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Pulsars play a crucial astrophysical role as the highly energetic compactradio, X-ray, and gamma-ray sources. Our previous works show that the radiopulsars found as the pulsing gamma sources by the Large Area Telescope (LAT) onthe board of the Fermi Gamma-Ray Space Telescope have high values of magneticfield near the light cylinder, two-three orders of magnitude stronger comparingwith the magnetic fields of radio pulsars: $\log B_{lc}$ (G) are 3.60-3.95 and1.75. Moreover, their losses of the rotation energy are also three ordershigher than the corresponding values for the main group of radio pulsars onaverage:$\log \dot E$ (erg/s) = 35.37-35.53 and 32.64. The correlation betweengamma-ray luminosities and radio luminosities is found. It allows us to selectthose objects from all set of the known radio pulsars that can be detected asgamma pulsars with the high probability. We give the list of such radio pulsarsand propose to search for gamma emisson from these objects. On the other hand,the known catalog of gamma pulsars contains some sources which are not known asradio pulsars at this moment. Some of them have the large values of gammaluminosities and according to the obtained correlation, we can expect markedradio emission from these objects. We give the list of such pulsars andexpected flux densities to search for radiation at frequencies 1400 and 111MHz.

Radio pulsars with expected gamma radiation and gamma pulsars as pulsating radio emitters