Reconstruction of simulated strong lensing data of NGC 1300 from Birrer & Amara (2018). Top panels: data, distribution of the noise-weighted data residuals for both LensCharm and Lenstronomy where the gray dashed line depicts a standard normal distribution, input source, and distribution of the uncertainty weighted residuals of LensCharm evaluated at reconstructed source flux above 0.5 (from left to right). Middle panels: results of the LensCharm reconstruction: lensed source reconstruction, residuals between the lensed light and the data, source reconstruction, and residuals between the input source and the LensCharm reconstruction (from left to right). Bottom panels: results of the Lenstronomy reconstruction, which follow the same order as the middle panels.