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most citedThe rapid formation a large rotating disk galaxy three billion years after the Big Bang

478 citations · 4k across the 47 of their papers we have counts for

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astro-ph2006★ 478 cited

The rapid formation a large rotating disk galaxy three billion years after the Big Bang

R. Genzel, L. Tacconi, F. Eisenhauer +16

[Abridged] Over the past two decades observations and theoretical simulations have established a global frame-work of galaxy formation and evolution in the young Universe. Galaxies…

astro-ph2006★ 13 cited

Galaxy morphology and evolution from SWAN Adaptive Optics imaging

G. Cresci, R. I. Davies, A. J. Baker +4

We present the results from adaptive optics (AO) assisted imaging in the Ks band of an area of 15 arcmin^2 for SWAN (Survey of a Wide Area with NACO). We derive the high resolution…

astro-ph2006★ 135 cited

Dynamical properties of Ultraluminous Infrared Galaxies. II. Traces of dynamical evolution and end products of local ultraluminous mergers

K. M. Dasyra, L. J. Tacconi, R. I. Davies +8

We present results from our Very Large Telescope large program to study the dynamical evolution of local Ultraluminous Infrared Galaxies (ULIRGs) and QSOs. This paper is the second…

astro-ph2006★ 39 cited

Lyman Break Galaxies Under a Microscope: The Small Scale Dynamics and Mass of an Arc in the Cluster 1E0657-56

N. P. H. Nesvadba, M. D. Lehnert, F. Eisenhauer +8

Using the near-infrared integral-field spectrograph SPIFFI on the VLT, we have studied the spatially-resolved dynamics in the z=3.2 strongly lensed galaxy 1E0657-56 ``arc+core''. T…

astro-ph2006★ 215 cited

The Star-Forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC3227

R. Davies, J. Thomas, R. Genzel +7

We report R~4300 VLT SINFONI adaptive optics integral field K-band spectroscopy of the nucleus of the Seyfert 1 galaxy NGC3227 at a spatial resolution of 0.085" (7pc). We present t…

astro-ph2006

SINFONI's take on Star Formation, Molecular Gas, and Black Hole Masses in AGN

R. Davies, R. Genzel, L. Tacconi +3

We present some preliminary (half-way) results on our adaptive optics spectroscopic survey of AGN at spatial scales down to 0.085arcsec. Most of the data were obtained with SINFONI…