The Three Discrete Nulling Timescales of PSR J1717-4054

TL;DR

This study investigates PSR J1717-4054, revealing three discrete nulling timescales and detailed pulsar properties, bridging the gap between classical nullers and long-term intermittent pulsars.

Contribution

The paper identifies and characterizes three distinct nulling timescales in PSR J1717-4054 and provides comprehensive measurements of its fundamental properties.

Findings

Nulls occur on three discrete timescales: hours, thousands of rotations, and tens of rotations.

No subpulse structure or flux variation during active states.

Stringent limits on emission during inactive states (<0.1% of active flux).

Abstract

PSR J1717-4054 is one of the small class of pulsars which null on intermediate (~hour) timescales. Such pulsars represent an important link between classical nullers, whose emission vanishes for a few rotations, and the intermittent pulsars which null for months and years. Using the Parkes radio telescope and the Australia Telescope Compact Array, we have studied the emission from PSR J1717-4054 over intervals from single pulses to years. We have identified and characterised nulling at three discrete timescales: the pulsar emits during "active states" separated by nulls lasting many thousands of rotations, while active states themselves are interrupted by nulls with a bimodal distribution of durations; one to two rotations, or tens of rotations. We detect no subpulse structure or flux density variations during active states, and we place stringent limits (<0.1% of the mean active flux density) on pulsed emission during inactive states. Finally, our high-quality data have also allowed us to measure for the first time many important properties of PSR J1717-4054, including its position, spindown rate, spectrum, polarization characteristics, and pulse broadening in the interstellar medium.