Notes. Sources marked with an asterisk were used to derive an estimate for the LPPS gain (see Sect. 3.2). The column headed by an M (method) lists how the pulsar was detected – through a periodicity search (p), through a direct fold using a known ephemeris (d), or through single-pulse searches (s). The next column, headed by α, lists the distance to the beam center in degrees at which the pulsar was detected (based on the ATNF pulsar database positions). The DM and period columns list the values as reported by PRESTO (without errors or digit significance) after folding the data on the known ephemeris using 256 bins. The next two columns report the peak and the cumulative S/N derived from the pulse profiles. For profiles where the off-pulse baseline is not flat (because of RFI), the signal-to-noise ratios are left blank. The last column shows the peak S/N of the brightest pulse found in the single-pulse search as reported by PRESTO (not corrected for zero-DM filtering).