![Figure 32](figure11.png)
Figure 32: GWR foreground produced by detached and semidetached WD binaries as it was expected
to be detected by LISA. The assumed integration time is 1 yr. The ‘noisy’ black line gives the
total power spectrum, the white line shows the average. The dashed lines show the expected LISA
sensitivity for a
of 1 and 5 [408]. Semidetached WD binaries contribute to the peak between
and
. Image reproduced with permission from [518], copyright by ESO.
![S∕N](article1241x.gif)
![log f ≃ − 3.4](article1242x.gif)
![− 3.0](article1243x.gif)