Unidentified γ-ray emission towards the SNR Kes 41 revisited

L. Supan; G. Castelletti; A. D. Supanitsky; M. G. Burton

doi:10.1051/0004-6361/201834075

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Volume 619 (November 2018)

A&A, 619 (2018) A109

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Table 1

Fluxes in the GeV range for the γ-ray source detected in correspondence with SNR Kes 41.

E_c	Energy range	Flux (E²dN∕dE)	TS
(GeV)	(GeV)	(10⁻¹² erg cm⁻² s⁻¹)
0.5	0.30−0.84	13.8 ± 2.3 ± 4.4	133
1.4	0.84−2.34	11.5 ± 1.1 ± 2.8	163
3.9	2.34−6.55	8.4 ± 0.8 ± 2.1	150
10.9	6.55−18.3	2.9 ± 0.7 ± 1.3	28
30.6	18.3−51.2	≤0.9^a	8
85.6	51.2−143	≤1.6^a	3

Notes. For each flux, the first quoted error corresponds to the statistic uncertainty, while the second error depicts the systematic uncertainty. ^(a) Values corresponding to 95% confidence level upper limits.

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