Monte-Carlo simulations of the gravitational wave signals from galactic binaries with periods of less than 1 hour. The left plot is on a log-log scale. The right hand plot has a linear scale for the signal amplitude; insets show expanded (in frequency) views of narrow-band regions near 3mHz and 6 mHz where the reduced number at higher frequencies is more evident
E. S. Phinney (Caltech)