377 citations · 2.8k across the 40 of their papers we have counts for
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Very high contrast IFU spectroscopy of AB Doradus C: 9 mag contrast at 0.2" without a coronagraph using spectral deconvolution
Niranjan Thatte, Roberto Abuter, Matthias Tecza +3
We present an extension of the spectral deconvolution method (Sparks & Ford 2002) to achieve very high contrast at small inner working radii. We apply the method to the specific ca…
New Photometry and Spectra of AB Doradus C: An Accurate Mass Determination of a Young Low-Mass Object with Theoretical Evolutionary Tracks
Laird M. Close, Niranjan Thatte, Eric L. Nielsen +3
We present new photometric and spectroscopic measurements for the unique, young, low-mass evolutionary track calibrator AB Dor C. While the new Ks photometry is similar to that pre…
Extreme gas kinematics in the z=2.2 powerful radio galaxy MRC1138-262: Evidence for efficient AGN feedback in the early Universe?
N. P. H. Nesvadba, M. D. Lehnert, F. Eisenhauer +3
To explain the properties of the most massive low-redshift galaxies and the shape of their mass function, recent models of galaxy evolution include strong AGN feedback to complemen…
SPIFFI observations of the starburst SMMJ14011+0252: Already old, fat, and rich by z = 2.565
M. Tecza, A. J. Baker, R. I. Davies +10
Using the SPectrometer for Infrared Faint Field Imaging (SPIFFI) on the ESO VLT, we have obtained J, H, and K band integral field spectroscopy of the z = 2.565 luminous submillimet…
Submillimeter Galaxies as Tracers of Mass Assembly at Large M
R. Genzel, A. J. Baker, R. J. Ivison +19
Luminous submillimeter galaxies (SMGs) have been known for some time to produce a substantial fraction of the far-IR/submillimeter background. New observations show that these syst…
A Geometric Determination of the Distance to the Galactic Center
F. Eisenhauer, R. Schoedel, R. Genzel +5
We report new astrometric and spectroscopic observations of the star S2 orbiting the massive black hole in the Galactic Center, which were taken at the ESO VLT with the adaptive op…