Lindblom, Lee (2009) Optimal calibration accuracy for gravitational-wave detectors. Physical Review D, 80 (4). Art. No. 042005. ISSN 0556-2821. http://resolver.caltech.edu/CaltechAUTHORS:20091002-085200392
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Calibration errors in the response function of a gravitational-wave detector degrade its ability to detect and then to measure the properties of any detected signals. This paper derives the needed levels of calibration accuracy for each of these data-analysis tasks. The levels derived here are optimal in the sense that lower accuracy would result in missed detections and/or a loss of measurement precision, while higher accuracy would be made irrelevant by the intrinsic noise level of the detector. Calibration errors affect the data-analysis process in much the same way as errors in theoretical waveform templates. The optimal level of calibration accuracy is expressed therefore as a joint limit on modeling and calibration errors: increased accuracy in one reduces the accuracy requirement in the other.
|Additional Information:||© 2009 The American Physical Society. Received 28 June 2009; published 18 August 2009. I thank Michael Landry for stimulating my interest in the questions addressed here and for comments and suggestions for improving an earlier draft of this paper. I also thank Benjamin Owen and Yanbei Chen for several helpful discussions on these issues. This research was supported in part by a grant from the Sherman Fairchild Foundation, by NSF Grants No. DMS-0553302, No. PHY-0601459, and No. PHY-0652995, and by NASA Grant No. NNX09AF97G.|
|Classification Code:||PACS: 04.80.Nn; 04.30.-w; 06.20.fb; 07.05.Kf|
|Official Citation:||Optimal calibration accuracy for gravitational-wave detectors Lee Lindblom, Phys. Rev. D 80, 042005 (2009), DOI:10.1103/PhysRevD.80.042005|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||05 Oct 2009 17:48|
|Last Modified:||26 Dec 2012 11:26|
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