Hostname: page-component-7bb8b95d7b-fmk2r Total loading time: 0 Render date: 2024-10-03T16:30:14.108Z Has data issue: false hasContentIssue false

1,000,000 Giant Pulses from the Crab Pulsar

Published online by Cambridge University Press:  04 June 2018

Mitchell B. Mickaliger
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK email: mitchell.mickaliger@manchester.ac.uk
Ben W. Stappers
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK email: mitchell.mickaliger@manchester.ac.uk
Cees G. Bassa
Affiliation:
ASTRON, The Netherlands Institute for Radio Astronomy, Postbus 2, NL-7990 AA Dwingeloo, The Netherlands
Aldus G. Fletcher
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK email: mitchell.mickaliger@manchester.ac.uk
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Crab pulsar was first detected soon after the discovery of pulsars, and has long been studied for its unique traits. One of these traits, giant pulses that can be upwards of 1000 times brighter than the average pulse, was key to the Crab’s initial detection. Giant pulses are only seen in a few pulsars, and their energy distributions distinguish them from normal pulsed emission. There have been many studies over a period of decades to measure the power-law slope of these energy distributions, which provide insight into the possible emission mechanism of these giant pulses.

The 42-foot telescope at Jodrell Bank Observatory monitors the Crab pulsar on a daily basis. We have single-pulse data dating back to 2012, containing roughly 1,000,000 giant pulses, the largest sample of Crab giant pulses to date. This large set of giant pulses allows us to do a range of science, including pulse-width studies and in-depth studies of giant-pulse energy distributions. The latter are particularly interesting, as close inspection of the high-energy tail of the energy distribution allows us to investigate the detectability of extragalactic giant-pulsing pulsars. Also, by calculating rates from these energy distributions, we may be able to shed light on a possible link between Fast Radio Bursts and giant pulses.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Cordes, J. M., & Wasserman, I., 2016, MNRAS, 457, 232Google Scholar
Weltevrede, P., 2016, A&A, 590, A109Google Scholar