spike generates and drizzles point-spread functions (PSFs) for space-based imaging instruments. It supports model and empirical PSF creation for instruments aboard the Hubble Space Telescope (HST), James Webb Space Telescope (JWST), and Nancy Grace Roman Space Telescope (Roman). Spike handles image ingestion, coordinate reading, PSF generation via TinyTim (ascl:1010.057) or WebbPSF/HST empirical methods, and correct drizzling or resampling to match final image processing.