Abstract
ABSTRACT In this paper, we present the results of the second census of pulsars in the decametre wave range at the Ukrainian T-shaped Radio telescope, second modification (UTR-2). Over the past 10 yr, the worldwide number of discovered nearby pulsars has doubled, which means that there is some urgency to search for a low-frequency radio emission from these newly discovered sources. To increase the sensitivity of this census, 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, and their flux densities and the shape of their pulses were obtained. The dispersion measures for 10 pulsars and the rotation periods for eight pulsars were refined. For several pulsars, the scattering time constant and FWHM were estimated in the decametre wave range. The upper limits of flux densities for 102 pulsars that have not yet been detected were also estimated.
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