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This paper derives accuracy standards for model gravitational waveforms required to ensure proper use of the Allen $\chi^2$ discriminator in gravitational wave (GW) data analysis.
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S. Babak, R. Biswas, P. R. Brady, D. A. Brown, K. Cannon, C. D. Capano, J. H. Clayton, T. Cokelaer, J. D. E. Creighton, T. Dent, A. Dietz, S. Fairhurst, N. Fotopoulos, G. González, C. Hanna, I. W. Harry, G. Jones, D. Keppel, D. J. A. McKechan, L. Pekowsky, S. Privitera, C. Robinson, A. C. Rodriguez, B. S. Sathyaprakash, A. S. Sengupta, M. Vallisneri, R. Vaulin, and A. J. Weinstein, Phys. Rev. D 87
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T. D. Canton, A. H. Nitz, A. P. Lundgren, A. B. Nielsen, T. D. Duncan A. Brown, I. W. Harry, B. Krishnan, A. J. Miller, K. Wette, K. Wiesner, and J. L. Willis, Phys. Rev. D 90
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B. P. Abbott, R. Abbott, T. D. Abbott, M. R. Abernathy, F. Acernese, K. Ackley, C. Adams, T. Adams, P. Addesso, R. X. Adhikari, and et al., Physical Review Letters 116
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The LIGO Scientific Collaboration and the Virgo Collaboration, Phys. Rev. Lett. , 221101 (2016)
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