Example of a simulated galaxy processed with piXedfit. We show the synthetic images of GALEX, LSST, and Euclid for TNG275545 with the O1 orientation index. Observational effects were introduced to the original synthetic images from the TNG50-SKIRT Atlas database in the form of simulated noise and convolution with the PSF of the corresponding cameras. The FWHM of the PSF as well as the pixel size of the images are $5\stackrel{″}{.}05$ and $1\stackrel{″}{.}5$, respectively. The pixels are binned with piXedfit to increase the S/N of the spatially resolved SEDs.