Erratum: Placing limits on the stochastic gravitational-wave background using European Pulsar Timing Array data

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ID: 271633
2012
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Abstract
This correction resolves a puzzling inconsistency: the excessive discrepancy of two orders of magnitude between results obtained with this analytic approximation and those of more detailed investigations (i.e. Ölmez, Mandic & Siemens ; Sanidas, Battye & Stappers ). In Sanidas et al. (), the authors presented an absolute upper limit on the string tension , using our limit on the amplitude of the stochastic gravitational wave background and taking into account the uncertainties involved in the cosmic string model parameters. The one order of magnitude difference between our revised constraint and their results is now well justified within the approximations of Damour & Vilenkin (). This is discussed in more detail by Sanidas et al. () and has recently been pointed out by Shlaer, Vilenkin & Loeb () as well.
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verbiest2012monthlyerratum: Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors R. Van Haasteren,Y. Levin,G. H. Janssen,K. Lazaridis,M. Kramer,B. W. Stappers,G. Desvignes,M. B. Purver,A. G. Lyne,R. D. Ferdman,A. Jessner,I. Cognard,G. Theureau,N. D'amico,A. Possenti,Marta Burgay,Alessandro Corongiu,J. W. T. Hessels,R. Smits,J. P. W. Verbiest;R. Van Haasteren;Y. Levin;G. H. Janssen;K. Lazaridis;M. Kramer;B. W. Stappers;G. Desvignes;M. B. Purver;A. G. Lyne;R. D. Ferdman;A. Jessner;I. Cognard;G. Theureau;N. D'amico;A. Possenti;Marta Burgay;Alessandro Corongiu;J. W. T. Hessels;R. Smits;J. P. W. Verbiest;
Journal monthly notices of the royal astronomical society
Year 2012
DOI
10.1111/j.1365-2966.2012.20916.x
URL
https://sciprofiles.com/publication/view/84e4bf43b5ac4ca6e400f3bbd6988877
Keywords
stochastic erratum gravitational placing limits european pulsar using european wave background pulsar timing timing array

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