Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-22T17:17:26.824Z Has data issue: false hasContentIssue false
  • English
  • Français

The Green Bank North Celestial Cap Pulsar Survey: Status and Future

Published online by Cambridge University Press:  04 June 2018

Ryan S. Lynch
Ryan S. Lynch*
Affiliation:
Green Bank Observatory, PO Box 2, Green Bank, WV, 24944, USA email: [email protected] Center for Gravitational Waves and Cosmology, Department of Physics and Astronomy, West Virginia University, White Hall, Box 6315, Morgantown, WV 26506, USA
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 ongoing Green Bank North Celestial Cap pulsar survey is using the Green Bank Telescope to search for pulsars and transients over 85% of the celestial sphere. The survey has resulted in over 150 new pulsars, among which are high-precision millisecond pulsars, several binary pulsars, including at least one relativistic double neutron star system, nulling pulsars, and several nearby millisecond pulsars. We find no fast radio bursts in the survey to date. We present these results and discuss the future prospects for the survey.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S337: Pulsar Astrophysics the Next Fifty Years , September 2017 , pp. 13 - 16
Copyright
Copyright © International Astronomical Union 2018 

References

Archibald, A. M., Stairs, I. H., Ransom, S. M., et al. 2009, Science, 324, 1411Google Scholar
Chawla, P., Kaspi, V. M., Josephy, A., et al. 2017, ApJ, 844, 140Google Scholar
Crawford, F., Rane, A., Tran, L., et al. 2016, MNRAS, 460, 3370CrossRefGoogle Scholar
Hellings, R. W., & Downs, G. S., 1983, ApJ, 265, L39Google Scholar
Kaplan, D. L., Bhalerao, V. B., van Kerkwijk, M. H., et al. 2013, ApJ, 765, 158Google Scholar
Kaplan, D. L., Stovall, K., Ransom, S. M., et al. 2012, ApJ, 753, 174Google Scholar
Lorimer, D. R., Bailes, M., McLaughlin, M. A., Narkevic, D. J., & Crawford, F., 2007, Science, 318, 777Google Scholar
Lynch, R. S., et al. in prep.Google Scholar
Lyne, A. G., Burgay, M., Kramer, M., et al. 2004, Science, 303, 1153Google Scholar
Manchester, R. N., IPTA., 2013, Classical and Quantum Gravity, 30, 224010Google Scholar
McLaughlin, M. A., 2013, Classical and Quantum Gravity, 30, 224008Google Scholar
McLaughlin, M. A., Lyne, A. G., Lorimer, D. R., et al. 2006, Nature, 439, 817Google Scholar
Ransom, S. M., Stairs, I. H., Archibald, A. M., et al. 2014, Nature, 505, 520Google Scholar
Stovall, K., Lynch, R. S., Ransom, S. M., et al. 2014, ApJ, 791, 67CrossRefGoogle Scholar
Thornton, D., Stappers, B., Bailes, M., et al. 2013, Science, 341, 53Google Scholar
van Haarlem, M. P., Wise, M. W., Gunst, A. W., et al. 2013, A&A, 556, A2Google Scholar