LMC N132D: A mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV

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Table 1

Spectral fit parameters for the H.E.S.S. and Fermi-LAT plus H.E.S.S. data sets.

Data	χ² /ndof	Γ		Φ₀ (1 TeV)	E_c∕E_b
			×10⁻¹⁴ TeV cm^-2 s^-1
H.E.S.S. PL	3.9/2	2.32 ± 0.22		13.1 ± 4.3	–
Fermi-LAT + H.E.S.S PL	8.2/6	2.13 ± 0.05		9.7 ± 1.6	–
Fermi-LAT + H.E.S.S ECPL	6.4/5	2.08 ± 0.06		12.3 ± 2.9	E_c = 19 TeV

Fermi-LAT + H.E.S.S BPL	4.2/4	1.47 ± 0.43	2.31 ± 0.14	12.8 ± 2.9	E_b = 24 GeV

Notes. PL stands for “power law”, ECPL for “power law with an exponential cutoff”, and “BPL” for “broken power law” (see text for details).

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