We measure the extinction curves of 220 million stars with Gaia XP spectra and near-infrared photometry from 2MASS and WISE. We use a data-driven model that is developed from 2023MNRAS.524.1855Z, with variable extinction curves, to determine stellar parameters and extinction curves simultaneously.
For bulk downloads and the trained model, see https://doi.org/10.5281/zenodo.10719756.