Notes. Here we show the data we used to make Fig. 9. We note that some targets may have multiple observations. For consistency in the paper, we fixed our FoV (< 0.735″). It is possible to increase the FoV to detect more extended disks using RDI. The ADI and RDI detections only indicate the detection within our adopted FoV. We note that this table should not be treated as a complete result of disk detections by SPHERE/IRDIS in the dual-band mode using the H23 filter. because our FoV is limited and we only included archival data released before 2021 January 1. ^(a)The H-band magnitudes are adopted from Skrutskie et al. (2006) ^(b)The parameters used in the RDI reduction. The number of PCs used in the PCA subtraction and the number of reference images used in the reference library. ^(c)No clear disk structure was detected in the ADI image using a FoV of 0.735″ in radius. However, we indeed detected similar disk structures as the ADI-PCA image reported in Ginski et al. (2016) when we adopted a larger FoV of 1.2″ in the ADI-PCA subtraction.