Dataset: Measuring the Gravitational Response to Structure

This archive contains the data products, analysis outputs, and code used in Chaplin (2026), Measuring the Gravitational Response, which empirically quantifies a scale-selective and structure-conditioned gravitational lensing response using CMB lensing (κ) and large-scale structure tracers. The dataset includes: Processed κ×δg cross-correlation outputs Structure-conditioned response metrics Dark-matter-compatible null test ensembles Rotation, masking, and scale-localization diagnostics Scripts required to reproduce all reported figures and summary statistics The archive is intended to support independent replication, robustness testing, and alternative theoretical interpretation. No specific gravitational or dark-matter model is assumed by the data products themselves.