Cross mission FERMI SWIFT

This new cross-mission dataset merges long-term observational assets from the Fermi Gamma-ray Space Telescope and the Neil Gehrels Swift Observatory into a unified multi-wavelength celestial time-series catalog. By pairing Fermi's transient trigger events (such as Gamma-Ray Bursts and Solar Flares) with Swift's corresponding instrument exposure profiles (across the BAT, XRT, and UVOT bands), the dataset synchronizes high-energy particle physics with wide-field electromagnetic telemetry. Consolidating these separate instrument logs into a continuous, sequentially ordered tracking array allows the pipeline to map astronomical coordinates and exposure stresses into dense, interlocking ribbon geometries, providing an expansive data horizon for tracking celestial events over a multi-year baseline.