of statistical properties of the lensing excursion angles
- Comparing approximate methods for mock catalogues and covariance matrices III: Bispectrum
- Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory
- CMB weak-lensing beyond the Born approximation: a numerical approach
- On the validity of the Born approximation for beyond-Gaussian weak lensing observables
- GLAMER Part I: A Code for Gravitational Lensing Simulations with Adaptive Mesh Refinement
- Cosmological constraints from the CFHTLenS shear measurements using a new, accurate and flexible way of predicting nonlinear mass clustering
- Fast Spherical Harmonic Analysis: a quick algorithm for generating and/or inverting full sky, high resolution CMB Anisotropy maps
- GLAMER Part II: Multiple Plane Gravitational Lensing
- Imprints of relativistic effects on the asymmetry of the halo cross-correlation function: from linear to non-linear scales
- CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
- Gravitational Lensing Simulations I : Covariance Matrices and Halo Catalogues
- Mocking the Weak Lensing universe: the LensTools python computing package
- MOKA: a new tool for Strong Lensing Studies
- The Lensed Arc Production Efficiency of Galaxy Clusters: A Comparison of Matched Observed and Simulated Samples
- The Born and Lens-Lens Corrections to Weak Gravitational Lensing Angular Power Spectra
- A Large Sky Simulation of the Gravitational Lensing of the Cosmic Microwave Background
- Cluster strong lensing in the Millennium Simulation: The effect of galaxies and structures along the line-of-sight
- Full-sky maps for gravitational lensing of the CMB
- Optimized detection of shear peaks in weak lensing maps
- CMB-lensing beyond the Born approximation
- Re-capturing cosmic information
- Sample variance in weak lensing: how many simulations are required?
- Galaxies going MAD: The Galaxy-Finder Comparison Project
- Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
- The effect of baryons in the cosmological lensing PDFs
- Measuring the three-dimensional shear from simulation data, with applications to weak gravitational lensing
- SUNGLASS: A new weak lensing simulation pipeline
- Measuring primordial non-Gaussianity with weak-lensing surveys
- Weak Lensing Observables in the Halo Model
- Streams Going Notts: The tidal debris finder comparison project
- Magnification Bias Corrections to Galaxy-Lensing Cross-Correlations
- MultiDarkLens Simulations: weak lensing light-cones and data base presentation
- Scale dependence of galaxy biasing investigated by weak gravitational lensing: An assessment using semi-analytic galaxies and simulated lensing data
- Systematic Effects on Tangential and Radial Arc Statistics: The Finite Source Size and Ellipticities of the Lens and Source
- Effect of lensing non-Gaussianity on the CMB power spectra
- ICE-COLA: fast simulations for weak lensing observables
- Disentangling dark sector models using weak lensing statistics
- Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects
- Fast Weak Lensing Simulations with Halo Model
- Lensed CMB temperature and polarization maps from the Millennium Simulation
- Lensed arc statistics: comparison of Millennium-simulation galaxy clusters to Hubble Space Telescope observations of an X-ray selected sample
- Multiple Lensing of the Cosmic Microwave Background anisotropies
- Weak Lensing Peaks in Simulated Light-Cones: Investigating the Coupling between Dark Matter and Dark Energy
- High precision simulations of weak lensing effect on Cosmic Microwave Background polarization
- A Semi-analytic Ray-tracing Algorithm for Weak Lensing
- RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
- Dark Energy from the log-transformed convergence field
- Removing BAO-peak Shifts with Local Density Transforms
- General Relativistic corrections in density-shear correlations
- The self similarity of weak lensing peaks
- Weighted density fields as improved probes of modified gravity models
Cited by in corpus (32)
- Euclid. I. Overview of the Euclid mission
- Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
- Nuw CDM cosmology from the weak lensing convergence PDF
- Euclid Preparation. XXVIII. Forecasts for ten different higher-order weak lensing statistics
- Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
- On the road to percent accuracy V: the non-linear power spectrum beyond CDM with massive neutrinos and baryonic feedback
- Weak-lensing observables in relativistic N-body simulations
- The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
- DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
- The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
- DEMNUni: The imprint of massive neutrinos on the cross-correlation between cosmic voids and CMB lensing
- Probability distribution function of the aperture mass field with large deviation theory
- Comparison of delensing methodologies and assessment of the delensing capabilities of future experiments
- Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
- Cosmological forecasts with the clustering of weak lensing peaks
- The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts
- Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
- Estimating the Integrated Bispectrum from Weak Lensing Maps
- Box Replication Effects in Weak Lensing Light-cone Construction
- Fast estimation of aperture-mass statistics I: aperture mass variance and an application to the CFHTLenS data
- Baryonification extended to thermal Sunyaev Zeldovich
- DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
- Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in -body simulations
- Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
- Accurate relativistic observables from post-processing light cone catalogues
- Weak-lensing tunnel voids in simulated light cones: A new pipeline to investigate modified gravity and massive neutrinos signatures
- Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
- The FLAMINGO project: cosmology with the redshift dependence of weak gravitational lensing peaks
- A deconstruction of methods to derive one-point lensing statistics
- AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
- A Hamiltonian, post-Born, three-dimensional, on-the-fly ray tracing algorithm for gravitational lensing
- Solving small-scale clustering problems in approximate lightcone mocks