Determining gravitational wave radiation from close galaxy pairs using a binary population synthesis approach

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Fig. 6

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Strain amplitude h as a function of the frequency for the BPS simulations of individual resolvable MBHBs. The gray scale gives the density distribution of the resolvable systems. Other lines are cited by the sensitivity studies (Sesana et al. 2008; Yardley et al. 2010) using the PTA detector.

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