Galactic center observed in the L- and H + K band with NACO and SINFONI in 2012. North is up, east is to the left. Here, the position of the DSO/G2 is marked with a dashed circle. Sgr A* is located at the position of the “x”. The Keplerian orbital fit is based on the Brγ line maps of the DSO/G2 (left image) between 2005 and 2016. The K-band continuum image is a background-subtracted high-pass filtered image with 10 000 iterations. For the convolution and deconvolution process, a Gaussian-shaped APSF is used with an FWHM of 4.7 px. The right image is a cutout of a NACO L-band mosaic observed in 2012 with a pixel scale of 27 mas px⁻¹. The total integration of the NACO image is ∼450 s, the on-source integration time of the SINFONI cube is ∼610 min.