Average pulse profiles for pulsars re-detected in LOTAS. Both pulsars found in the blind periodicity search and pulsars re-detected by folding on previously known ephemerides are shown. For each pulsar the name, period, reduced chi-squared (in brackets) and DM are quoted. The reduced chi-squared is a proxy for the signal-to-noise of the pulse profile and is reported by PRESTO. Periods marked with “(topo)” are topocentric values as produced by the direct folding feature of the pipeline (Sect. 4.4).