The radio-emitting neutron star population encompasses objects with spin periods ranging
from milliseconds to tens of seconds. As they age and spin more slowly, their radio emission …

We have observed 123 pulsars with periods longer than 0.1 s in the Meterwavelength Single
Pulse Polarimetric Emission Survey. In this work, a detailed study of the polarization …

Searching for periodic non-accelerated signals in the presence of ideal white noise using
the fully phase-coherent fast-folding algorithm (FFA) is theoretically established as a more …

The recent discovery of a radio-emitting neutron star with an ultralong spin period of 76 s,
PSR J0901-4046, raises a fundamental question on how such a slowly rotating magnetized …

We report the observations of single pulse emission from the pulsar B0809+ 74 at 150 MHz
using the Polish LOFAR station, PL-611. The three major phenomena of subpulse drifting …

Observations suggest that coherent radio emission from pulsars is excited in a dense pulsar
plasma by curvature radiation from charge bunches. Numerous studies propose that these …

We report on our investigation of the evolution of a system of spark discharges in the inner
acceleration region (IAR) above the pulsar polar cap. The surface of the polar cap is heated …

Context. Current wisdom suggests that the observed population of neutron stars are
manifestations of their birth scenarios and their thermal and magnetic field evolution …

A novel scheme has been developed to show that the observed phase behavior associated
with subpulse drifting from two pulsars, J1034− 3224 and J1720− 2933, can be used to …

We present an analysis of the subpulse drift in PSR J1750− 3503, which is characterized by
abrupt transitions of drift direction. As the pulsar does not exhibit other mode changes or …