| What is limiting near-infrared astrometry in the Galactic Center? (2009) | |||||||||
Abstract | |||||||||
| We systematically investigate the error sources for high-precision astrometry from adaptive optics based near-infrared imaging data. We focus on the application in the crowded stellar field in the Galactic Center. We show that at the level of . Comment: accepted by MNRAS, 13 pages, 14 figures | |||||||||
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