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We open the discussion into how the Laser Interferometer Space Antenna (LISA)observations of supermassive black-hole (SMBH) mergers (in the mass range~10^6-10^8 Msun) may be complementary to pulsar timing-based gravitational wavesearches. We consider the toy model of determining pulsar distances byexploiting the fact that LISA SMBH inspiral observations can place tightparameter constraints on the signal present in pulsar timing observations. Wealso suggest, as a future path of research, the use of LISA ring-downobservations from the most massive (>~ a few 10^7 Msun) black-hole mergers, forwhich the inspiral stage will lie outside the LISA band, as both a trigger andconstraint on searches within pulsar timing data for the inspiral stage of themerger.

Is there potential complementarity between LISA and pulsar timing?