Detections by LISA of circumbinary exoplanets (red) and BDs (blue) in the optimistic (B1) scenario for 4 yr (left panel) and 8 yr (right panel) of observations. The SSOs mass (M, or M sin(i) for those planet whose inclination is not known yet), as a function of the SSO-to-binary separation (a) is shown, together with values of known exoplanets (data were taken from https://exoplanetarchive.ipac.caltech.edu). The horizontal dotted line corresponds to the limits in mass we explored: 13 and 0.08 M_J.