Noise residuals for GW150914 using maximum likelihood and numerical relativity templates

13 May 2019 Jackson Andrew D. Liu Hao Naselsky Pavel

We reexamine the results presented in a recent work by Nielsen et al. [1], in which the properties of the noise residuals in the 40\,ms chirp domain of GW150914 were investigated. This paper confirmed the presence of strong (i.e., about 0.80) correlations between residual noise in the Hanford and Livingston detectors in the chirp domain as previously seen by us [2] when using a numerical relativity template given in [3]... (read more)

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  • INSTRUMENTATION AND METHODS FOR ASTROPHYSICS
  • HIGH ENERGY ASTROPHYSICAL PHENOMENA