Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

Abstract

We measure cosmic weak lensing shear power spectra with the Subaru Hyper Suprime-Cam (HSC) survey first-year shear catalog covering 137deg${}^2$ of the sky. Thanks to the high effective galaxy number density of $\sim$17 arcmin${}^{-2}$ even after conservative cuts such as magnitude cut of $i<24.5$ and photometric redshift cut of $0.3\le z\le 1.5$, we obtain a high significance measurement of the cosmic shear power spectra in 4 tomographic redshift bins, achieving a total signal-to-noise ratio of 16 in the multipole range $300\le \ell \le 1900$. We carefully account for various uncertainties in our analysis including the intrinsic alignment of galaxies, scatters and biases in photometric redshifts, residual uncertainties in the shear measurement, and modeling of the matter power spectrum. The accuracy of our power spectrum measurement method as well as our analytic model of the covariance matrix are tested against realistic mock shear catalogs. For a flat $\Lambda$ cold dark matter ($\Lambda$CDM) model, we find $S_8\equiv {\sigma }_8({\Omega }_{\mathrm{m}}/0.3{)}^{\alpha }=0.800_{-0.028}^{+0.029}$ for $\alpha =0.45$ ($S_8=0.780_{-0.033}^{+0.030}$ for $\alpha =0.5$) from our HSC tomographic cosmic shear analysis alone. In comparison with Planck cosmic microwave background constraints, our results prefer slightly lower values of $S_8$, although metrics such as the Bayesian evidence ratio test do not show significant evidence for discordance between these results. We study the effect of possible additional systematic errors that are unaccounted in our fiducial cosmic shear analysis, and find that they can shift the best-fit values of $S_8$ by up to $\sim 0.6\sigma$ in both directions. The full HSC survey data will contain several times more area, and will lead to significantly improved cosmological constraints.

arXiv comment43 pages, 21 figures, accepted for publication in PASJ

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• KaRMMa -- Kappa Reconstruction for Mass Mapping
• Probing Cosmology and Cluster Astrophysics with Multi-Wavelength Surveys I. Correlation Statistics
• Redshift requirements for cosmic shear with intrinsic alignment
• Consistency of cosmic shear analyses in harmonic and real space
• Self-calibration and robust propagation of photometric redshift distribution uncertainties in weak gravitational lensing
• Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• The Impact of Line Misidentification on Cosmological Constraints from Euclid and other Spectroscopic Galaxy Surveys
• Probing Modified Gravity with Integrated Sachs-Wolfe CMB and Galaxy Cross-correlations
• Cascading Dark Energy
• Multicomponent multiscatter capture of Dark Matter
• Clustering dark energy imprints on cosmological observables of the gravitational field
• Weak lensing clusters from HSC survey first-year data: Mitigating the dilution effect of foreground and cluster member galaxies
• Impact of baryons in cosmic shear analyses with tomographic aperture mass statistics
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Enhancing cosmic shear with the multi-scale lensing PDF
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• A Faster Fourier Transform? Computing Small-Scale Power Spectra and Bispectra for Cosmological Simulations in $\mathcal{O}(N^2)$ Time
• Localizing Transformations of the Galaxy-Galaxy Lensing Observable
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• A Model of Interacting Dark Matter and Dark Radiation for $H_0$ and ${\sigma }_8$ Tensions
• Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• The effects of varying depth in cosmic shear surveys
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Galaxy morphoto-Z with neural Networks (GaZNets). I. Optimized accuracy and outlier fraction from Imaging and Photometry
• Mitigating the effects of undersampling in weak lensing shear estimation with metacalibration
• Cosmology from weak lensing alone and implications for the Hubble tension
• Higher order statistics of shear field: a machine learning approach
• Observable Predictions for Massive-Neutrino Cosmologies with Model-Independent Dark Energy
• Sufficiency of a Gaussian power spectrum likelihood for accurate cosmology from upcoming weak lensing surveys
• Towards a full $w$CDM map-based analysis for weak lensing surveys
• A comparative study of cosmological constraints from weak lensing using Convolutional Neural Networks
• Evolution mapping: a new approach to describe matter clustering in the non-linear regime
• A Composite Likelihood Approach for Inference under Photometric Redshift Uncertainty
• Early dark energy by dark Higgs, and axion-induced non-thermal trapping
• Fast estimation of aperture mass statistics II: Detectability of higher order statistics in current and future surveys
• Nature of supersonic turbulence and density distribution function in the multiphase interstellar medium
• DESI Legacy Imaging Surveys Data Release 9: Cosmological Constraints from Galaxy Clustering and Weak Lensing using the Minimal Bias Model
• Cosmological constraints from weak lensing scattering transform using HSC Y1 data
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• KiDS-1000: cross-correlation with Planck cosmic microwave background lensing and intrinsic alignment removal with self-calibration
• Shear Measurement with Poorly Resolved Images
• Cosmological forecasts with the clustering of weak lensing peaks
• The Halo Spin Transition as a Probe of Dark Energy
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Towards a Bias-Free Selection Function in Shear Measurement
• Deconstructing the Planck TT Power Spectrum to Constrain Deviations from $\Lambda$CDM
• Cosmological bound on neutrino masses in the light of $H_0$ tension
• SuperCLASS -- III. Weak lensing from radio and optical observations in Data Release 1
• Exploring Mirror Twin Higgs Cosmology with Present and Future Weak Lensing Surveys
• Altered Axion Abundance from a Dynamical Peccei-Quinn Scale
• Cosmological Probes of Structure Growth and Tests of Gravity
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• Cosmological evolution of viable models in the generalized scalar-tensor theory
• Accelerating cosmological inference with Gaussian processes and neural networks -- an application to LSST Y1 weak lensing and galaxy clustering
• The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing
• A roadmap to cosmological parameter analysis with third-order shear statistics III: Efficient estimation of third-order shear correlation functions and an application to the KiDS-1000 data
• Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables
• A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
• Role of the Hubble Scale in the Weak Lensing vs. CMB Tension
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• Cosmological constraints using Minkowski functionals from the first year data of the Hyper Suprime-Cam
• An empirical approach to model selection: weak lensing and intrinsic alignments
• Simulating image coaddition with the Nancy Grace Roman Space Telescope: I. Simulation methodology and general results
• Effects of galaxy intrinsic alignment on weak lensing peak statistics
• Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies
• Deep+Wide Lensing Surveys will Provide Exquisite Measurements of the Dark Matter Halos of Dwarf Galaxies
• Brighter-fatter effect in near-infrared detectors -- III. Fourier-domain treatment of flat field correlations and application to WFIRST
• Reconstructing Probability Distributions with Gaussian Processes
• Status of the $S_8$ Tension: A 2026 Review of Probe Discrepancies
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• Separating the Intrinsic Alignment Signal and the Lensing Signal using Self-Calibration in Photo-z Surveys with KiDS450 and KV450 Data
• Early dark energy constraints with late-time expansion marginalization
• Baryonic feedback measurement from KV450 cosmic shear analysis
• Searching for eV-mass Axion-like Particles with Cross Correlations between Line Intensity and Weak Lensing Maps
• Cosmological Constraints from Weak Lensing Peaks: Can Halo Models Accurately Predict Peak Counts?
• Euclid: Covariance of weak lensing pseudo-$C_{\ell }$ estimates. Calculation, comparison to simulations, and dependence on survey geometry
• The miniJPAS survey quasar selection II: Machine learning classification with photometric measurements and uncertainties
• Exact joint likelihood of pseudo-$C_{\ell }$ estimates from correlated Gaussian cosmological fields
• Conformally and Disformally Coupled Vector field Models of Dark Energy
• Euclid preparation. LIII. LensMC, weak lensing cosmic shear measurement with forward modelling and Markov Chain Monte Carlo sampling
• Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
• Quantum yield and charge diffusion in the Nancy Grace Roman Space Telescope infrared detectors
• Signatures of Light Massive Relics on nonlinear structure formation
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• Cosmological Model Parameter Dependence of the Matter Power Spectrum Covariance from the DEUS-PUR $Cosmo$ Simulations
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Gravitino Cosmology Helped by a Right Handed (S)Neutrino
• Dark Matter Cosmology with Varying Viscosity: a Possible Resolution to the $S_8$ Tension
• Galaxy Deblending using Residual Dense Neural networks
• Weak-lensing Mass Reconstruction of Galaxy Clusters with Convolutional Neural Network
• Constraining $f(R)$ Gravity with a $k$-cut Cosmic Shear Analysis of the Hyper Suprime-Cam First-Year Data
• The integrated angular bispectrum of weak lensing
• Avoiding the Geometric Boundary Effect in Shear Measurement
• Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- I. Constraining physical processes in local star-forming galaxies
• Mitigating the Noise-Source Coupling Effect in Shear Measurement
• Forecast of cross-correlation of CSST cosmic shear tomography with AliCPT-1 CMB lensing
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Interpreting Internal Consistency of DES Measurements
• A field-level emulator for modeling baryonic effects across hydrodynamic simulations
• Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
• Improving the astrometric solution of the Hyper Suprime-Cam with anisotropic Gaussian processes
• A roadmap to cosmological parameter analysis with third-order shear statistics II: Analytic covariance estimate
• Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure
• Mass-varying Dark Matter from a Phase Transition
• Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample
• PhoSim-NIRCam: Photon-by-photon image simulations of the James Webb Space Telescope's Near-Infrared Camera
• Cosmological studies from tomographic weak lensing peak abundances and impacts of photo-z errors
• Fast estimation of aperture-mass statistics I: aperture mass variance and an application to the CFHTLenS data
• Euclid preparation. LIX. Angular power spectra from discrete observations
• Mitigating baryonic effects with a theoretical error covariance
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Constraining the growth rate of structure with phase correlations
• The DAMIC-M Low Background Chamber
• Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol
• Chameleon Early Dark Energy and the Hubble Tension
• Limit on the dark matter mass from its interaction with photons
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• What is the super-sample covariance? A fresh perspective for second-order shear statistics
• E/B mode decomposition of HSC-Y1 cosmic shear using COSEBIs: cosmological constraints and comparison with other two-point statistics
• Simulating image coaddition with the Nancy Grace Roman Space Telescope: III. Software improvements and new linear algebra strategies
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• SuperCLASS -- I. The Super CLuster Assisted Shear Survey: Project overview and Data Release 1
• Accurate Kappa Reconstruction Algorithm for masked shear catalog (AKRA)
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• Equality scale-based and sound horizon-based analysis of the Hubble tension
• Quasi-2D Weak Lensing Cosmological Constraints Using the PDF-SYM method
• Ray-tracing log-normal simulation for weak gravitational lensing: application to the cross-correlation with galaxies
• Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential. Effect of the redshift bin mismatch
• Improved Weak Lensing Photometric Redshift Calibration via StratLearn and Hierarchical Modeling
• Impact of cosmological signatures in two-point statistics beyond the linear regime
• Testing Quadratic Maximum Likelihood estimators for forthcoming Stage-IV weak lensing surveys
• Radio-Optical Galaxy Shape and Shear Correlations in the COSMOS Field using 3 GHz VLA Observations
• Impact of the primordial fluctuation power spectrum on the reionization history
• Subaru Telescope -- History, Active/Adaptive Optics, Instruments, and Scientific Achievements
• Covariances of density probability distribution functions. Lessons from hierarchical models
• The matter fluctuation amplitude inferred from the weak lensing power spectrum and correlation function in CFHTLenS data
• Kinematic Lensing with the Roman Space Telescope
• The Impact of Light Polarization Effects on Weak Lensing Systematics
• High-Significance Detection of Correlation Between the Unresolved Gamma-Ray Background and the Large Scale Cosmic Structure
• A test for the redshift dependence of ${\sigma }_8$ using $f{\sigma }_8$ measurements
• Reconstruction of weak lensing mass maps for non-Gaussian studies in the celestial sphere
• A Framework for Measuring Weak-Lensing Magnification Using the Fundamental Plane
• Weak Lensing Constraints on Dark Matter-Baryon Interactions with $N$-Body Simulations and Machine Learning
• AMICO galaxy clusters in KiDS-DR3: constraints on $\Lambda$CDM from extreme value statistics
• Fast simulation mapping: from standard to modified gravity cosmologies using the bias assignment method
• Proca-stinated Cosmology II: Matter, Halo, and Lensing Statistics in the vector Galileon
• Cool dark sector, concordance, and a low ${\sigma }_8$
• Euclid: Photometric redshift calibration with self-organising maps
• Blending and obscuration in weak lensing magnification
• AKRA 2.0: Accurate Kappa Reconstruction Algorithm for masked shear catalog
• Knowing when to stop
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• Optimizing Redshift Distribution Inference through Joint Self-Calibration and Clustering-Redshift Synergy
• Mapping Variations of Redshift Distributions with Probability Integral Transforms
• Effect of lensing magnification on type Ia supernova cosmology
• Weak lensing peak statistics -- steepness versus height
• FPFS Shear Estimator: Systematic Tests on the Hyper Suprime-Cam Survey First Year Data
• Measuring the gravitomagnetic distortion from rotating halos I: methods
• Cosmology of Single Species Hidden Dark Matter
• The density profile of Milky Way dark matter halo constrained from the OGLE microlensing sky map
• Quantum Statistical Effects on Warm Dark Matter and the Mass Constraint from the Cosmic Structure at Small Scales
• 6x2pt: Forecasting gains from joint weak lensing and galaxy clustering analyses with spectroscopic-photometric galaxy cross-correlations
• Detecting Modeling Bias with Continuous Time Flow Models on Weak Lensing Maps
• Accounting for Correlations When Fitting Extra Cosmological Parameters
• Cosmological consequences of intrinsic alignments super-sample covariance
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
• The Impact of Tomographic Redshift Bin Width Errors on Cosmological Probes
• Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures
• Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
• Supermassive Dark Stars and their remnants as a possible solution to three recent cosmic dawn puzzles
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• Decaying Dark Matter: Simulations and Weak-Lensing Forecast
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles
• Constraining cosmology with N-body simulations for future spectroscopic galaxy surveys at $2\le z\le 3$
• Cosmic shear beyond 2-point statistics: Accounting for galaxy intrinsic alignment with projected tidal fields
• Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
• Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
• Effect of dust in circumgalactic haloes on the cosmic shear power spectrum
• Cross-correlations between mm-wave line-intensity mapping and weak lensing surveys: preliminary consideration of long-term prospects
• A Novel Framework for Modeling Weakly Lensing Shear Using Kinematics and Imaging at Moderate Redshift
• Superhorizon isocurvature fluctuations relax tensions
• The Covariance of Photometric and Spectroscopic Two-Point Statistics: Implications for Cosmological Parameter Inference
• Dark Energy Survey Year 3 Results: Three-Point Shear Correlations and Mass Aperture Moments
• Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• Large-scale structure with superhorizon isocurvature dark energy
• $S_8$ from peculiar velocities: agreement with Planck for Tully--Fisher and supernovae, tension for the fundamental plane
• Replicating weak-lensing summary-statistic covariances with normalizing flows
• Scaling pair count to next galaxy surveys
• Encyclopedia of Astrophysics: The Expanding Universe
• Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
• CMB lensing tomography with clustering estimation of lens redshift distributions
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• Euclid: Optimising tomographic redshift binning for 3$\times$2pt power spectrum constraints on dark energy
• Cosmic Shear in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Configuration Space Results
• Non-Gaussian likelihood of weak lensing power spectra
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field