The Kilo-Degree Survey

Abstract

The Kilo Degree Survey (KiDS) is a 1500 square degree optical imaging survey with the recently commissioned OmegaCAM wide-field imager on the VLT Survey Telescope (VST). A suite of data products will be delivered to the European Southern Observatory (ESO) and the community by the KiDS survey team. Spread over Europe, the KiDS team uses Astro-WISE to collaborate efficiently and pool hardware resources. In Astro-WISE the team shares, calibrates and archives all survey data. The data-centric architectural design realizes a dynamic 'live archive' in which new KiDS survey products of improved quality can be shared with the team and eventually the full astronomical community in a flexible and controllable manner.

20 pages, Accepted for publication in topical issue of Experimental Astronomy on Astro-WISE information system

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Cited by in corpus (303)

• Challenges for $\Lambda$CDM: An update
• Large-Scale Galaxy Bias
• Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
• Cosmology with cosmic shear observations: a review
• The SAMI Galaxy Survey: instrument specification and target selection
• The Hyper Suprime-Cam Software Pipeline
• The Dark Energy Survey Data Release 1
• Gravitational Lensing Analysis of the Kilo Degree Survey
• Weak lensing for precision cosmology
• The realm of the galaxy protoclusters
• The first and second data releases of the Kilo-Degree Survey
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
• Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3
• The first-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey
• HACC: Simulating Sky Surveys on State-of-the-Art Supercomputing Architectures
• The Dark Energy Survey Image Processing Pipeline
• The third data release of the Kilo-Degree Survey and associated data products
• The SPTpol Extended Cluster Survey
• KiDS-450: Testing extensions to the standard cosmological model
• KiDS-450: The tomographic weak lensing power spectrum and constraints on cosmological parameters
• CFHTLenS: The relation between galaxy dark matter haloes and baryons from weak gravitational lensing
• The Atacama Cosmology Telescope: CMB Polarization at $200<\ell <9000$
• Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• The Strong Gravitational Lens Finding Challenge
• DustPedia - A Definitive Study of Cosmic Dust in the Local Universe
• Surveying the reach and maturity of machine learning and artificial intelligence in astronomy
• The bright-star masks for the HSC-SSP survey
• Effect of galaxy mergers on star formation rates
• Constraints on the Richness-Mass Relation and the Optical-SZE Positional Offset Distribution for SZE-Selected Clusters
• Fisher for complements: Extracting cosmology and neutrino mass from the counts-in-cells PDF
• Dark Energy Survey Year 1 Results: Galaxy-Galaxy Lensing
• LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, Design and Target Catalogue
• IM3SHAPE: A maximum-likelihood galaxy shear measurement code for cosmic gravitational lensing
• The halo model as a versatile tool to predict intrinsic alignments
• Phenotypic redshifts with self-organizing maps: A novel method to characterize redshift distributions of source galaxies for weak lensing
• Cosmological Constraints From Weak Lensing Peak Statistics With CFHT Stripe 82 Survey
• Mergers Do Trigger AGNs out to z $\sim$ 0.6
• The Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel'dovich effect
• The SAMI Galaxy Survey: Global stellar populations on the size-mass plane
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• The XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters
• Constraints on the Alignment of Galaxies in Galaxy Clusters from $\sim$14,000 Spectroscopic Members
• VEGAS: A VST Early-type GAlaxy Survey. I. Presentation, wide-field surface photometry, and substructures in NGC 4472
• Towards emulating cosmic shear data: Revisiting the calibration of the shear measurements for the Kilo-Degree Survey
• First discoveries of z~6 quasars with the Kilo Degree Survey and VISTA Kilo-Degree Infrared Galaxy survey
• KiDS+GAMA: Intrinsic alignment model constraints for current and future weak lensing cosmology
• First test of Verlinde's theory of Emergent Gravity using Weak Gravitational Lensing measurements
• Intrinsic galaxy shapes and alignments II: Modelling the intrinsic alignment contamination of weak lensing surveys
• Galaxy And Mass Assembly (GAMA): Assimilation of KiDS into the GAMA database
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• Deep learning for galaxy surface brightness profile fitting
• The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey
• Observational Properties of Ultra-Diffuse Galaxies in the Field: Field-UDGs are Predominantly Blue and Starforming
• Source Selection for Cluster Weak Lensing Measurements in the Hyper Suprime-Cam Survey
• Evaluation of probabilistic photometric redshift estimation approaches for The Rubin Observatory Legacy Survey of Space and Time (LSST)
• HOLISMOKES -- II. Identifying galaxy-scale strong gravitational lenses in Pan-STARRS using convolutional neural networks
• Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples
• Photometric redshifts for the Kilo-Degree Survey. Machine-learning analysis with artificial neural networks
• Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids
• The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
• The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign. I. Overview and classification of candidates selected by two techniques
• Do current cosmological observations rule out all Covariant Galileons?
• KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes
• Galaxy-Galaxy Lensing in the DES Science Verification Data
• The Two-Halo Term in Stacked Thermal Sunyaev-Zel'dovich Measurements: Implications for Self-Similarity
• The masses of satellites in GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• Partially Acoustic Dark Matter Cosmology and Cosmological Constraints
• Bright galaxy sample in the Kilo-Degree Survey Data Release 4: selection, photometric redshifts, and physical properties
• The Growth of Intracluster Light in XCS-HSC Galaxy Clusters from $0.1<z<0.5$
• Morpho-z: improving photometric redshifts with galaxy morphology
• Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS
• Blasts from the Past: Supernova Shock Breakouts among X-Ray Transients in the XMM-Newton Archive
• Deblending galaxy superpositions with branched generative adversarial networks
• Weak-Lensing Mass Calibration of the Atacama Cosmology Telescope Equatorial Sunyaev-Zeldovich Cluster Sample with the Canada-France-Hawaii Telescope Stripe 82 Survey
• Photometric classification of emission line galaxies with Machine Learning methods
• The road ahead of Horndeski: cosmology of surviving scalar-tensor theories
• Enhancing BOSS bispectrum cosmological constraints with maximal compression
• Machine Learning based photometric redshifts for the KiDS ESO DR2 galaxies
• The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3
• Improving Photometric Redshift Estimation using GPz: size information, post processing and improved photometry
• Wide-Field Lensing Mass Maps from DES Science Verification Data
• KiDS-SQuaD II: Machine learning selection of bright extragalactic objects to search for new gravitationally lensed quasars
• Game of cones: A nulling strategy for modelling lensing convergence in cones with large deviation theory
• The Impact of Magnification and Size Bias on Weak Lensing Power Spectrum and Peak Statistics
• The Fornax Deep Survey with VST. IX. The catalog of sources in the FDS area, with an example study for globular clusters and background galaxies
• Investigating Deep Learning Methods for Obtaining Photometric Redshift Estimations from Images
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Unbiased methods for removing systematics from galaxy clustering measurements
• KiDS-1000: Cosmology with improved cosmic shear measurements
• Cosmological constraints from a joint analysis of cosmic microwave background and spectroscopic tracers of the large-scale structure
• Deep Learning for Strong Lensing Search: Tests of the Convolutional Neural Networks and New Candidates from KiDS DR3
• Quasar lenses and pairs in the VST-ATLAS and Gaia
• The quiescent fraction of isolated low surface brightness galaxies: Observational constraints
• A direct measurement of tomographic lensing power spectra from CFHTLenS
• Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 square degrees of KiDS weak lensing data
• Impact of theoretical priors in cosmological analyses: the case of single field quintessence
• Probing dark energy with tomographic weak-lensing aperture mass statistics
• KiDS-Legacy calibration: unifying shear and redshift calibration with the SKiLLS multi-band image simulations
• Support Vector Machine classification of strong gravitational lenses
• Galaxy and Mass Assembly (GAMA): Variation in Galaxy Structure Across the Green Valley
• AMICO galaxy clusters in KiDS-DR3: Constraints on cosmological parameters and on the normalisation of the mass-richness relation from clustering
• Robust Strong Lensing Time Delay Estimation
• Effects of baryons on weak lensing peak statistics
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck II: Cross-correlation measurements and cosmological constraints
• Detection and Removal of Artifacts in Astronomical Images
• Cross-correlation of weak lensing and gamma rays: implications for the nature of dark matter
• CFHTLenS: A Weak Lensing Shear Analysis of the 3D-Matched-Filter Galaxy Clusters
• Persistent homology in cosmic shear II: A tomographic analysis of DES-Y1
• Data-driven, interpretable photometric redshifts trained on heterogeneous and unrepresentative data
• A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties derived from the SED Fitting with Optical, Infrared, and Radio Data
• KiDS-i-800: Comparing weak gravitational lensing measurements in same-sky surveys
• The eROSITA Final Equatorial-Depth Survey (eFEDS): A multiwavelength view of WISE mid-infrared galaxies/active galactic nuclei
• The WaZP galaxy cluster sample of the Dark Energy Survey Year 1
• North Ecliptic Pole merging galaxy catalogue
• Prospects of testing late-time cosmology with weak lensing of gravitational waves and galaxy surveys
• The two-loop bispectrum of large-scale structure
• The DESI $N$-body Simulation Project I: Testing the Robustness of Simulations for the DESI Dark Time Survey
• A New Method for Wide-Field Near-IR Imaging with the Hubble Space Telescope
• Simulation tests of galaxy cluster constraints on chameleon gravity
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• Statistical uncertainties and systematic errors in weak lensing mass estimates of galaxy clusters
• Probing galaxy bias and intergalactic gas pressure with KiDS Galaxies-tSZ-CMB lensing cross-correlations
• Photometric redshifts with machine learning, lights and shadows on a complex data science use case
• Cross-correlation between Subaru Hyper Suprime-Cam Galaxy Weak Lensing and Planck Cosmic Microwave Background Lensing
• Surrogate modelling the Baryonic Universe I: The colour of star formation
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• Producing a BOSS-CMASS sample with DES imaging
• Fast Generation of Covariance Matrices for Weak Lensing
• A Spectroscopically Confirmed Double Source Plane Lens System in the Hyper Suprime-Cam Subaru Strategic Program
• Hierarchical modeling and statistical calibration for photometric redshifts
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• 3D Weak Gravitational Lensing of the CMB and Galaxies
• Multi-color detection of gravitational arcs
• Luminous red galaxies in the Kilo Degree Survey: selection with broad-band photometry and weak lensing measurements
• CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
• Angular ellipticity correlations in a composite alignment model for elliptical and spiral galaxies and inference from weak lensing
• Discovery of three strongly lensed quasars in the Sloan Digital Sky Survey
• Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising maps
• The frequency of dust lanes in edge-on spiral galaxies identified by Galaxy Zoo in KiDS imaging of GAMA targets
• The observability of galaxy merger signatures in nearby gas-rich spirals
• The PAU Survey: narrowband photometric redshifts using Gaussian processes
• The PAU Survey: Intrinsic alignments and clustering of narrow-band photometric galaxies
• A quasar hiding behind two dusty absorbers. Quantifying the selection bias of metal-rich, damped Lyman-alpha absorption systems
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• The Effect of Minor and Major Mergers on the Evolution of Low Excitation Radio Galaxies
• Mitigating the effects of undersampling in weak lensing shear estimation with metacalibration
• Higher order statistics of shear field: a machine learning approach
• Galaxy morphoto-Z with neural Networks (GaZNets). I. Optimized accuracy and outlier fraction from Imaging and Photometry
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• Sufficiency of a Gaussian power spectrum likelihood for accurate cosmology from upcoming weak lensing surveys
• Analytic marginalization of $N(z)$ uncertainties in tomographic galaxy surveys
• Finding Strong Gravitational Lenses Through Self-Attention
• Self-consistent bulge/disk/halo galaxy dynamical modeling using integral field kinematics
• Detection of Cosmic Magnification via Galaxy Shear -- Galaxy Number Density Correlation from HSC Survey Data
• Cosmology through arc statistics I: sensitivity to ${\Omega }_m$ and ${\sigma }_8$
• Reproducible $k$-means clustering in galaxy feature data from the GAMA survey
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• Cosmological Probes of Structure Growth and Tests of Gravity
• Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree Survey
• The PAU Survey: Measurements of the 4000 Å spectral break with narrow-band photometry
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Mapping dark matter on the celestial sphere with weak gravitational lensing
• Do galaxy mergers prefer under-dense environments?
• Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
• Weak Gravitational Lensing Shear Estimation with Metacalibration for the Roman High-Latitude Imaging Survey
• Intrinsic and extrinsic correlations of galaxy shapes and sizes in weak lensing data
• ASKAP Commissioning Observations of the GAMA 23 Field
• Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies
• Mixture Models for Photometric Redshifts
• Constraints on Dark Energy Models Using Late Universe Probes
• Early dark energy constraints with late-time expansion marginalization
• An adapted filter function for density split statistics in weak lensing
• Simulation-based inference of deep fields: galaxy population model and redshift distributions
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• Galaxy And Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
• Optimising Spectroscopic and Photometric Galaxy Surveys: Same-sky Benefits for Dark Energy and Modified Gravity
• Wide Area VISTA Extra-galactic Survey (WAVES): Unsupervised star-galaxy separation on the WAVES-Wide photometric input catalogue using UMAP and $\mathrm{HDBSCAN}$
• Weak Gravitational Lensing Systematics from Image Combination
• CosmoDM and its application to Pan-STARRS data
• The first shear measurements from precision weak lensing
• Galaxy And Mass Assembly: Galaxy Zoo spiral arms and star formation rates
• The mass-size relation of galaxy clusters
• Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
• TEGLIE: Transformer encoders as strong gravitational lens finders in KiDS
• Reconstructing the projected gravitational potential of galaxy clusters from galaxy kinematics
• Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
• Galaxy And Mass Assembly (GAMA): Self-Organizing Map Application on Nearby Galaxies
• Weak Lensing Measurement of Filamentary Structure with the SDSS BOSS and Subaru Hyper Suprime-Cam Data
• Initial results from a laboratory emulation of weak gravitational lensing measurements
• Simulation-Based Inference Benchmark for Weak Lensing Cosmology
• The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey Galaxy Cluster Catalogue
• Cross-correlation between $Planck$ CMB lensing potential and galaxy catalogues from HELP
• The gravitational and lensing-ISW bispectrum of 21cm radiation
• Mass-Richness relations for X-ray and SZE-selected clusters at $0.4<z<2.0$ as seen by $Spitzer$ at 4.5$\mu$m
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Constraints on the Spacetime Dynamics of an Early Dark Energy Component
• Dark Energy Survey Year 6 Results: Cell-based Coadds and Metadetection Weak Lensing Shape Catalogue
• The Loneliest Galaxies in the Universe: A GAMA and GalaxyZoo Study on Void Galaxy Morphology
• Distinguishing Coupled Dark Energy Models with Neural Networks
• Probing star formation and ISM properties using galaxy disk inclination III: Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
• A Comparative Study of Convolutional Neural Networks for the Detection of Strong Gravitational Lensing
• Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at $z=$ 4.5-8.5
• Forecasting Super-Sample Covariance in Future Weak Lensing Surveys with SuperSCRAM
• The PAU Survey: Photometric redshift estimation in deep wide fields
• Galaxy cluster optical mass proxies from probabilistic memberships
• Shear Nulling after PSF Gaussianisation: moment-based weak lensing measurements with subpercent noise bias
• Euclid preparation. XXXI. The effect of the variations in photometric passbands on photometric-redshift accuracy
• Intrinsic alignments of galaxies around cosmic voids
• The Observable Supernova Rate in Galaxy-Galaxy Lensing Systems with the TESS Satellite
• Emergent gravity fails to explain color-dependent galaxy-galaxy lensing signals from SDSS Dr7
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• Analysis of biasing from noise from the Nancy Grace Roman Space Telescope: implications for weak lensing
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• Data challenges as a tool for time-domain astronomy
• The Impact of Photometric Redshift Errors on Lensing Statistics in Ray-Tracing Simulations
• Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
• E/B mode decomposition of HSC-Y1 cosmic shear using COSEBIs: cosmological constraints and comparison with other two-point statistics
• Determining the time before or after a galaxy merger event
• A rising tide: Intrinsic alignments since the turn of the millennium
• High-resolution imaging follow-up of doubly imaged quasars
• Hypercompact stellar clusters: morphological renditions and spectro-photometric models
• High-$z$ Universe probed via Lensing by QSOs (HULQ) I. Number Estimates of QSO-QSO and QSO-Galaxy Lenses
• Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
• Dynamical cluster masses from photometric surveys
• Revealing new high redshift quasar populations through Gaussian mixture model selection
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Learning Spectral Templates for Photometric Redshift Estimation from Broadband Photometry
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Compressing combined probes: redshift weights for joint lensing and clustering analyses
• Total and dark mass from observations of galaxy centers with Machine Learning
• Cosmological Inference with Cosmic Voids and Neural Network Emulators
• A Model for the Redshift-Space Galaxy 4-Point Correlation Function
• CFHTLenS: Galaxy bias as function of scale, stellar mass, and colour. Conflicts with predictions by semi-analytic models
• On the effect of projections on convergence peak counts and Minkowski functionals
• Cosmological signatures of a Rapid Diluted Energy Density
• A Method for Unmasking Incomplete Astronomical Signals: Application to CO Multi-line Imaging of Nearby Galaxies Project
• Reconstruction of weak lensing mass maps for non-Gaussian studies in the celestial sphere
• Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA
• HI Intensity Mapping with the MIGHTEE Survey: First Results of the HI Power Spectrum
• CLAP. I. Resolving miscalibration for deep learning-based galaxy photometric redshift estimation
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• $\mathtt{ComEst}$: a Completeness Estimator of Source Extraction on Astronomical Imaging
• Synthetic Galaxy Clusters and Observations Based on Dark Energy Survey Year 3 Data
• Transformers as Strong Lens Detectors- From Simulation to Surveys
• Three-Dimensional Reconstruction of Weak Lensing Mass Maps with a Sparsity Prior. I. Cluster Detection
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• Weak Lensing Reconstruction by Counting DECaLS Galaxies
• Multi-band analysis of strong gravitationally lensed post-blue nugget candidates from the Kilo-Degree Survey
• The mass distribution in an assembling super galaxy group at $z=0.37$
• Euclid preparation. LXVII. Deep learning true galaxy morphologies for weak lensing shear bias calibration
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Weak Gravitational Lensing
• FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
• Probing gravity with the DES-CMASS sample and BOSS spectroscopy
• Quantifying the Detectability of Milky Way Satellites with Image Simulations: a Case Study with KiDS
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
• DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
• Galaxy-galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
• Cosmic shear nulling as a geometrical cosmological probe: Methodology and sensitivity to cosmological parameters and systematics
• The SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts
• Probing Time-Dependent Dark Energy with the Flux Power Spectrum of the Lyman $\alpha$ Forest
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• A data compression and optimal galaxy weights scheme for Dark Energy Spectroscopic Instrument and weak lensing datasets
• Chasing the peak: optimal statistics for weak shear analyses
• Neural Networks for cosmological model selection and feature importance using Cosmic Microwave Background data
• Optical+NIR analysis of a Newly Confirmed Einstein ring at z$\sim$1 from the Kilo-Degree Survey: Dark matter fraction, total and dark matter density slope and IMF
• Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
• Quantifying the impact of detection bias from blended galaxies on cosmic shear surveys
• Using Deep Learning Methods to Detect for Ultra-diffuse Galaxies in KiDS
• Cosmic magnification on high-redshift submillimeter galaxies
• On the Dusty Proximate Damped Lyman-α System toward Q2310-3358 at z = 2.40
• Galaxy And Mass Assembly (GAMA): The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field
• CNN photometric redshifts in the SDSS at $r\le 20$
• Intrinsic alignments of galaxies in multiple projections
• Photometric redshifts for quasars from WISE-PS1-STRM
• Galaxy And Mass Assembly: A Comparison between Galaxy-Galaxy Lens Searches in KiDS/GAMA
• $\text{SBi3PCF:}$ Simulation-based inference with the integrated 3PCF
• The effect of spiral arms on the Sérsic photometry of galaxies
• Spectral distortions in the decaying QCD dark matter scenario
• Ringing the universe with cosmic emptiness: void properties through a combined analysis of stacked weak gravitational and Doppler lensing
• Euclid: Improving redshift distribution reconstruction using a deep-to-wide transfer function
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• Hybrid-z: Enhancing Kilo-Degree Survey bright galaxy sample photometric redshifts with deep learning
• GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference
• Towards including super-sample covariance in the unbinned likelihood for cluster abundance cosmology
• Identification of gravitational lenses obscured by foreground light in the KiDS dataset using U-Nets and ResNets
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation
• TOPz: Photometric redshifts using template fitting applied to the GAMA survey
• Deep ASKAP EMU Survey of the GAMA23 field: Properties of radio sources