paper

Long-term Observations of Three Nulling Pulsars

arXiv:1502.07675 · doi:10.1093/mnras/stv392

Abstract

We present an analysis of approximately 200 hours of observations of the pulsars J16345107, J17174054 and J18530505, taken over the course of 14.7 yr. We show that all of these objects exhibit long term nulls and radio-emitting phases (i.e. minutes to many hours), as well as considerable nulling fractions (NFs) in the range . PSR J17174054 is also found to exhibit short timescale nulls () and burst phases () during its radio-emitting phases. This behaviour acts to modulate the NF, and therefore the detection rate of the source, over timescales of minutes. Furthermore, PSR J18530505 is shown to exhibit a weak emission state, in addition to its strong and null states, after sufficient pulse integration. This further indicates that nulls may often only represent transitions to weaker emission states which are below the sensitivity thresholds of particular observing systems. In addition, we detected a peak-to-peak variation of in the spin-down rate of PSR J17174054, over timescales of hundreds of days. However, no long-term correlation with emission variation was found.

10 pages, 8 figures, accepted for publication in MNRAS

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Long-term Observations of Three Nulling Pulsars · wovepaper