The High Time Resolution Universe Survey - III. Single-pulse searches and preliminary analysis

TL;DR

The HTRU survey's single-pulse search method has discovered 11 new neutron stars and confirmed two others, revealing the dynamic nature of the radio sky and providing insights into various neutron star populations and their activity cycles.

Contribution

This paper introduces the HTRU survey's single-pulse search technique, initial results, and analysis of neutron star populations, highlighting improved sensitivity and new discoveries.

Findings

11 new neutron stars discovered

Confirmed two previously unconfirmed neutron stars

Supports many RRATs are high-null-fraction pulsars

Abstract

We present the search methods and initial results for transient radio signals in the High Time Resolution Universe (HTRU) Survey. The HTRU survey's single-pulse search, the software designed to perform the search, and a determination of the HTRU survey's sensitivity to single pulses are described. Initial processing of a small fraction of the survey has produced 11 discoveries, all of which are sparsely-emitting neutron stars, as well as provided confirmation of two previously unconfirmed neutron stars. Most of the newly discovered objects lie in regions surveyed previously, indicating both the improved sensitivity of the HTRU survey observing system and the dynamic nature of the radio sky. The cycles of active and null states in nulling pulsars, rotating radio transients (RRATs), and long-term intermittent pulsars are explored in the context of determining the relationship between these populations, and of the sensitivity of a search to the various radio-intermittent neutron star populations. This analysis supports the case that many RRATs are in fact high-null-fraction pulsars (i. e. with null fraction >~0.95), and indicates that intermittent pulsars appear distinct from nulling pulsars in their activity cycle timescales. We find that in the measured population, there is a deficit of pulsars with typical emission timescales greater than ~300 s that is not readily explained by selection effects. The HTRU low-latitude survey will be capable of addressing whether this deficit is physical. We predict that the HTRU survey will explore pulsars with a broad range of nulling fractions (up to and beyond 0.999), and at its completion is likely to increase the currently known RRATs by a factor of more than two.