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Paper: Observing the Evolution of Disk Galaxies
Volume: 379, Cosmic Frontiers
Page: 344
Authors: Tamm, A.; Tenjes, P.
Abstract: Imaging depth and resolution, made available by adaptive optics and the HST, enable resolving galactic disks already at redshifts z ≈ 3. Rotation curves can be obtained at up to z ≈ 1, allowing for the construction of self-consistent mass distribution models. Examples of both cases are presented.
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