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We have observed Halpha emission from a sample of 13 star-forming galaxiesfrom the WiggleZ Dark Energy Survey in the redshift range z~1.2-1.5 and stellarmass range 9.8<log(M_*/M_sun)<11.6 with the integral field spectrograph OSIRISon Keck, taking advantage of Laser Guide Star Adaptive Optics. We detectmultiple emission, 1-2 kpc size sub-components, or 'clumps' within the Halphaspatial emission in 4 galaxies, extended emission in 4 galaxies and compactspheroidal emission in 5 galaxies. Considering our results in the context ofunstable disk formation and a merger sequence, we find evidence of orderedorbital motion in the majority of galaxies as would be found in unstablegaseous disks.

Clumpology of Starbursts in the WiggleZ Dark Energy Survey