An extreme particle accelerator in the Galactic plane: HESS J1826−130

Open Access

Table 3

Comparison of ECPL spectral models for the HESS J1826−130 integration region (Total), plus the north and south semi-circle regions.

Region	Normalization	Index	Cut-off energy	Integral flux (>1 TeV)
	(10⁻¹³ cm⁻² s⁻¹ TeV⁻¹)		(TeV)	(% Crab Nebula)
Total	10.10 ± 0.69_stat ± 2.02_sys	1.78 ± 0.10_stat ± 0.20_sys	15.2	4.9
North semi-circle	4.64 ± 0.49_stat ± 0.93_sys	1.69 ± 0.14_stat ± 0.20_sys	15.8	2.4
South semi-circle	5.06 ± 0.49_stat ± 1.01_sys	1.88 ± 0.14_stat ± 0.20_sys	16.4	2.3

Notes. The integral flux (in % Crab Nebula) is given for the same energy range (above 1 TeV).

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