Multiwavelength finding chart of the inner ≈0.8 pc of the Galactic center. For this representation of the fraction of the inner parsec, we used ALMA continuum data observed at (9.99 ± 1.58)×10¹⁰ Hz, which are represented as green in the plot. The red background image and blue emission was observed with NACO in the K- and L-band, respectively. We overlay the plot with the Doppler-shifted Brγ emission line observed at 2.1648 μm using ERIS (magenta) and a related width of ±330 km/s. The contour lines represent 9%, 13%, 26%, 30%, 43%, and 65% of the peak emission of IRS 13 of about 0.9 × 10⁻⁶W/cm² (Maillard et al. 2004).