sgRNA junction counts obtained with sgDI-tector correlate with Finkel et al.’s junction counts obtained with STAR (panels A,B) while Periscope results show a lower correlation (panels C,D). Left (right) column contains the results for data at 5 (24) hpi. Only data for the first biological replicate are presented here. ORF 10 junctions are never found by both STAR and by DI-tector, while a single read has been detected by Periscope at 5 hpi. One pseudocount has been added to junctions which are not detected by one tool while being detected by the other. The black dashed line is the diagonal line, added to ease the comparison between the different methods.
