Marin, FelipeBlake, ChrisPoole, Gregory BMcBride, Cameron KBrough, SarahColless, MatthewContreras, CarlosCouch, WarrickCroton, DarrenCroom, SSharp, RobertForster, KarlGilbank, DavidMadore, BarryWyder, Ted2015-12-130035-8711http://hdl.handle.net/1885/74571Higher order statistics are a useful and complementary tool for measuring the clustering of galaxies, containing information on the non-Gaussian evolution and morphology of large-scale structure in the Universe. In this work we present measurements of theAuthor/s retain copyrightKeywords: Methods; Observations - large-scale structure of - Universe; Statistical - cosmological parameters - cosmologyThe WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with three-point correlation functions201310.1093/mnras/stt5202016-02-24