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The search for gravitational waves f λ method sources10 -16 Hz 10 9 ly Anisotropy of CBR - Primordial10 -9 Hz 10 ly Timing of ms pulsars - Primordial- Cosmic strings10 -4 - 10 -1Hz0.01 - 10AUDoppler Tracking ofspacecraftLaser interferometersin space LISA- Bynary stars- Supermassive BH (10 3 -10 7 M o )formation, coalescence, inspiral10 - 10 3 Hz 300 - 30000kmLaser interferometerson EarthLIGO, VIRGO, GEO,TAMA- Inspiral of NS and BH binaries(1-1000 M o )- Supernovae- Pulsars10 3 Hz 300 km Cryogenic resonantdetectorsALLEGRO, AURIGA,EXPLORER, NAUTILUS- NS and BH binary coalescence- Supernovae- ms pulsars