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We present the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY)Pilot Phase I HI kinematic models. This first data release consists of HIobservations of three fields in the direction of the Hydra and Norma clusters,and the NGC 4636 galaxy group. In this paper, we describe how we generate andpublicly release flat-disk tilted-ring kinematic models for 109/592 unique HIdetections in these fields. The modelling method adopted here - which we callthe WALLABY Kinematic Analysis Proto-Pipeline (WKAPP) and for which thecorresponding scripts are also publicly available - consists of combiningresults from the homogeneous application of the FAT and 3DBAROLO algorithms tothe subset of 209 detections with sufficient resolution and S/N in order togenerate optimized model parameters and uncertainties. The 109 models presentedhere tend to be gas rich detections resolved by at least 3-4 synthesized beamsacross their major axes, but there is no obvious environmental bias in themodelling. The data release described here is the first step towards thederivation of similar products for thousands of spatially-resolved WALLABYdetections via a dedicated kinematic pipeline. Such a large publicly availableand homogeneously analyzed dataset will be a powerful legacy product that thatwill enable a wide range of scientific studies.

WALLABY Pilot Survey: Public release of HI kinematic models for more than 100 galaxies from phase 1 of ASKAP pilot observations