Weak lensing, Big Magnification: Recovering hidden lensing information from galaxy positions
astro-ph.CO
Submitted: 2026-10-02
Updated: 2026-10-02
Terminology
Sources
- The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s
- AtLAST -- Cosmology with submillimetre galaxies magnification bias
- Enhancing weak lensing redshift distribution characterization by optimizing the Dark Energy Survey Self-Organizing Map Photo-z method
- Dark Energy Survey Year 6 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Cosmic magnification on multi-catalogue Herschel submillimetre galaxies
- Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample
- Dark Energy Survey Year 3 Results: Multi-Probe Modeling Strategy and Validation
- Dark Energy Survey Year 6 Results: improved mitigation of spatially varying observational systematics with masking for the MagLim++ lens sample
- The NumPy array: a structure for efficient numerical computation
- Dark Energy Survey Year 6 Results: MagLim++ Lens Sample Selection and Measurements of Galaxy Clustering
- Dark Energy Survey Year 6 Results: Redshift Calibration of the Weak Lensing Source Galaxies
- KiDS-1000 cosmic shear reanalysis using MetaCalibration
- Constraining the Stellar-to-Halo Mass Relation with Galaxy Clustering and Weak Lensing from DES Year 3 Data
- Anisotropic redshift distributions in photometric galaxy clustering and their cosmological impact
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