The Hyper Suprime-Cam SSP Survey: Overview and Survey Design

Abstract

Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2m Subaru telescope on the summit of Maunakea in Hawaii. A team of scientists from Japan, Taiwan and Princeton University is using HSC to carry out a 300-night multi-band imaging survey of the high-latitude sky. The survey includes three layers: the Wide layer will cover 1400 deg${}^2$ in five broad bands ($grizy$), with a $5\sigma$ point-source depth of $r\approx 26$. The Deep layer covers a total of 26~deg${}^2$ in four fields, going roughly a magnitude fainter, while the UltraDeep layer goes almost a magnitude fainter still in two pointings of HSC (a total of 3.5 deg${}^2$). Here we describe the instrument, the science goals of the survey, and the survey strategy and data processing. This paper serves as an introduction to a special issue of the Publications of the Astronomical Society of Japan, which includes a large number of technical and scientific papers describing results from the early phases of this survey.

arXiv comment14 pages, 7 figures, 5 tables. Corrected for a typo in the coordinates of HSC-Wide spring equatorial field in Table 5

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• Massive black hole and Population III galaxy formation in over-massive dark matter halos with violent merger histories
• KiDS-Legacy: Consistency of cosmic shear measurements and joint cosmological constraints with external probes
• Tidal destruction in a low mass galaxy environment: the discovery of tidal tails around DDO 44
• Reaching for the Edge I: Probing the Outskirts of Massive Galaxies with HSC, DECaLS, SDSS, and Dragonfly
• The Signatures of Self-Interacting Dark Matter and Subhalo Disruption on Cluster Substructure
• Cosmological constraints from HSC survey first-year data using deep learning
• The Hyper Suprime-Cam SSP Transient Survey in COSMOS: Overview
• Minkowski Functionals of Convergence Maps and the Lensing Figure of Merit
• Quintessential $\alpha$-attractor inflation: forecasts for Stage IV galaxy surveys
• Classifying Galaxy Morphologies with Few-Shot Learning
• A Comprehensive Examination of the Optical Morphologies of 719 Isolated Galaxies in the AMIGA Sample
• Studying Type II supernovae as cosmological standard candles using the Dark Energy Survey
• Rapidly Evolving Transients from the Hyper Suprime-Cam SSP Transient Survey
• Optical properties of infrared-bright dust-obscured galaxies viewed with Subaru Hyper Suprime-Cam
• Galaxy-Galaxy Lensing in HSC: Validation Tests and the Impact of Heterogeneous Spectroscopic Training Sets
• The Extremely Luminous Quasar Survey in the Pan-STARRS 1 Footprint (PS-ELQS)
• X-ray emission from cosmic web filaments in SRG/eROSITA data
• Testing gravity with galaxy-galaxy lensing and redshift-space distortions using CFHT-Stripe 82, CFHTLenS and BOSS CMASS datasets
• COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
• Properties of AGN Multiband Optical Variability in the HSC SSP Transient Survey
• Hundreds of weak lensing shear-selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S19A data
• ODIN: Where Do Lyman-alpha Blobs Live? Contextualizing Blob Environments within the Large-Scale Structure
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• Identification of tidal features in deep optical galaxy images with Convolutional Neural Networks
• Photometric redshifts with machine learning, lights and shadows on a complex data science use case
• A recently quenched isolated dwarf galaxy outside of the Local Group environment
• Photometric redshifts and Galaxy Clusters for DES DR2, DESI DR9, and HSC-SSP PDR3 Data
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• The Star-forming Main Sequence of the Host Galaxies of Low-redshift Quasars
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\mathbf{z}\sim 4$: hidden AGN and star formation activity
• Power Spectrum of Intrinsic Alignments of Galaxies in IllustrisTNG
• Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
• Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). VIII. New galaxy-scale lenses from the HSC SSP
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• The Mass-Metallicity Relation at $z\sim 0.8$: Redshift Evolution and Parameter Dependency
• Spin Parity of Spiral Galaxies II: A catalogue of 80k spiral galaxies using big data from the Subaru Hyper Suprime-Cam Survey and deep learning
• The impact of very massive stars on the chemical evolution of extremely metal-poor galaxies
• Combining the CLAUDS & HSC-SSP surveys: U+grizy(+YJHKs) photometry and photometric redshifts for 18M galaxies in the 20 deg2 of the HSC-SSP Deep and ultraDeep fields
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) XII. Extended [C II] Structure (Merger or Outflow) in a z = 6.72 Red Quasar
• The UV Luminosity Function of Protocluster Galaxies at $z\sim 4$: the Bright-end Excess and the Enhanced Star Formation Rate Density
• Observable signatures of stellar-mass black holes in active galactic nuclei
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• The eROSITA Final Equatorial-Depth Survey (eFEDS): LOFAR view of brightest cluster galaxies and AGN feedback
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• First HETDEX Spectroscopic Determinations of Ly$\alpha$ and UV Luminosity Functions at $z=2-3$: Bridging a Gap Between Faint AGN and Bright Galaxies
• High-resolution three-dimensional simulations of gas removal from ultrafaint dwarf galaxies. I. Stellar feedback
• Galaxy and Mass Assembly (GAMA): Extended Intra-Group Light in a group at $z=0.2$ from deep Hyper-Suprime Cam images
• Probing Feedback via IGM tomography and Ly$\alpha$ forest with Subaru PFS, TMT/ELT, and JWST
• COSMOS2020: UV selected galaxies at $z\ge 7.5$
• Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses
• Wavelength Dependent PSFs and their impact on Weak Lensing Measurements
• Detecting Pair-Instability Supernovae at z<5 with the James Webb Space Telescope
• The Compact Structures of Massive $z\sim 0.7$ Post-Starburst Galaxies in the SQuIGG$\vec{L}$E Sample
• Structure of the Milky Way stellar halo out to its outer boundary with blue horizontal-branch stars
• EMPRESS. VI. Outflows Investigated in Low-Mass Galaxies with $M_{\ast }=10^4-10^7{M}_{\odot }$: Weak Feedback in Low-Mass Galaxies?
• Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam
• Quantifying the role of ram pressure stripping of galaxies within galaxy groups
• SILVERRUSH X: Machine Learning-Aided Selection of $9318$ LAEs at $z=2.2$, $3.3$, $4.9$, $5.7$, $6.6$, and $7.0$ from the HSC SSP and CHORUS Survey Data
• Sumo Puff: Tidal Debris or Disturbed Ultra-Diffuse Galaxy?
• The Missing Satellite Problem Outside of the Local Group: I -- Pilot Observation
• A systematic study on the rise time-peak luminosity relation for bright optical transients powered by wind shock breakout
• The Sloan Digital Sky Survey Reverberation Mapping Project: Quasar Host Galaxies at $z<0.8$ from Image Decomposition
• Anisotropic separate universe simulations
• New constraints on the mass bias of galaxy clusters from the power spectra of the thermal Sunyaev-Zeldovich effect and cosmic shear
• SCUBA-2 observations of candidate starbursting protoclusters selected by Planck and Herschel-SPIRE
• An FMOS Survey of moderate-luminosity broad-line AGN in COSMOS, SXDS and E-CDF-S
• Identifying galaxy groups at high redshift from incomplete spectroscopic data: I. The group finder and application to zCOSMOS
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• MIGHTEE-HI: the HI Size-Mass relation over the last billion years
• A Unified Catalog-level Reanalysis of Stage-III Cosmic Shear Surveys
• Discovery of Protoclusters at z~3.7 & 4.9: Embedded in Primordial Superclusters
• Consistency of cosmic shear analyses in harmonic and real space
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck I: Construction of CMB Lensing Maps and Modeling Choices
• A machine--vision method for automatic classification of stellar halo substructure
• The Mean Absorption Line Spectra of a Selection of Luminous z~6 Lyman Break Galaxies
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• The impact of AGN feedback on galaxy intrinsic alignments in the Horizon simulations
• Astrophysical Tests of Dark Matter Self-Interactions
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Self-calibration and robust propagation of photometric redshift distribution uncertainties in weak gravitational lensing
• Beyond Ultra-diffuse Galaxies. I. Mass--Size Outliers among the Satellites of Milky Way Analogs
• Subaru Hyper Suprime-Cam View of Quasar Host Galaxies at z < 1
• Field-level inference of galaxy intrinsic alignment from the SDSS-III BOSS survey
• The PAU Survey: narrowband photometric redshifts using Gaussian processes
• A Mock Catalog of Gravitationally Lensed Quasars for the LSST Survey
• An Optimal Estimator of Intrinsic Alignments for Star-forming Galaxies in IllustrisTNG Simulation
• The stellar mass in and around isolated central galaxies: connections to the total mass distribution through galaxy-galaxy lensing in the Hyper Suprime-Cam survey
• AGN X-ray luminosity function and absorption function in the Early Universe ($3\le z\le 6$)
• Weak lensing clusters from HSC survey first-year data: Mitigating the dilution effect of foreground and cluster member galaxies
• Velocity dispersion and dynamical mass for 270 galaxy clusters in the Planck PSZ1 catalogue
• ArtPop: A Stellar Population and Image Simulation Python Package
• SILVERRUSH. IX. Lya Intensity Mapping with Star-Forming Galaxies at z=5.7 and 6.6: A Possible Detection of Extended Lya Emission at $\gtrsim$100 comoving kpc around and beyond the Virial-Radius Scale of Galaxy Dark Matter Halos
• Identification of AKARI infrared sources by Deep HSC Optical Survey: Construction of New Band-Merged Catalogue in the NEP-Wide field
• A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to $z\approx 1.1$ in the Hyper Suprime-Cam survey
• A 16 deg${}^2$ survey of emission-line galaxies at z<1.6 from HSC-SSP PDR2 and CHORUS
• Photometric Redshift Uncertainties in Weak Gravitational Lensing Shear Analysis: Models and Marginalization
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Outside the Lyman-break box: detecting Lyman continuum emitters at $3.5<z<5.1$ with CLAUDS
• WEAVE-StePS. A stellar population survey using WEAVE at WHT
• Galaxy Morphologies Revealed with Subaru HSC and Super-Resolution Techniques I: Major Merger Fractions of L_UV~3-15 L_UV* Dropout Galaxies at z~4-7
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• The impact of human expert visual inspection on the discovery of strong gravitational lenses
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• The HectoMAP Redshift Survey: First Data Release
• Effects of overlapping sources on cosmic shear estimation: Statistical sensitivity and pixel-noise bias
• Statistical strong lensing. III. Inferences with complete samples of lenses
• Cosmology with the sub-millimetre galaxies magnification bias: Tomographic Analysis
• Galaxy morphoto-Z with neural Networks (GaZNets). I. Optimized accuracy and outlier fraction from Imaging and Photometry
• Dust and Power: Unravelling the merger - active galactic nucleus connection in the second half of cosmic history
• MIGHTEE-HI: The HI mass-stellar mass relation over the last billion years
• The Obscured Fraction of Quasars at Cosmic Noon
• Strategies for optimal sky subtraction in the low surface brightness regime
• The SAMI Galaxy Survey: Using Tidal Streams and Shells to Trace the Dynamical Evolution of Massive Galaxies
• Calibrating photometric redshift measurements with the Multi-channel Imager (MCI) of the China Space Station Telescope (CSST)
• Mitigating the effects of undersampling in weak lensing shear estimation with metacalibration
• CHORUS. III. Photometric and Spectroscopic Properties of Ly$\alpha$ Blobs at $z=4.9-7.0$
• Higher order statistics of shear field: a machine learning approach
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• Orphan GRB afterglow searches with the Pan-STARRS1 COSMOS survey
• The dominant origin of diffuse Ly$\alpha$ halos around LAEs explored by SED fitting and clustering analysis
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IX. Identification of Two Red Quasars at z > 5.6
• Difficulties in Mid-Infrared selection of AGN in dwarf galaxies
• The brightest UV-selected galaxies in protoclusters at $z\sim 4$: Ancestors of Brightest Cluster Galaxies?
• The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX) I. Sample selection
• CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). I. The Optical Counterparts of FIRST Radio Sources
• The Infrared Medium-deep Survey. IV. Low Eddington Ratio of A Faint Quasar at $z\sim 6$: Not Every Supermassive Black Hole is Growing Fast in the Early Universe
• Classifying Stars, Galaxies and AGN in CLAUDS+HSC-SSP Using Gradient Boosted Decision Trees
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray properties of Subaru optically-selected clusters
• Estimating redshift distributions using Hierarchical Logistic Gaussian processes
• The LOFAR-eFEDS survey: The incidence of radio and X-ray AGN and the disk-jet connection
• Constraining dark matter decays with cosmic microwave background and weak lensing shear observations
• Constraining axion and compact dark matter with interstellar medium heating
• A Composite Likelihood Approach for Inference under Photometric Redshift Uncertainty
• Discovery of merging twin quasars at z = 6.05
• Mass Bias of Weak Lensing Shear-selected Galaxy Cluster Samples
• The correlation of extragalactic $\gamma$-rays with cosmic matter density distributions from weak-gravitational lensing
• A new discovery space opened by eROSITA: Ionised AGN outflows from X-ray selected samples
• MIGHTEE-HI: deep spectral line observations of the COSMOS field
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IV. Rapidly Growing (Super-)Massive Black Holes in Extremely Radio-Loud Galaxies
• Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck
• Probing magnetic fields in the circumgalactic medium using polarization data from MIGHTEE
• Galaxy And Mass Assembly (GAMA): Comparing Visually and Spectroscopically Identified Galaxy Merger Samples
• Active gas features in three HSC-SSP CAMIRA clusters revealed by high angular resolution analysis of MUSTANG-2 SZE and XXL X-ray observations
• The observed cosmic star formation rate density has an evolution which resembles a Γ(a, bt) distribution and can be described successfully by only 2 parameters
• The COSMOS-Web ring: in-depth characterization of an Einstein ring lensing system at z~2
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• Massive Early-Type Galaxies in the HSC-SSP: Flux Fraction of Tidal Features and Merger Rates
• The Stellar Mass - Black Hole Mass Relation at $z\sim 2$ Down to ${\mathcal{M}}_{\mathrm{BH}}\sim 10^7{M}_{\odot }$ Determined by HETDEX
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• The SRG/eROSITA All-Sky Survey: Weak-Lensing of eRASS1 Galaxy Clusters in KiDS-1000 and Consistency Checks with DES Y3 & HSC-Y3
• Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
• Cosmological constraints from weak lensing scattering transform using HSC Y1 data
• Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). III. Discovery of a z = 4.72 Radio Galaxy with Lyman Break Technique
• Fast estimation of aperture mass statistics II: Detectability of higher order statistics in current and future surveys
• Covariances for cosmic shear and galaxy-galaxy lensing in the response approach
• HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Sky Subtraction in an Era of Low Surface Brightness Astronomy
• Observational constraints of an anisotropic boost due to the projection effects using redMaPPer clusters
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• Measurement of redshift dependent cross correlation of HSC clusters and Fermi $\gamma$ rays
• Cosmological Probes of Structure Growth and Tests of Gravity
• Angular clustering and host halo properties of [OII] emitters at $z>1$ in the Subaru HSC survey
• 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
• The Nature of Low Surface Brightness Galaxies in the Hyper Suprime-Cam Survey
• TOPz: Photometric redshifts for J-PAS
• X-ray luminosity-star formation rate scaling relation: Constraints from the eROSITA Final Equatorial Depth Survey (eFEDS)
• Detection of Cosmic Magnification via Galaxy Shear -- Galaxy Number Density Correlation from HSC Survey Data
• RELICS: ICL Analysis of the $z=0.566$ merging cluster WHL J013719.8-08284
• CircleZ: Reliable Photometric redshifts for AGN computed using only photometry from Legacy Survey Imaging for DESI
• Merger Signatures are Common, but not Universal, In Massive, Recently-Quenched Galaxies at z~0.7
• Photometric Biases in Modern Surveys
• Fractal dimension of optical cirrus in Stripe82
• The whole picture of the large-scale structure of the CL1604 supercluster at z$\sim$0.9
• The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
• Extending Ultra-Diffuse Galaxy Abundances to Milky Way Analogs
• Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation
• 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
• Central velocity dispersion catalog of LAMOST-DR7 galaxies
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• The Infrared Medium-deep Survey. \Romannum{7}. Faint Quasars at $z\sim 5$ in the ELAIS-N1 Field
• Euclid Preparation XXXIII. Characterization of convolutional neural networks for the identification of galaxy-galaxy strong lensing events
• A General Framework for Removing Point Spread Function Additive Systematics in Cosmological Weak Lensing Analysis
• Neutral Hydrogen Observations of Low Surface Brightness Galaxies around M101 and NGC 5485
• 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
• Low X-ray surface brightness clusters: Implications on the scatter of the $M-T$ and $L-T$ relations
• Hyper Suprime-Cam Legacy Archive
• Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field
• Searching for Moving Objects in HSC-SSP: Pipeline and Preliminary Results
• A Challenge to Identify an Optical Counterpart of the Gravitational Wave Event GW151226 with Hyper Suprime-Cam
• Deblending Galaxies with Generative Adversarial Networks
• Weak Lensing Study in VOICE Survey I: Shear Measurement
• MUSSES2020J: The Earliest Discovery of a Fast Blue Ultraluminous Transient at Redshift 1.063
• Impact of Point Spread Function Higher Moments Error on Weak Gravitational Lensing II: A Comprehensive Study
• The AMIGA sample of isolated galaxies. XIV. Disc breaks and interactions through ultra-deep optical imaging
• Weak Gravitational Lensing Shear Estimation with Metacalibration for the Roman High-Latitude Imaging Survey
• The halo model with beyond-linear halo bias: unbiasing cosmological constraints from galaxy-galaxy lensing and clustering
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• Disentangling the multi-phase circumgalactic medium shared between a dwarf and a massive star-forming galaxy at z~0.4
• The Extended Disk Galaxy Exploration Science Survey: Description and Surface Brightness Profile Properties
• Ionizing radiation from AGNs at z>3.3 with the Subaru Hyper Suprime-Cam Survey and the CFHT Large Area U-band Deep Survey (CLAUDS)
• Deep+Wide Lensing Surveys will Provide Exquisite Measurements of the Dark Matter Halos of Dwarf Galaxies
• Brightest Cluster Galaxies Are Statistically Special From $z=0.3$ to $z=1$
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• Discovery of an unusually compact lensed Lyman Break Galaxy from the Hyper Suprime-Cam Survey
• Lensed quasar search via time variability with the HSC transient survey
• The HSC-SSP Transient Survey: Implications from Early Photometry and Rise Time of Normal Type Ia Supernovae
• TDCOSMO XV: Population Analysis of Lines of Sight of 25 Strong Galaxy-Galaxy Lenses with Extreme Value Statistics
• Linear Systematics Mitigation in Galaxy Clustering in the Dark Energy Survey Year 1 Data
• Simulation-based inference of deep fields: galaxy population model and redshift distributions
• Dark Energy Survey Year 3 Results: Redshift Calibration of the MagLim Lens Sample from the combination of SOMPZ and clustering and its impact on Cosmology
• Search and characterization of remnant radio galaxies in the XMM$-$LSS deep field
• Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments
• PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field II
• Extreme nature of four blue-excess dust-obscured galaxies revealed by optical spectroscopy
• Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg${}^2$ at z=0.3-0.6
• EMPRESS. XI. SDSS and JWST Search for Local and z~4-5 Extremely Metal-Poor Galaxies (EMPGs): Clustering and Chemical Properties of Local EMPGs
• MaNGA 8313-1901: gas accretion observed in a blue compact dwarf galaxy?
• SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 6
• Estimating Sky Level
• The Rest-frame $H$-band Luminosity Function of Red Sequence Galaxies in Clusters at $1.0<z<1.3$
• COSMOS-Web: The emergence of the Hubble Sequence
• HOLISMOKES -- XI. Evaluation of supervised neural networks for strong-lens searches in ground-based imaging surveys
• Accurate field-level weak lensing inference for precision cosmology
• The eROSITA Final Equatorial-Depth Survey (eFEDS): The first archetypal Quasar in the feedback phase discovered by eROSITA
• Quasars at intermediate redshift are not special; but they are often satellites
• Morphological Parameters and Associated Uncertainties for 8 Million Galaxies in the Hyper Suprime-Cam Wide Survey
• Dwarf Galaxy Discoveries from the KMTNet Supernova Program II. The NGC 3585 Group and Its Dynamical State
• AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from angular power spectrum and correlation function
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• Photometric classification of HSC transients using machine learning
• Detection of anisotropic satellite quenching in galaxy clusters up to $z\sim 1$
• 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
• Dark Energy Survey Year 1 Results: Wide field mass maps via forward fitting in harmonic space
• The SCUBA-2 Large eXtragalactic Survey: 850um map, catalogue and the bright-end number counts of the XMM-LSS field
• OSSOS XII: Variability studies of 65 Trans-Neptunian Objects using the Hyper Suprime-Cam
• The HI Bias during the Epoch of Reionization
• Mixed Warm Dark Matter Constraints using Milky Way Satellite Galaxy Counts
• Paving the Way for Euclid and JWST via Optimal Selection of High-z Quasars
• The SRG/eROSITA All-Sky Survey : Subaru/HSC-SSP weak-lensing mass measurements for the eRASS1 Galaxy Clusters
• Subaru narrow-band imaging search for Lyman continuum from galaxies at z>3 in the GOODS-N field
• CHORUS IV: Mapping the Spatially Inhomogeneous Cosmic Reionization with Subaru HSC
• Beyond the Local Volume. II. Population Scaleheights and Ages of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
• Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey
• A model for galaxy-galaxy strong lensing statistics in surveys
• The ACT-DR5 MCMF Galaxy Cluster Catalog
• Denser Environments Cultivate Larger Galaxies: A Comprehensive Study beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies
• Discovery of a Bimodal Environmental Distribution of Compact Ellipticals in the Local Universe
• Getting ready for the LSST data -- estimating the physical properties of $z<2.5$ main sequence galaxies
• DESI Complete Calibration of the Color-Redshift Relation (DC3R2): Results from early DESI data
• The eROSITA Final Equatorial-Depth Survey (eFEDS) -- Splashback radius of X-ray galaxy clusters using galaxies from HSC survey
• A Recipe for Unbiased Background Modeling in Deep Wide-Field Astronomical Images
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• How dark are filaments in the cosmic web?
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Velocity Dispersions of Massive Quiescent Galaxies from Weak Lensing and Spectroscopy
• The XXL Survey XLIV. Sunyaev-Zel'dovich mapping of a low-mass cluster at z~1: a multi-wavelength approach
• The eROSITA Final Equatorial Depth Survey (eFEDS): the hard X-ray selected sample
• 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
• Improving Photometric Redshift Estimates with Training Sample Augmentation
• A deep radio view of the evolution of the cosmic star-formation rate density from a stellar-mass selected sample in VLA-COSMOS
• Multi-band Photometry of Trans-Neptunian Objects in the Subaru Hyper Suprime-Cam Survey
• ODIN: Clustering Analysis of 14,000 Lyα Emitting Galaxies at z=2.4, 3.1, and 4.5
• Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• More connected, more active: galaxy clusters and groups at z~1 and the connection between their quiescent galaxy fractions and large-scale environments
• Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics
• The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey Galaxy Cluster Catalogue
• Mitigating the impact of fiber assignment on clustering measurements from deep galaxy redshift surveys
• Pix2Prof: fast extraction of sequential information from galaxy imagery via a deep natural language 'captioning' model
• SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z>6
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• The nature of H$\alpha$-selected galaxies along the large-scale structure at z=0.4 revealed by Subaru Hyper Suprime-Cam survey
• Simulation-Based Inference Benchmark for Weak Lensing Cosmology
• Proper motion measurements for stars up to $100$ kpc with Subaru HSC and SDSS Stripe 82
• JWST/NIRSpec spectroscopy of intermediate-mass quiescent galaxies at $z\sim 3-4$
• HSC-XD 52: An X-ray detected AGN in a low-mass galaxy at $z\sim 0.56$
• XXL-HSC: An updated catalogue of high-redshift ($z⩾3.5$) X-ray AGN in the XMM-XXL northern field. Constraints on the bright end of the soft logN-logS
• Faint Quasars Live in the Same Number Density Environments as Lyman Break Galaxies at z ~ 4
• Beyond Ultra-diffuse Galaxies. II. Environmental Quenching of Mass-Size Outliers among the Satellites of Milky Way Analogs
• Intracluster light is a biased tracer of the dark matter distribution in clusters
• Fast generation of mock galaxy catalogues with COLA
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• eROSITA Final Equatorial-Depth Survey (eFEDS): eFEDS X-ray view of WERGS Radio Galaxies selected by the Subaru/HSC and VLA/FIRST survey
• HOLISMOKES XIII: Strong-lens candidates at all mass scales and their environments from the Hyper-Suprime Cam and deep learning
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group
• Dark Energy Survey Year 6 Results: Cell-based Coadds and Metadetection Weak Lensing Shape Catalogue
• Impact of nonlinear growth of the large-scale structure on CMB B-mode delensing
• X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field
• A catalog of galaxy clusters identified from SCUSS, SDSS, and unWISE
• Miscentering of Optical Galaxy Clusters Based on Sunyaev-Zeldovich Counterparts
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Chromatic Effects on the PSF and Shear Measurement for the Roman Space Telescope High-Latitude Wide Area Survey
• Measuring the X-ray luminosities of DESI groups from eROSITA Final Equatorial-Depth Survey: I. X-ray luminosity -- halo mass scaling relation
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• Constraints on the rate of supernovae lasting for more than a year from Subaru/Hyper Suprime-Cam
• Fast estimation of aperture-mass statistics I: aperture mass variance and an application to the CFHTLenS data
• High Star Formation Rates of Low Eddington Ratio Quasars at $z\gtrsim 6$
• A deep analysis for New Horizons' KBO search images
• Uncovering Tidal Treasures: Automated Classification of Faint Tidal Features in DECaLS Data
• Using Dark Energy Explorers and Machine Learning to Enhance the Hobby-Eberly Telescope Dark Energy Experiment
• Intrinsic galaxy alignments in the KiDS-1000 bright sample: dependence on colour, luminosity, morphology, and galaxy scale
• MIGHTEE-HI: Discovery of an HI-rich galaxy group at z = 0.044 with MeerKAT
• Type Ia Supernova Magnitude Step from the local Dark Matter Environment
• 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
• Scaling relations of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program Field
• HSC16aayt: Slowly evolving interacting transient rising for more than 100 days
• A Fresh Look at AGN Spectral Energy Distribution Fitting with the XMM-SERVS AGN Sample
• On constraining Cosmology and the Halo Mass Function with Weak Gravitational Lensing
• Weak Lensing Trispectrum and Kurt-Spectra
• Euclid and KiDS-1000: Quantifying the impact of source-lens clustering on cosmic shear analyses
• Kinematics of disk galaxies in (proto-)clusters at z=1.5
• The Average Soft X-ray Spectra of eROSITA Active Galactic Nuclei
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• The Active Galactic Nuclei in the Hobby-Eberly Telescope Dark Energy Experiment Survey (HETDEX) II. Luminosity Function
• Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies
• Galaxy clusters at z~1 imaged by ALMA with the Sunyaev-Zel'dovich effect
• LOFAR properties of SILVERRUSH Ly$\alpha$ emitter candidates in the ELAIS-N1 field
• Optical and near-infrared spectroscopy of quasars at $z>6.5$: public data release and composite spectrum
• Cluster candidates with massive quiescent galaxies at $z\sim 2$
• X-ray spectral properties of dust-obscured galaxies in the XMM-SERVS coverage of the XMM-LSS field
• Magnification bias in the shear-ratio test: a viable mitigation strategy
• Optimising LSST Observing Strategy for Weak Lensing Systematics
• Euclid preparation. XXXI. The effect of the variations in photometric passbands on photometric-redshift accuracy
• King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z=0.55 using the Subaru Hyper Suprime-Cam
• MIGHTEE-HI: The radial acceleration relation with resolved stellar mass measurements
• The XMM Cluster Survey: An independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies
• The evolution of galaxy scaling relations in clusters at 0.5<z<1.5
• Intrinsic alignments of galaxies around cosmic voids
• A robust two-parameter description of the stellar profile of elliptical galaxies
• Improved Tomographic Binning of 3x2pt Lens Samples: Neural Network Classifiers and Optimal Bin Assignments
• Growth and Geometry Split in Light of the DES-Y3 Survey
• The Infrared Medium-deep Survey. IX. Discovery of Two New $z\sim 6$ Quasars and Space Density down to $M_{1450}\sim -23.5$ mag
• Validation of Emission-Line Galaxies Target Selection Algorithms for the Dark Energy Spectroscopic Instrument Using the MMT Binospec
• Analysis of biasing from noise from the Nancy Grace Roman Space Telescope: implications for weak lensing
• Photometric redshift estimation of strongly lensed galaxies
• E/B mode decomposition of HSC-Y1 cosmic shear using COSEBIs: cosmological constraints and comparison with other two-point statistics
• Stage IV baryonic feedback correction for non-Gaussianity inference
• 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
• The XXL Survey L. Active galactic nucleus contamination in galaxy clusters: Detection and cosmological impact
• Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• A rising tide: Intrinsic alignments since the turn of the millennium
• ALMA Observations for CO Emission from Luminous Lyman-break Galaxies at $z=6.0293$-$6.2037$
• High-$z$ Universe probed via Lensing by QSOs (HULQ) I. Number Estimates of QSO-QSO and QSO-Galaxy Lenses
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• A new observable for cosmic shear
• The Impact of Photometric Redshift Errors on Lensing Statistics in Ray-Tracing Simulations
• Clustering of galaxies around AGN in the HSC Wide survey
• Searching for cold gas traced by MgII quasar absorbers in massive X-ray-selected galaxy clusters
• SDSS-IV MaNGA: the physical origin of off-galaxy H$\alpha$ blobs in the local Universe
• Chasing Nomadic Worlds: A New Class of Deep Space Missions
• Pure-mode correlation functions for cosmic shear and application to KiDS-1000
• Probing Quintessence using BAO imprint on the cross-correlation of weak lensing and post-reionization HI 21 cm signal
• Compressing combined probes: redshift weights for joint lensing and clustering analyses
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Searching for low-redshift faint galaxies with MMT/Hectospec
• The Role of Dust, UV Luminosity and Large-scale Environment on the Escape of Lya Photons: A Case Study of a Protocluster field at z = 3.1
• The matter fluctuation amplitude inferred from the weak lensing power spectrum and correlation function in CFHTLenS data
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• Strongly lensed candidates from the HSC transient survey
• The XXL Survey LI. Pressure profile and $Y_{\mathrm{SZ}}$-$M$ scaling relation in three low-mass galaxy clusters at $z\sim 1$ observed with NIKA2
• Squeezing Full-Shape Dynamical Dark Energy Constraints with Galaxy Alignments
• Constraining Hot Dark Matter Sub-Species with Weak Lensing and the Cosmic Microwave Background Radiation
• Accurate Kappa Reconstruction Algorithm for masked shear catalog (AKRA)
• An Accurate P${}^3$M Algorithm for Gravitational Lensing Studies in Simulations
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Impacts of pre-initial conditions on anisotropic separate universe simulations: a boosted tidal response in the epoch of reionization
• Optical Spectroscopy of Dual Quasar Candidates from the Subaru HSC-SSP program
• The relationship of SMBHs and host galaxies at $z<4$ in the deep optical variability-selected AGN sample in the COSMOS field
• A low-inclination neutral Trans-Neptunian Object in a extreme orbit
• Search for extended Lyman-$\alpha$ emission around 9k quasars at z=2-3
• MIGHTEE-\HI: Possible interactions with the galaxy NGC~895
• The SLACS strong lens sample, debiased. II. Lensing-only constraints on the stellar IMF and dark matter contraction in early-type galaxies
• 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
• Morpho-Photometric Classification of KiDS DR5 Sources Based on Neural Networks: A Comprehensive Star-Quasar-Galaxy Catalog
• The quasar luminosity function at $z\sim 5$ via deep learning and Bayesian information criterion
• Joint inference of multiplicative and additive systematics in galaxy density fluctuations and clustering measurements
• Universal conditional distribution function of [OII] luminosity of galaxies, and prediction for the [OII] luminosity function at redshift $z<3$
• Environments around quasars at $z\sim$3 revealed by wide-field imaging with Subaru HSC and CFHT
• The First SRG/eROSITA All-Sky Survey. Characterization of clusters of galaxies misclassified in the eRASS1 point source catalog
• Euclid: Photometric redshift calibration with self-organising maps
• CLAP. I. Resolving miscalibration for deep learning-based galaxy photometric redshift estimation
• Dwarf-Dwarf interactions and their influence on star formation : Insights from post-merger galaxies
• Environmental impact on star-forming galaxies in a $z\sim 0.9$ cluster during course of galaxy accretion
• AKRA 2.0: Accurate Kappa Reconstruction Algorithm for masked shear catalog
• Dark Energy Survey Year 3 Results: Deep Field Optical + Near-Infrared Images and Catalogue
• The Complete Spitzer Survey of Stellar Structure in Galaxies (CS${}^4$G)
• Position-Dependent Correlation Function of Weak Lensing Convergence
• UNIONS Optical Identifications for VLASS Radio Sources in the Euclid Sky (UNVEIL) I. A Catalog of ~146,000 Radio Galaxies up to z~5
• Informed total-error-minimizing priors: Interpretable cosmological parameter constraints despite complex nuisance effects
• The miniJPAS survey: Maximising the photo-z accuracy from multi-survey datasets with probability conflation
• Using Machine Learning to Determine Morphologies of $z<1$ AGN Host Galaxies in the Hyper Suprime-Cam Wide Survey
• KMTNet Nearby Galaxy Survey: Overview and a Survey Description
• Tackling the Problem of Distributional Shifts: Correcting Misspecified, High-Dimensional Data-Driven Priors for Inverse Problems
• Photometric Selection of type 1 Quasars in the XMM-LSS Field with Machine Learning and the Disk-Corona Connection
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties
• MUSUBI (MegaCam Ultra-deep Survey: $u^{\ast }$-Band Imaging)-Data for the COSMOS and SXDS Fields
• Quasars Have Fewer Close Companions than Normal Galaxies
• Tracing the Total Stellar Mass and Star Formation of High-Redshift Protoclusters
• AstroClearNet: Deep image prior for multi-frame astronomical image restoration
• Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
• Testing Cotton gravity as dark matter substitute with weak lensing
• Synthetic Galaxy Clusters and Observations Based on Dark Energy Survey Year 3 Data
• A New Polar Ring Galaxy Discovered in the COSMOS Field
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Low-density star cluster formation: discovery of a young faint fuzzy on the outskirts of the low-mass spiral galaxy NGC 247
• Weak lensing peak statistics -- steepness versus height
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• Quantifying the effect of field variance on the H$\alpha$ luminosity function with the New Numerical Galaxy Catalogue (${\nu }^2$GC)
• UFig v1: The ultra-fast image generator
• Weak Gravitational Lensing
• Weak Lensing Reconstruction by Counting DECaLS Galaxies
• The Gravitational-wave Optical Transient Observer (GOTO): prototype performance and prospects for transient science
• Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
• Counterparts of Candidate Dusty Starbursts at z > 6
• Cosmic flexion
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Ultra-Faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3
• An empirical method for mitigating an excess up-scattering mass bias on the weak lensing mass estimates for shear-selected cluster samples
• Effect of lensing magnification on type Ia supernova cosmology
• Euclid Preparation: XIV. The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Data Release 3
• An estimate of resident time of the Oort Cloud new comets in planetary region
• The informativeness of [C II] line-intensity mapping as a probe of the H I content and metallicity of galaxies at the end of reionization
• The uncommon intracluster medium features of the first massive clusters selected independently of their baryon content
• Strong lensing cross sections for isothermal models - I. Finite source effects in the circular case
• Z-Sequence: Photometric redshift predictions for galaxy clusters with sequential random k-nearest neighbours
• DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
• Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
• Properties of environment around AGN and luminous galaxy pairs through HSC wide survey
• X-ray study of the double source plane gravitational lens system Eye of Horus observed with XMM-Newton
• The SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts
• Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe
• On the tomographic cluster clustering as a cosmological probe
• Reconstructing redshift distributions with photometric galaxy clustering
• Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIV. A Candidate Type-II Quasar at z=6.1292
• Data-driven Cosmology from Three-dimensional Light Cones
• Impact of weak-lensing mass-mapping algorithms on cosmology inference
• Cosmological-Scale Lyman-alpha Forest Absorption Around Galaxies and AGN Probed with the HETDEX and SDSS Spectroscopic Data
• A machine learning approach to assessing the presence of substructure in quasar host galaxies using the Hyper Suprime-Cam Subaru Strategic Program
• On the Origin of the Strong Optical Variability of Emission-line Galaxies
• The environment of QSO triplets at 1 $\lesssim$ z $\lesssim$ 1.5
• Low surface brightness galaxies from BASS+MzLS with Machine Learning
• Environment of SDSS quasars at $z=0.4$$-$$1.0$ explored by Subaru HSC
• The X-ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-Driven Massive Star Explosions
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
• The Jet Paths of Radio AGN and their Cluster Weather
• Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey
• Black holes as telescopes: Discovering supermassive binaries through quasi-periodic lensed starlight
• The Intracluster Light of Abell 3667: Unveiling an Optical Bridge in LSST Precursor Data
• Do blue galaxy-clusters have hot intracluster gas?
• Environmental Quenching of Low Surface Brightness Galaxies near Milky Way mass Hosts
• Cosmological consequences of intrinsic alignments super-sample covariance
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• Exploring the spatially-resolved capabilities of the J-PAS survey with Py2DJPAS
• The X-ray$-$UV Luminosity Relation of eROSITA Quasars
• HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Hyper Suprime-Cam Y3 results: photo-$z$ bias calibration with lensing shear ratios and cosmological constraints from cosmic shear
• Mitigating the impact of fiber assignment on the measurement of galaxy-lensing cross correlation
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• Confirming HSC strong lens candidates with DESI Spectroscopy. I. Project overview and first results
• Exploring faint white dwarfs and the luminosity function with Subaru HSC and SDSS in Stripe 82
• Signatures of large-scale cold fronts in the optically-selected merging cluster HSC J085024+001536
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• Measuring the evolution of stellar bars with the host galaxy's spin
• Selecting Clusters and Protoclusters via Stellar Mass Density: II. Application to HSC-SSP Observations
• Dusty Clump Survival in Supernova Ejecta: Dust-Mediated Growth vs. Crushing by the Reverse Shock
• Robustness of Neural Ratio and Posterior Estimators to Distributional Shifts for Population-Level Dark Matter Analysis in Strong Gravitational Lensing
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• Can luminous Lyman alpha emitters at $z$ $\simeq$ 5.7 and $z$ $\simeq$ 6.6 suppress star formation?
• Constraining Power of Wavelet vs. Power Spectrum Statistics for CMB Lensing and Weak Lensing with Learned Binning
• Colors of Centaurs observed by the Subaru/Hyper Suprime-Cam and implications for their origin
• ImageMM: Joint multi-frame image restoration and super-resolution
• X-Ray bright optically faint active galactic nuclei in the Subaru Hyper Suprime-Cam wide survey
• A New Estimator for Phase Statistics
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Cosmic magnification on high-redshift submillimeter galaxies
• H$\alpha$ emission in the outskirts of galaxies at z=0.4
• Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network
• GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference
• Quiescent Galaxy Size, Velocity Dispersion, and Dynamical Mass Evolution
• The Exploration of Local VolumE Satellites (ELVES) Survey: A Nearly Volume-Limited Sample of Nearby Dwarf Satellite Systems
• The FAST Hundred-Deg${}^2$ HI Deep (HD${}^2$) Survey: Early Results from the Pilot Survey
• Identification of high-redshift X-ray active galactic nuclei in the 4XMM-DR11 serendipitous catalogue using DES data: Comparative analysis with optically-selected QSOs
• Identifying AGN host galaxies by Machine Learning with HSC+WISE
• Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScience
• The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
• The X-ray statistical properties of dust-obscured galaxies detected by eROSITA
• Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data
• Measuring weak lensing masses on individual clusters
• Zwicky Transient Facility and Globular Clusters: The RR Lyrae gri-Band Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity Relations
• Optimizing the Roman Space Telescope High-Latitude Wide Area Survey for mitigating chromatic PSF effects on shear measurement
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
• Isophotal signatures of the brightest cluster galaxy - intracluster light transition
• A Novel Framework for Modeling Weakly Lensing Shear Using Kinematics and Imaging at Moderate Redshift
• Evaluating the V-band Photometric Metallicity with Fundamental Mode RR Lyrae in the Kepler Field
• Passive spiral galaxies deeply captured by Subaru Hyper Suprime-Cam
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field
• Using a Neural Network Classifier to Select Galaxies with the Most Accurate Photometric Redshifts
• Connecting galaxy evolution in clusters with their radial profiles and phase space distribution: results from the IllustrisTNG hydrodynamical simulations
• Bright Star Subtraction Pipeline for LSST: Phase one report
• High-$z$ Universe probed via Lensing by QSOs (HULQ) II. Deep GMOS spectroscopy of a QSO lens candidate
• Impact of Point Spread Function Higher Moments Error on Weak Gravitational Lensing
• Size-Mass Relation Shows Its Colours: Contrasting Physical Imprints of Galaxy Evolution in Rest-Frame UV and Optical
• Cosmology with the Roman Space Telescope -- Synergies with CMB lensing
• Prospects for detecting asteroid-mass primordial black holes in extreme mass-ratio inspirals with continuous gravitational waves
• The effect of spiral arms on the Sérsic photometry of galaxies
• Intrinsic alignments of galaxies in multiple projections
• Clustering analysis of medium-band selected high-redshift galaxies
• D${}_4$CNN$\times$AnaCal: Physics-Informed Machine Learning for Accurate and Precise Weak Lensing Shear Estimation
• Highly Efficient Selection of High-Redshift Emission-Line Galaxies for future DESI-like surveys with Deep Multi-band Imaging
• J-PAS: forecast on the primordial power spectrum reconstruction
• Merger fraction in galaxy groups and clusters at z < 0.2: A non-parametric morphological study with Subaru Hyper Suprime-Cam
• $\text{SBi3PCF:}$ Simulation-based inference with the integrated 3PCF
• Revising Indirect Dark Matter Constraints with Updated Astrophysical $J$-Factor Priors
• Skykatana: a scalable framework to construct sky masks for the Vera Rubin Observatory and large astronomical surveys
• Photometric Redshift Estimation Using Scaled Ensemble Learning
• Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset
• An empirical nonlinear power spectrum overdensity-response
• Properties of Polarized Radio Sources in the Wide Chandra Deep Field South from 2 to 4GHz
• On Weak Lensing Response Functions
• SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and Evolution
• Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
• SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies