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Table 2.

Best-fit parameter values for the H.E.S.S. 2-component model.

Par. [unit] Value
Component A (PL spectral model)

RA [deg] 272.551 ± 0.025stat ± 0.018sys
()
Dec. [deg] −19.344 ± 0.023stat ± 0.013sys
σ [deg] 0.622 ± 0.032stat ± 0.020sys(a)
e 0.824 ± 0.025stat
ϕ [deg] 50.0 ± 3.1stat
N0 [10−12 TeV−1 cm−2 s−1] 8.42 ± 0.40stat ± 1.14sys
Γ 2.239 ± 0.027stat ± 0.020sys
E0 [TeV] 1 (fixed)

Component A (ECPL spectral model)

RA [deg] 272.554 ± 0.025stat ± 0.019sys
()
Dec. [deg] −19.344 ± 0.021stat ± 0.012sys
σ [deg] 0.613 ± 0.031stat ± 0.015sys(a)
e 0.820 ± 0.025stat
ϕ [deg] 51.3 ± 3.1stat
N0 [10−12 TeV−1 cm−2 s−1] 9.05 ± 0.47stat ± 0.91sys
Γ 1.90 ± 0.05stat ± 0.05sys
Ec [TeV]
E0 [TeV] 1 (fixed)

Component B

RA [deg] 272.400 ± 0.010stat
()
Dec. [deg] −19.406 ± 0.009stat
σ [deg] 0.0953 ± 0.0072stat ± 0.0034sys
N0 [10−12 TeV−1 cm−2 s−1] 0.95 ± 0.11stat ± 0.011sys
Γ 1.98 ± 0.05stat ± 0.03sys
E0 [TeV] 1 (fixed)

Notes. For component A, we provide the best-fit values for the assumption of a PL spectral model and an ECPL spectral model. σ, e, and ϕ denote the 1-σ radius, eccentricity, and position angle of the Gaussian spatial model, respectively. N0, Γ, E0, and Ec are parameters of the spectral models, as defined in Eqs. (1) and (2). Systematic uncertainties have been derived as described in Appendix B.

(a)

For the asymmetric component A, σ refers to the semi-major axis. The extents of the semi-minor axis compute to 0.353 ± 0.029stat and 0.351 ± 0.028stat for the PL and ECPL spectral model, respectively.

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