Physics
Scientist
University of Cologne, Germany
A two component hot spot/ring model for the NIR flares of Sagittarius A*
Interferometric observations of the galactic center: LBT and VLTI
Prospects for observing the Galactic Center: combining LBT LINC-NIRVANA observations in the near-infrared with observations in the mm/sub-mm wavelength domain
The orbiting spot model gives constraints on the parameters of the supermassive black hole in the Galactic Center
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