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Searching for pulsars in future radio continuum surveys

Published online by Cambridge University Press:  04 June 2018

Shi Dai ,
Simon Johnston  and
George Hobbs
Shi Dai*
Affiliation:
CSIRO Astronomy and Space Science, Australia Telescope National Facility, PO Box 76, Epping, NSW, Australia
Simon Johnston
Affiliation:
CSIRO Astronomy and Space Science, Australia Telescope National Facility, PO Box 76, Epping, NSW, Australia
George Hobbs
Affiliation:
CSIRO Astronomy and Space Science, Australia Telescope National Facility, PO Box 76, Epping, NSW, Australia
*
*email: [email protected]
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Abstract

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Radio continuum surveys are equally sensitive to all pulsars, not affected by dispersion measure smearing, scattering or orbital modulation of spin periods, and therefore allow us to search for extreme pulsars, such as sub-millisecond pulsars, pulsar-black hole systems and pulsars in the Galactic Centre. As we move towards the Square Kilometre Array (SKA) era, searching for pulsars in continuum images will complement conventional pulsar searches, and make it possible to find extreme objects.

Keywords

methods: observational - pulsars: general - radio continuum: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S337: Pulsar Astrophysics the Next Fifty Years , September 2017 , pp. 328 - 329
Copyright
Copyright © International Astronomical Union 2018 

References

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