Notes. Pulsar names in bold are newly discovered pulsars, the first two rows contain unique LOFAR discoveries and the other pulsars with bold names signify independent discoveries – i.e. unpublished sources recently found by competing surveys such as the GBNCC (Stovall et al. 2014). The M column contains the method through which the pulsar was detected: (p) in the blind periodicity search, (d) through folding on a known ephemeris, and (s) by inspecting condensed single-pulse plots. The α column gives the distance to the center of the nearest tied-array beam. These distances are based on the ATNF catalog value. For the LOTAS discoveries the timing position was used. The DMs and periods quoted are taken from the PRESTO diagnostics of the folds; these values were optimized during the folding process in order to maximize the S/N. There is no error or digit significance information for these. The columns S/N_p and S/N_cum quote respectively the peak and cumulative S/N if they could be derived automatically. The S/N were derived from profiles with 100 bins. The S/N_s column contains the S/N of the brightest single pulse detected, possibly in another beam than the periodicity search detection.