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The Future of Pulsar Research and Facilities

Published online by Cambridge University Press:  04 June 2018

Matthew Bailes
Matthew Bailes*
Affiliation:
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, H11 PO Box 218, Hawthorn, Australia, 3122 email: [email protected] ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav)
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Abstract

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Radio pulsars have been responsible for many astonishing astrophysical and fundamental physics breakthroughs since their discovery 50 years ago. In this review I will discuss many of the highlights, most of which were only possible because of the provision of large-scale observing facilities. The next 50 years of pulsar astronomy can be very bright, but only if our governments properly plan and fund the infrastructure necessary to enable future discoveries. Being a small sub-field of astronomy places an onus on the pulsar community to have an open-source/open access approach to data, software, and major observing facilities to enable new groups to emerge to keep the field vibrant.

Keywords

pulsarsradio pulsarsradio telescopes
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S337: Pulsar Astrophysics the Next Fifty Years , September 2017 , pp. 165 - 170
Copyright
Copyright © International Astronomical Union 2018 

References

Alpar, M. A., et al. (1982), Nature, 300, 728.CrossRefGoogle Scholar
Antoniadis, M. A., et al. (2013), Science, 340, 448.CrossRefGoogle Scholar
Archibald, A., et al. (2009), Science, 324, 1411.CrossRefGoogle Scholar
Backer, D. C., et al. (1982), Nature, 300, 615.CrossRefGoogle Scholar
Bailes, M., (1989), ApJ, 342, 917.CrossRefGoogle Scholar
Bailes, M., et al. (2017), PASA, in press.Google Scholar
Burgay, M., (2003), Nature, 426, 531.CrossRefGoogle Scholar
Cordes, J., Romani, R. & Lundgren, S. (1993), Nature, 362, 133.CrossRefGoogle Scholar
Demorest, P., et al. (2010), Nature, 467, 1081.CrossRefGoogle Scholar
Foster, R., et al. (1993), ApJ, 410, 91.CrossRefGoogle Scholar
Fruchter, A., et al. (1988), Nature, 333, 237.CrossRefGoogle Scholar
Hewish, A., et al. (1968), Nature, 217, 709-713.CrossRefGoogle Scholar
Hessels, J. W. T., et al. (2006), Science, 311, 1901.CrossRefGoogle Scholar
Hulse, R. & Taylor, J. H. (1974), ApJ, 191, 59.CrossRefGoogle Scholar
Hulse, R. & Taylor, J. H. (1975), ApJ, 195, 51.CrossRefGoogle Scholar
Jacoby, B. A., et al. (2003), ApJ, 599, 99.CrossRefGoogle Scholar
Jacoby, B. A., et al. (2009), ApJ, 699, 2009.CrossRefGoogle Scholar
Johnston, S., et al. (1992) ApJ, 387, 37.CrossRefGoogle Scholar
Johnston, S., et al. (1993) Nature, 361, 163.CrossRefGoogle Scholar
Kaspi, V. M., et al. (2000) ApJ, 543, 321.CrossRefGoogle Scholar
Kulkarni, S. R. (1986) ApJ, 306, 85.CrossRefGoogle Scholar
Large, M. I., Vaughan, A. E. & Mills, B. Y. (1968), Nature, 220, 753.CrossRefGoogle Scholar
Lyne, A. G., Anderson, B. & Salter, M., (1982) MNRAS, 201, 503.CrossRefGoogle Scholar
Lyne, A. G. & Lorimer, D. R., (1994) Nature, 369, 127.CrossRefGoogle Scholar
Lyne, A. G., et al. (1987) Nature, 328, 399.CrossRefGoogle Scholar
Lyne, A. G., et al. (2004) Science, 303, 1153.CrossRefGoogle Scholar
Lorimer, D. R., et al. (2007) Science, 318, 777.CrossRefGoogle Scholar
Manchester, R. N., et al. (1991) Nature, 352, 219.CrossRefGoogle Scholar
Radhakrishnan, V. & Manchester, R. N. (1968), Nature, 222, 228.CrossRefGoogle Scholar
Radhakrishnan, V. & Cooke, D. J. (1969), ApL, 3, 225.Google Scholar
Ransom, S. M., et al. (2005) Science, 307, 892.CrossRefGoogle Scholar
Ransom, S. M., et al. (2014) Nature, 505, 520.CrossRefGoogle Scholar
Spitler, L., et al. (2016) Science, 531, 202.Google Scholar
Staelin, D. H. & Reifenstein, (1968), Science, 162, 1481.CrossRefGoogle Scholar
Taylor, J. H., (1974) A&AS, 15, 367.Google Scholar
Thornton, D., et al. (2013) Science, 341, 53.CrossRefGoogle Scholar
Weisberg, J. M. & Taylor, J. H. (1984), PhRvL, 52, 1348.Google Scholar
Wolszczan, A. & Frail, D. A. (1992), Nature, 355, 145.CrossRefGoogle Scholar