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Uploaded on Dec 24, 2006
Original site: http://www.mpe.mpg.de/ir/GC/index.php Since 1992 we have observed the central parsec of the galactic center in near infrared wavelengths. Until 2002 we mainly used our Speckle-Camera SHARP I on the NTT located at La Silla, Chile, for K band observations; since 2002 our main instrument is the adaptive optics assisted NIR-camera NAOS/CONICA at the VLT on Cerro Paranal, Chile, performing H, K and L imaging.