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Fig. B.1


All-sky representation (grayscale indicates flux density) of the TGSS ADR survey in aitoff projection, marking the sky area included in this data release. The missing coverage towards the south celestial pole is due to the declination limit of GMRT, as well as the two lowest TGSS declination rows which were very difficult to process. The missing pointings of a single observing session under very difficult ionospheric conditions are visible towards the western edge. Also noticable are the regions near extremely bright sources such as Cas A, Cen A and Cyg A, where imaging artifacts dominate the image background. This representation was created using Aladin (Bonnarel et al. 2000).

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