Galactic latitude distributions of pulsars with DM < 30 pc/cm³ (Manchester et al. 2005) and the (probably) cosmic sources found in this work as a function of galactic longitude. The lower left panel shows galactic co-ordinates of the pulsars and transients. On the right one, the total histograms of the b distributions are presented. The number of pulsars in the globular clusters NGC 5904, Messier 3 (NGC 5272), NGC 362, and 47 Tucanae (NGC 104) is indicated by different types of hatching.