  Our paper presents the results of the second census of pulsars in decametre
wave range at UTR-2 radio telescope. Over the past ten years, the number of
discovered nearby pulsars in the world has doubled, which has made it urgent to
search for a low-frequency radio emission from newly discovered sources. To
increase this census sensitivity, the integration time was doubled compared
with the first census of 2010-2013. As a result, the decametre radio emission
of 20 pulsars was detected, their flux densities and the shape of pulses were
obtained. The dispersion measure for 10 pulsars and the rotation period for 8
pulsars were refined. For several pulsars the scattering time constant and FWHM
were estimated in decametre wave range. Upper limits of flux densities of 102
not yet detected pulsars were also estimated.
