piXedfit provides a self-contained set of tools for analyzing spatially resolved properties of galaxies using imaging data or a combination of imaging data and the integral field spectroscopy (IFS) data. piXedfit has six modules that can handle all tasks in the analysis of the spatially resolved SEDs of galaxies, including images processing, a spatial-matching between reduced broad-band images with an IFS data cube, pixel binning, performing SED fitting, and making visualization plots for the SED fitting results.
https://ui.adsabs.harvard.edu/abs/2021ApJS..254...15A; ; if you use the pixel binning module (piXedfit_bin), please also cite https://ui.adsabs.harvard.edu/abs/2017MNRAS.469.2806A