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Table 2.

Results of the energy cutoff analysis for 25 unidentified γ-ray sources in the HGPS catalog.

Source Ecut,  γ (TeV) Sγ Ecut,  h (TeV) Emax (TeV) Γ N p-value T (h)
HESS J1800−240 34.7 0.0 510.1 12 2.44 ± 0.03 5 9.6e−01 10
HESS J1641−463 21.3 0.1 184.9 13 2.38 ± 0.03 5 9.8e−01 27
HESS J1908+063 31.1 1.0 154.0 30 2.22 ± 0.04 6 8.2e−01 12
HESS J1852−000 29.2 0.0 119.7 30 2.12 ± 0.06 6 8.0e−01 23
HESS J1634−472 20.3 0.5 107.8 30 2.30 ± 0.05 6 2.8e−01 14
HESS J1828−099 14.5 0.0 64.6 12 2.19 ± 0.07 5 8.3e−01 20
HESS J1023−575 13.5 2.0 35.3 32 2.38 ± 0.07 6 2.1e−01 23
HESS J1858+020 10.6 0.3 33.5 13 2.30 ± 0.04 5 9.5e−01 22
HESS J1841−055 8.4 2.7 29.9 12 2.42 ± 0.07 5 9.8e−03 14
HESS J1503−582 8.3 0.0 28.4 14 2.7 ± 0.1 5 3.4e−01 18
HESS J1507−622 10.6 2.4 26.3 15 2.10 ± 0.07 5 4.5e−01 13
HESS J1646−458 7.4 0.0 22.7 13 2.6 ± 0.1 5 7.1e−01 10
HESS J1457−593 7.7 0.0 18.1 15 2.6 ± 0.1 5 7.3e−01 4
HESS J1843−033 9.9 2.8 16.6 30 2.2 ± 0.1 6 1.7e−03 17
HESS J1018−589 B 8.6 2.3 14.7 15 2.1 ± 0.1 5 6.3e−01 21
HESS J1632−478 5.3 0.1 10.0 13 2.46 ± 0.06 5 4.0e−01 15
HESS J1741−302 4.5 0.0 9.2 7 2.2 ± 0.2 6 5.3e−01 145
HESS J1702−420 5.2 0.2 9.1 13 2.1 ± 0.1 5 1.7e−01 4
HESS J1809−193 3.4 1.0 5.0 12 2.3 ± 0.1 5 1.6e−01 10
HESS J1616−508 3.2 1.1 3.8 13 2.3 ± 0.1 5 1.1e−02 4
HESS J1808−204 2.1 0.0 2.7 12 2.1 ± 0.2 5 1.3e−01 37
HESS J1026−582 5.0 2.0 2.3 32 2.0 ± 0.2 5 7.0e−03 22
HESS J1804−216 1.3 1.1 1.8 12 2.7 ± 0.1 5 2.6e−04 19
HESS J1708−443 2.2 1.2 1.3 13 2.0 ± 0.2 5 4.2e−02 8
HESS J1746−285 1.2 0.6 0.7 6 2.0 ± 0.2 7 4.0e−01 259

Notes. The source name refers to the HGPS (Abdalla et al. 2018). Ecut,  γ is the lower limit on the exponential energy cutoff of the γ-ray spectrum (Eq. (3) with β = 1). Sγ is the significance of an F-test for a power-law model against an exponential cutoff in the γ-ray spectrum (again modeled by Eq. (3) with β = 1). Ecut,  h is the upper limit on the energy cutoff of a hadron population in a purely hadronic model (Eq. (1)). Emax is the maximum bin-center energy of the spectral points for the source used in the analysis. Γ is the power-law index of the best least-square fit to the public HGPS data. Errors are statistical only. N is the number of spectral points for the source used in the analysis. The p-values refer to a χ2 goodness-of-fit test for the power-law model. The HESS livetime used for the spectral analysis of the source in the HGPS is indicated by T. All upper limits are at 90% CL. The results are in descending order in Ecut,  h.

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