This is the dream of multi-messenger astronomy:
Simulations show that next generation gravitational wave detectors will be able to detect the initial part of the wave before the actual merger of objects (or collision?). If you can identify this signal in time, you could make the 'regular' telescopes look into that particular direction and look for a signal in light, and you could use a neutrino detector at the same time (think IceCube, KM3NeT, Baikal and others that look at large parts of the sky) to look in the neutrino channel.
This way you would have gravitational wave-, light- and neutrino-channels from a single object. This is still many years (decades?) away, but would be incredible for studying exotic objects.
If you mean, measuring the neutrino baseline difference when a GW passes through the Earth, perhaps. I never thought about it, but its definitely intriguing.