Tyul'bashev, S.A.S.A.Tyul'bashevTyul'bashev, V.S.V.S.Tyul'bashevKitaeva, M.A.M.A.KitaevaChernyshova, A.I.A.I.ChernyshovaMalofeev, V.M.V.M.MalofeevChashei, I.V.I.V.ChasheiShishov, V.I.V.I.ShishovDagkesamanskii, R.D.R.D.DagkesamanskiiKlimenko, S.V.S.V.KlimenkoNikitin, I.N.I.N.NikitinNikitina, L.D.L.D.Nikitina2022-03-052022-03-052017https://publica.fraunhofer.de/handle/publica/25073810.1134/S1063772917100109In the course of monitoring interplanetary scintillations of a large number of sources using the Big Scanning Antenna of the Lebedev Physical Institute, a search for pulsars with periods >0.4 s at declinations &#8722;9CR < d < 42CR and right ascensions 0h < a < 24h was simultaneously carried out. The search was conducted using four years of observations carried out at 110.25MHz in six frequency channels making up a 2.5 MHz band and having a time resolution of 100 ms. The initial identification of pulsar candidates was done using Fourier power spectra averaged over the entire observational period; the pulsar candidates were then verified using observations with higher frequency and time resolution: 32 frequency channels and a time resolution of 12.5 ms. Eighteen new pulsars were discovered in the studied area, whose main characteristics are presented.en003journal article