LPPS pulsar profiles. For each pulsar, the catalog name, detected pulse period, detected DM, and reduced chi-squared significance (in parentheses) from the automated search fold are given. One full rotational cycle is shown. Some of the brightest pulsars were detected multiple times; only the highest signal-to-noise detection is shown here. Several of the pulse profiles show scattering tails, e.g., PSRs B0523+11, B0611+22, B2111+46, making them excellent sources for studies of the interstellar medium. In many cases the off-pulse baseline is not flat due to RFI that could not be completely excised.