David Wilman
Universitäts-Sternwarte München
92 papers found
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The Evolution and Origin of Ionized Gas Velocity Dispersion fromz∼ 2.6 toz∼ 0.6 with KMOS3D
UploadThe KMOS3D Survey: Demographics and Properties of Galactic Outflows at z = 0.6–2.7
UploadThe KMOS Cluster Survey (KCS). III. Fundamental Plane of Cluster Galaxies atz≃ 1.80 in JKCS 041
UploadThe Evolution of the Tully–Fisher Relation betweenz∼ 2.3 andz∼ 0.9 with KMOS3D
UploadKMOS3DReveals Low-level Star Formation Activity in Massive Quiescent Galaxies at 0.7
UploadGalaxy Environment in the 3D-HSTFields: Witnessing the Onset of Satellite Quenching atz∼ 1–2
UploadKmos3d: Dynamical Constraints on the Mass Budget in Early Star-Forming Disks
UploadGalaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ̃ 1-2
UploadThe KMOS GTO Cluster Program: Absorption Line Spectroscopy of Cluster Galaxies at z\tilde1.5
UploadThe Angular Momentum Distribution and Baryon Content of Star-forming Galaxies at z \tilde 1-3
UploadThe ANGULAR MOMENTUM DISTRIBUTION AND BARYON CONTENT OF STAR-FORMING GALAXIES ATz∼ 1–3
UploadThe Evolution of Metallicity and Metallicity Gradients from z = 2.7 to 0.6 with KMOS$^3D$
UploadEvidence for a change in the dominant satellite galaxy quenching mechanism at z = 1
UploadNon-linearity and environmental dependence of the star-forming galaxies main sequence
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