File:GW170104 waveform reconstructions.svg

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Summary

Description
English: Time-domain detector data (gray), and 90% confidence intervals for waveforms reconstructed from the morphology-independent wavelet analysis (orange) and binary black hole (BBH) models from both waveform families (blue), whitened by each instrument's noise amplitude spectral density. The left ordinate axes are normalized such that the amplitude of the whitened data and the physical strain are equal at 200 Hz. The right ordinate axes are in units of noise standard deviations. The width of the BBH region is dominated by the uncertainty in the astrophysical parameters.
Date
Source https://arxiv.org/abs/1706.01812, GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2, Phys. Rev. Lett. 118, 221101
Author LIGO Scientific and Virgo Collaboration

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1 June 2017

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current20:07, 1 October 2017Thumbnail for version as of 20:07, 1 October 2017306 × 265 (1.9 MB)Geek3User created page with UploadWizard
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