Home List of Titles The High Time Resolution Universe Pulsar Survey III: single-pulse searches and preliminary analysis
Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/203139
|Download PDF (Accepted manuscript) (Adobe Acrobat PDF, 1 MB)|
- The High Time Resolution Universe Pulsar Survey III: single-pulse searches and preliminary analysis
- Burke-Spolaor, S.; Bailes, M.; Johnston, S.; Bates, S. D.; Bhat, N. D. R.; Burgay, M.; D'Amico, N.; Jameson, A.; Keith, M. J.; Kramer, M.; Levin, L.; Milia, S.; Possenti, A.; Stappers, B.; van Straten, W.
- 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 a null fraction of ≳0.95) and indicates that intermittent pulsars appear distinct from nulling pulsars in their activity cycle time-scales. We find that in the measured population, there is a deficit of pulsars with typical emission time-scales 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 2.
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing
- Monthly Notices of the Royal Astronomical Society, Vol. 416, no. 4 (Oct 2011), pp. 2465-2476
- Publication year
- FOR Code(s)
- 0201 Astronomical and Space Sciences
- Data analysis; Neutrons; Pulsars; Stars
- Wiley-Blackwell Publishing
- Publisher URL
- Copyright © 2011 The Authors. Journal compilation copyright © 2011 Royal Astronomical Society. The accepted manuscript is reproduced in accordance with the copyright policy of the publisher. The definitive publication is available at www.interscience.wiley.com.
- Research Projects
- Full text
- Peer reviewed