Chandra (2022-2023) 3–8 keV image (log scale) overlaid with the inferred polarization directions (solid arrows) and with corresponding uncertainties (dashed arrows) converted into either a direction toward the primary source in the reflection case (large Sgr A complex and its brightest part in white) or into the magnetic field direction in the synchrotron scenario for the nonthermal emission from G0.13-0.11 (in cyan). The polarization directions, rotated by 180 deg, are identical to the ones shown for the polarization signal, and the signal orientation was chosen to highlight the consistency with the directions toward Sgr A*, the Arches cluster, or the “wings” of the PWN G0.13-0.11.