Extended Data Fig. 1: One-dimensional projections of VHE events.
From: Resolving acceleration to very high energies along the jet of Centaurus A
Shown are projections of the VHE γ-ray emission from Centaurus A along the alignment of the semi-major axis obtained from the two-dimensional elliptical morphology fit (left; negative values correspond to φ = 43.4° and positive ones to φ + 180°) and perpendicular to it (right; φ + 90° for negative and φ + 270° for positive distances). The dashed red line shows the projection of the PSF on both sides. The blue line on the left panel corresponds to the PSF-convolved best-fit Gaussian model. Error bars on the ordinate denote statistical uncertainties (±1 s.d.), those along the abscissa illustrate the bin size.
