Dimensionless logarithmic COSEBI (see Appendix B) measurements from KiDS-1000 data. The E and B modes are shown in the top and bottom triangles, respectively. Each panel depicts results for a pair of redshift bins, z − ij. The solid red curves correspond to the best fitting model to the SEK COSEBIs as analyzed in Asgari et al. (2021, compare with their Fig. 3). The B modes are consistent with zero (p-value = 0.36) and the best-fit model describes the data very well (p-value = 0.2). We note that the COSEBI modes are discrete and the points are connected to one another for visual aid.