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2009

Use and Abuse of the Model Waveform Accuracy Standards

Lindblom, Lee

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Accuracy standards have been developed to ensure that the waveforms used for gravitational-wave data analysis are good enough to serve their intended purposes.

These standards place constraints on certain norms of the frequency-domain representations of the waveform errors.
Examples are given here of possible misinterpretations and misapplications of these standards, whose effect could be to vitiate the quality control they were intended to enforce.
Suggestions are given for ways to avoid these problems.

Use and Abuse of the Model Waveform Accuracy Standards · Around

Built on

A. Lazzarini and R. Weiss, LIGO science requirements document (1995), LIGO-E950018-02-E; See also, URL http://www.ligo.caltech.edu/~jzweizig/distribution/LSC_Data/
1995
Earlier work this paper cites.
S. Anderson et al., Tech. Rep. LIGO-T010095-00-Z, LIGO Project (2001), URL http://www.ligo.caltech.edu/docs/T/T010095-00.pdf
2001
Earlier work this paper cites.

Similar

L. Lindblom, B. J. Owen, and D. A. Brown, Phys. Rev. D 78
2008
Cited alongside, same era.
L. Lindblom, Phys. Rev. D 80
2009
Cited alongside, same era.
GWINC: Gravitational Wave Interferometer Noise Calculator , v1 default parameters, URL http://lhocds.ligo-wa.caltech.edu:8000/advligo/GWINC
Cited in the paper.

Then

M. A. Scheel, M. Boyle, T. Chu, L. E. Kidder, K. D. Matthews, and H. P. Pfeiffer, Phys. Rev. D 79
2009
Closest in time.
M. Boyle, D. A. Brown, and L. Pekowsky, Comparison of high-accuracy numerical simulations of black-hole binaries with stationary-phase post-Newtonian template waveforms for Initial and Advanced LIGO , arXiv:0901.1628 (2009), eprint 0901.1628
Original
2009
Closest in time.

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