“…During the preparation of this manuscript, some of the LOTAAS pulsars were presented as independent discoveries by Tyul'bashev et al (2016Tyul'bashev et al ( , 2017 2017), who report 18 new pulsars, of which ten match the sky position, spin period, and DM of LOTAAS pulsars (PSRs J0121+14, J0811+37, J0935+33, J1529+40, J1635+23, J1638+40, J1657+33, J1953+30, J2051+12 and J2350+31). Again using the same telescope and instrumentation, 25 RRAT candidates, discovered through their single pulses, were published by Tyul'bashev et al (2018). Although the Puschino sky positions and DMs have considerable uncertainties, it appears Tyul'bashev et al ( 2018) detect single pulses from PSRs J0139+33, J0317+13, J1404+11, J1740+27, J1848+15, J2051+12 and J2209+22 (note that J2051+12 is also presented by Tyul'bashev et al 2017).…”