The Evolution and Origin of Ionized Gas Velocity Dispersion from z ∼ 2.6 to z ∼ 0.6 with KMOS<sup>3D</sup> <sup>∗</sup>Hannah Übler, Stijn Wuyts, R. P. Saglia et al.|The Astrophysical Journal|2019Cited by 169
The KMOS<sup>3D</sup> Survey: Data Release and Final Survey Paper*Emily Wisnioski, Eva Wuyts, R. P. Saglia et al.|The Astrophysical Journal|2019Cited by 146
Kiloparsec Scale Properties of Star Formation Driven Outflows at z ∼ 2.3 in the SINS/zC-SINF AO Survey*R. L. Davies, Stijn Wuyts, Erica J. Nelson et al.|The Astrophysical Journal|2019Cited by 109
Rotation Curves in z ∼ 1–2 Star-forming Disks: Evidence for Cored Dark Matter DistributionsR. Genzel, Stijn Wuyts, R. P. Saglia et al.|The Astrophysical Journal|2020Cited by 104
The multiphase gas structure and kinematics in the circumnuclear region of NGC 5728Thomas Shimizu, Sylvain Veilleux, Mengxiang Lin et al.|Monthly Notices of the Royal Astronomical Society|2019Cited by 98