Showing 21–40 of 96 results
/ Date/ Name
Apr 7, 2016Galaxy And Mass Assembly (GAMA): Accurate Panchromatic Photometry from Optical Priors using LAMBDARJul 3, 2020KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysisJan 12, 2018The SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star FormationAug 15, 2022A Unified Catalog-level Reanalysis of Stage-III Cosmic Shear SurveysSep 22, 2017KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics-I: Inference from Analytical Prediction of High Signal-to-Noise Ratio Convergence PeaksFeb 12, 2015Herschel-ATLAS: The Surprising Diversity of Dust-Selected Galaxies in the Local Submillimetre UniverseNov 23, 2018KiDS+GAMA: Intrinsic alignment model constraints for current and future weak lensing cosmologyMay 11, 2017Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function to $z=0.1$ from the r-band selected equatorial regionsDec 14, 2018KiDS+VIKING-450: Cosmic shear tomography with optical+infrared dataJul 30, 2020KiDS-1000 catalogue: Redshift distributions and their calibrationNov 6, 2018Luminous red galaxies in the Kilo Degree Survey: selection with broad-band photometry and weak lensing measurementsJan 11, 2022Rubin-Euclid Derived Data Products: Initial RecommendationsApr 20, 2023ACT-DR5 Sunyaev-Zel'dovich Clusters: weak lensing mass calibration with KiDSDec 15, 2020Organised Randoms: Learning and correcting for systematic galaxy clustering patterns in KiDS using self-organising mapsOct 22, 2021The dark matter halo masses of elliptical galaxies as a function of observationally robust quantitiesAug 30, 2020Clustering of red-sequence galaxies in the fourth data release ofthe Kilo-Degree SurveyFeb 6, 2021Halo shapes constrained from a pure sample of central galaxies in KiDS-1000Sep 30, 2016G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDARMay 16, 2024KiDS-1000 and DES-Y1 combined: Cosmology from peak count statisticsOct 11, 2019KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs