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Erratum: Beating the Spin-down Limit on Gravitational Wave Emission from the Crab Pulsar (Astrophysical Journal (2008) 683 (L45))
Astrophysical Journal
  • B. Abbott, California Institute of Technology
  • R. Abbott, California Institute of Technology
  • R. Adhikari, California Institute of Technology
  • P. Ajith, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • B. Allen, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • G. Allen, Stanford University
  • R. Amin, Louisiana State University
  • S. B. Anderson, California Institute of Technology
  • W. G. Anderson, University of Wisconsin-Milwaukee
  • M. A. Arain, University of Florida
  • M. Araya, California Institute of Technology
  • H. Armandula, California Institute of Technology
  • P. Armor, University of Wisconsin-Milwaukee
  • Y. Aso, Columbia University in the City of New York
  • S. Aston, University of Birmingham
  • P. Aufmuth, Gottfried Wilhelm Leibniz Universität Hannover
  • C. Aulbert, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • S. Babak, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • S. Ballmer, California Institute of Technology
  • H. Bantilan, Carleton College, USA
  • B. C. Barish, California Institute of Technology
  • C. Barker, LIGO Hanford
  • D. Barker, LIGO Hanford
  • B. Barr, University of Glasgow
  • P. Barriga, The University of Western Australia
  • M. A. Barton, University of Glasgow
  • M. Bastarrika, University of Glasgow
  • K. Bayer, Massachusetts Institute of Technology
  • J. Betzwieser, California Institute of Technology
  • P. T. Beyersdorf, San Jose State University
  • I. A. Bilenko, Lomonosov Moscow State University
  • Tiffany Z. Summerscales, Andrews University
Document Type
Article
Publication Date
1-1-2009
Abstract

A processing error in the signal template used in this search led to upper limits about 30% lower than we now know is warranted by the early S5 data. We have re-analyzed that data and find new upper limits on the strain parameter h 0 of 4.9 × 10-25/3.9 × 10-25 for uniform/restricted prior assumptions concerning the Crab inclination and polarization angles. These results have now been superseded by upper limits of 2.6 × 10-25/2.0 × 10-25 based on the full S5 data and presented in Abbott et al. (2009). The multitemplate search was not affected by the error. © 2009. The American Astronomical Society.

DOI
https://doi.org/10.1088/0004-637X/706/1/L203
First Department
Physics
Citation Information
B. Abbott, R. Abbott, R. Adhikari, P. Ajith, et al.. "Erratum: Beating the Spin-down Limit on Gravitational Wave Emission from the Crab Pulsar (Astrophysical Journal (2008) 683 (L45))" Astrophysical Journal Vol. 706 Iss. 1 PART 2 (2009)
Available at: http://works.bepress.com/tiffany_summerscales/165/