First Data Release of the Hyper Suprime-Cam Subaru Strategic Program

Abstract

The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most outstanding questions in astronomy today, including the nature of dark matter and dark energy. The survey has been awarded 300 nights of observing time at the Subaru Telescope and it started in March 2014. This paper presents the first public data release of HSC-SSP. This release includes data taken in the first 1.7 years of observations (61.5 nights) and each of the Wide, Deep, and UltraDeep layers covers about 108, 26, and 4 square degrees down to depths of i~26.4, ~26.5, and ~27.0 mag, respectively (5sigma for point sources). All the layers are observed in five broad bands (grizy), and the Deep and UltraDeep layers are observed in narrow bands as well. We achieve an impressive image quality of 0.6 arcsec in the i-band in the Wide layer. We show that we achieve 1-2 per cent PSF photometry (rms) both internally and externally (against Pan-STARRS1), and ~10 mas and 40 mas internal and external astrometric accuracy, respectively. Both the calibrated images and catalogs are made available to the community through dedicated user interfaces and database servers. In addition to the pipeline products, we also provide value-added products such as photometric redshifts and a collection of public spectroscopic redshifts. Detailed descriptions of all the data can be found online. The data release website is https://hsc-release.mtk.nao.ac.jp/.

34 pages, 20 figures, 7 tables, moderate revision, accepted for publication in PASJ

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• The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Understanding X-ray and optical selection of galaxy clusters: A comparison of the XXL and CAMIRA cluster catalogues obtained in the common XXL-HSC SSP area
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• Measurement of redshift dependent cross correlation of HSC clusters and Fermi $\gamma$ rays
• RELICS: ICL Analysis of the $z=0.566$ merging cluster WHL J013719.8-08284
• Detection of Cosmic Magnification via Galaxy Shear -- Galaxy Number Density Correlation from HSC Survey Data
• The eROSITA Final Equatorial-Depth Survey (eFEDS): A complete census of X-ray properties of Subaru Hyper Suprime-Cam weak lensing shear-selected clusters in the eFEDS footprint
• The Infrared Medium-deep Survey. \Romannum{7}. Faint Quasars at $z\sim 5$ in the ELAIS-N1 Field
• A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
• HEROES: The Hawaii eROSITA Ecliptic Pole Survey Catalog
• The whole picture of the large-scale structure of the CL1604 supercluster at z$\sim$0.9
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• Brightest Cluster Galaxies Are Statistically Special From $z=0.3$ to $z=1$
• Impact of Point Spread Function Higher Moments Error on Weak Gravitational Lensing II: A Comprehensive Study
• Discovery of an unusually compact lensed Lyman Break Galaxy from the Hyper Suprime-Cam Survey
• Searching for Moving Objects in HSC-SSP: Pipeline and Preliminary Results
• Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field
• LOFAR Deep Fields: Probing a broader population of polarized radio galaxies in ELAIS-N1
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• ALMA resolves the first strongly-lensed Optical/NIR-dark galaxy
• Hyper Suprime-Cam Legacy Archive
• GaMPEN: A Machine Learning Framework for Estimating Bayesian Posteriors of Galaxy Morphological Parameters
• The eROSITA Final Equatorial-Depth Survey (eFEDS): The first archetypal Quasar in the feedback phase discovered by eROSITA
• Discovery of Strongly Lensed Quasars in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS)
• Optical follow-up observation for GW event S190510g using Subaru/Hyper Suprime-Cam
• Photometric classification of HSC transients using machine learning
• HOLISMOKES -- XI. Evaluation of supervised neural networks for strong-lens searches in ground-based imaging surveys
• CHORUS IV: Mapping the Spatially Inhomogeneous Cosmic Reionization with Subaru HSC
• Gaussian Process Classification for Galaxy Blend Identification in LSST
• Euclid preparation. LIII. LensMC, weak lensing cosmic shear measurement with forward modelling and Markov Chain Monte Carlo sampling
• Photometric Redshifts in the North Ecliptic Pole Wide Field based on a Deep Optical Survey with Hyper Suprime-Cam
• OpenUniverse2024: A shared, simulated view of the sky for the next generation of cosmological surveys
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed by High-z Radio Galaxies at z~4
• The HI Bias during the Epoch of Reionization
• Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space
• A Bayesian Approach to Strong Lens Finding in the Era of Wide-area Surveys
• The eROSITA Final Equatorial-Depth Survey (eFEDS) -- Splashback radius of X-ray galaxy clusters using galaxies from HSC survey
• Multi-band Photometry of Trans-Neptunian Objects in the Subaru Hyper Suprime-Cam Survey
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VII. Redshift Evolution of Radio Galaxy Environments at z=0.3-1.4
• The XXL Survey XLIV. Sunyaev-Zel'dovich mapping of a low-mass cluster at z~1: a multi-wavelength approach
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• High redshift LBGs from deep broadband imaging for future spectroscopic surveys
• Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data
• A deep radio view of the evolution of the cosmic star-formation rate density from a stellar-mass selected sample in VLA-COSMOS
• A Search for L4 Earth Trojan Asteroids Using a Novel Track-Before-Detect Multi-Epoch Pipeline
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• Understanding the chemical evolution of blue Edge-on Low Surface Brightness Galaxies
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Subaru Hyper Suprime-Cam Survey of Cygnus OB2 Complex -- I: Introduction, Photometry and Source Catalog
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• Evaluation of the Vertical Scale Height of L dwarfs in the Galactic Thin Disk
• Forklens: Accurate weak-lensing shear measurement with deep learning
• Search for Brown Dwarfs in IC 1396 with Subaru HSC: Interpreting the Impact of Environmental Factors on Sub-stellar Population
• Proper motion measurements for stars up to $100$ kpc with Subaru HSC and SDSS Stripe 82
• HSC-XD 52: An X-ray detected AGN in a low-mass galaxy at $z\sim 0.56$
• GALFIT-ing AGN Host Galaxies in COSMOS: HST vs. Subaru
• The nature of H$\alpha$-selected galaxies along the large-scale structure at z=0.4 revealed by Subaru Hyper Suprime-Cam survey
• Cosmological evolution of orientations of cluster-sized dark matter haloes and their central galaxies in the Horizon-AGN simulation
• Joint Survey Processing I: Compact oddballs in the COSMOS field -- low-luminosity Quasars at z > 6?
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Evolution of the galaxy merger fraction in the CLAUDS+HSC-SSP deep fields
• Faint Quasars Live in the Same Number Density Environments as Lyman Break Galaxies at z ~ 4
• Cosmic shear calibration with forward modeling
• X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field
• Multi-band Optical and Near-infrared Properties of Faint Submillimeter Galaxies with Serendipitous ALMA Detections
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• eROSITA Final Equatorial-Depth Survey (eFEDS): eFEDS X-ray view of WERGS Radio Galaxies selected by the Subaru/HSC and VLA/FIRST survey
• Searches for Population III Pair-Instability Supernovae: Impact of Gravitational Lensing Magnification
• Testing an indirect method for identifying galaxies with high levels of Lyman continuum leakage
• Constraining dark matter annihilation with HSC Low Surface Brightness Galaxies
• 1-arcsecond imaging of ELAIS-N1 field at 144MHz using the LoTSS survey with international LOFAR telescope
• SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation
• High Star Formation Rates of Low Eddington Ratio Quasars at $z\gtrsim 6$
• Constraints on the rate of supernovae lasting for more than a year from Subaru/Hyper Suprime-Cam
• Star Formation Properties of Sloan Digital Sky Survey BOSS Void Galaxies in the Hyper Suprime-Cam Survey
• Scaling relations of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program Field
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• The XXL survey: XLII. Detection and characterization of the galaxy population of distant galaxy clusters in the XXL-N/VIDEO field: A tale of variety
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• Kinematics of disk galaxies in (proto-)clusters at z=1.5
• Star Formation in Massive Galaxies at Redshift $z\sim 0.5$
• A deep analysis for New Horizons' KBO search images
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• A robust two-parameter description of the stellar profile of elliptical galaxies
• LOFAR properties of SILVERRUSH Ly$\alpha$ emitter candidates in the ELAIS-N1 field
• Beyond Mass: Detecting Secondary Halo Properties with Galaxy-Galaxy Lensing
• Galaxy clusters at z~1 imaged by ALMA with the Sunyaev-Zel'dovich effect
• Cluster candidates with massive quiescent galaxies at $z\sim 2$
• Tests of photometry: the case of the NGC 3370 ACS field
• The Weak Lensing Peak Statistics in the Mocks by the inverse-Gaussianization Method
• Renormalization group and UV completion of cosmological perturbations: Gravitational collapse as a critical phenomenon
• Photometric redshift estimation of strongly lensed galaxies
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• A new observable for cosmic shear
• E/B mode decomposition of HSC-Y1 cosmic shear using COSEBIs: cosmological constraints and comparison with other two-point statistics
• A Ghost in Boötes: The Least Luminous Disrupted Dwarf Galaxy
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IX. The Most Overdense Region at z~5 Inhabited by a Massive Radio Galaxy
• Radio emission from dust-obscured galaxies
• High-$z$ Universe probed via Lensing by QSOs (HULQ) I. Number Estimates of QSO-QSO and QSO-Galaxy Lenses
• The SAMI Galaxy Survey: rules of behaviour for spin-ellipticity radial tracks in galaxies
• Clustering of galaxies around AGN in the HSC Wide survey
• The matter fluctuation amplitude inferred from the weak lensing power spectrum and correlation function in CFHTLenS data
• Galaxy-galaxy lensing in the VOICE deep survey
• XXL-HSC: Host properties of X-ray detected AGNs in XXL clusters
• The relationship of SMBHs and host galaxies at $z<4$ in the deep optical variability-selected AGN sample in the COSMOS field
• The FLAMINGO project: cosmology with the redshift dependence of weak gravitational lensing peaks
• Fast multiscale galaxy cluster detection with weak lensing: towards a mass-selected sample
• Chasing Nomadic Worlds: A New Class of Deep Space Missions
• Searching for low-redshift faint galaxies with MMT/Hectospec
• Dwarf-Dwarf interactions and their influence on star formation : Insights from post-merger galaxies
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• The Sensitivity of the Redshift Distribution to Galaxy Demographics
• Environments around quasars at $z\sim$3 revealed by wide-field imaging with Subaru HSC and CFHT
• YOLO-CL cluster detection in the Rubin/LSST DC2 simulation
• The SLACS strong lens sample, debiased. II. Lensing-only constraints on the stellar IMF and dark matter contraction in early-type galaxies
• DES to HSC: Detecting low surface brightness galaxies in the Abell 194 cluster using transfer learning
• A Large Massive Quiescent Galaxy Sample at z~1.2
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• Environmental impact on star-forming galaxies in a $z\sim 0.9$ cluster during course of galaxy accretion
• A Framework for Measuring Weak-Lensing Magnification Using the Fundamental Plane
• AstroInspect: a web-based system to organize, assess, and visually inspect astronomical objects
• Fast and accurate collapse-time predictions for collisionless matter
• Joint inference of multiplicative and additive systematics in galaxy density fluctuations and clustering measurements
• The COSMOS-Web Lens Survey (COWLS) III: forecasts versus data
• Counterparts of Candidate Dusty Starbursts at z > 6
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• Low-density star cluster formation: discovery of a young faint fuzzy on the outskirts of the low-mass spiral galaxy NGC 247
• Cosmological Constraints with Void Lensing I: the Simulation-Based Inference Framework
• FPFS Shear Estimator: Systematic Tests on the Hyper Suprime-Cam Survey First Year Data
• Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
• Quantifying the effect of field variance on the H$\alpha$ luminosity function with the New Numerical Galaxy Catalogue (${\nu }^2$GC)
• FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• Euclid preparation. LXVII. Deep learning true galaxy morphologies for weak lensing shear bias calibration
• [CII] luminosity models and large-scale image cubes based on COSMOS 2020 and ALPINE-ALMA [CII] data back to the epoch of reionisation
• Three-Dimensional Reconstruction of Weak Lensing Mass Maps with a Sparsity Prior. I. Cluster Detection
• The mass and galaxy distribution around SZ-selected clusters
• Cosmological constraints from HSC Y1 lensing convergence PDF
• An empirical method for mitigating an excess up-scattering mass bias on the weak lensing mass estimates for shear-selected cluster samples
• Accelerating lensed quasar discovery and modeling with physics-informed variational autoencoders
• Blending effects on shear measurement synergy between Euclid-like and LSST-like surveys
• ADF22+: a declining faint end in the far-infrared luminosity function in the SSA22 protocluster at z=3.09
• Low surface brightness galaxies from BASS+MzLS with Machine Learning
• Z-Sequence: Photometric redshift predictions for galaxy clusters with sequential random k-nearest neighbours
• The superMIGHTEE project: MeerKAT and GMRT Together to Unveil the Deep Radio Sky
• Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• Do blue galaxy-clusters have hot intracluster gas?
• X-ray study of the double source plane gravitational lens system Eye of Horus observed with XMM-Newton
• Galaxy cluster count cosmology with simulation-based inference
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey
• VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Signatures of large-scale cold fronts in the optically-selected merging cluster HSC J085024+001536
• Exploring faint white dwarfs and the luminosity function with Subaru HSC and SDSS in Stripe 82
• X-Ray bright optically faint active galactic nuclei in the Subaru Hyper Suprime-Cam wide survey
• Analysis of Galactic cirrus filaments in HSC-SSP high-resolution deep images using artificial neural networks
• Characterizing CO Emitters in the SSA22-AzTEC26 Field
• Mitigating the impact of fiber assignment on the measurement of galaxy-lensing cross correlation
• Enhancing Ground-Based Observations of Trans-Neptunian Objects using a Single-Epoch Parallax Measurement from L2
• HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
• A MaNGA about the Legacy I: Connecting the Assembly of Stellar Halo with the Average Star Formation History in Low-Redshift Massive Galaxies
• Weak gravitational lensing shear measurement with FPFS: analytical mitigation of noise bias and selection bias
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
• The miniJPAS survey quasar selection I: Mock catalogues for classification
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field
• The X-ray statistical properties of dust-obscured galaxies detected by eROSITA
• Probing the warm dark matter mass with [C II] intensity mapping
• Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
• The $N_H$ Distribution of Hard X-ray Selected AGN in the NEP Field
• Merger fraction in galaxy groups and clusters at z < 0.2: A non-parametric morphological study with Subaru Hyper Suprime-Cam
• The contribution of the color space in LSST-like photometry for the selection of extragalactic globular cluster candidates
• Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset
• Impact of Point Spread Function Higher Moments Error on Weak Gravitational Lensing
• Joint Survey Processing II: Stellar Proper Motions in the COSMOS Field, from Hubble Space Telescope ACS and Subaru Telescope HSC Observations
• eROSITA (eRASS1) study of the Canis Major overdensity: Developing a multi-wavelength algorithm for classifying faint X-ray sources
• A Bibliometric Analysis of the Scholarly Impact of Early Subaru Telescope-based Publications