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VERITAS Detection of LS 5039 and HESS J1825-137
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VERITAS Detection of LS 5039 and HESS J1825-137

A. U Abeysekara, W Benbow, R Bird, R Brose, J. L Christiansen, A. J Chromey, W Cui, M. K Daniel, A Falcone, L Fortson, …
pp 102403-(2020). doi:10.1016/j.astropartphys.2019.102403
2020

Abstract

flux gamma ray: binary gamma ray: VHE HESS inverse scattering method pulsar star statistical VERITAS
With 8 h of observations, VERITAS confirms the detection of two very high energy gamma-ray sources. The gamma-ray binary LS 5039 is detected with a statistical significance of 8.8 σ . The measured flux above 1 TeV is (2.5±0.4)×10−12cm−2s−1 near inferior conjunction and (7.8±2.8)×10−13cm−2s−1 near superior conjunction. The pulsar wind nebula HESS J1825-137 is detected with a statistical significance of 6.7 σ and a measured flux above 1 TeV of (3.9±0.8)×10−12cm−2s−1 .

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