SPHERE/IFS reduced data for HD 112810. Here, we show an image with all data epochs and all wavelengths co-added, with the GRAPHIC/PCA (left) and ANDROMEDA (right) algorithms applied to remove stellar speckles. In both cases, these are S/N maps; for GRAPHIC/PCA each annulus is scaled by the variance in that annulus, causing sharp transitions between concentric annuli. We tried several data reduction approaches and varied the values of tuned parameters. While a few bright spots are seen very close to the inner working angle, these are detected at low significance and are not at consistent locations between epochs – indicating that these are residual stellar speckles. The disk signal is not visible in any IFS data, either in the individual or in the co-added epochs.