VERITAS detection of LS 5039 and HESS J1825-137
Lang, Mark J. ; Moriarty, Patrick
Lang, Mark J.
Moriarty, Patrick
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Repository DOI
Publication Date
2019-11-07
Type
Article
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Citation
Abeysekara, A.U., Benbow, W., Bird, R., Brose, R., Christiansen, J.L., Chromey, A.J., Cui, W., Daniel, M.K., Falcone, A., Fortson, L., Hanna, D., Hassan, T., Hervet, O., Holder, J., Hughes, G., Humensky, T.B., Kaaret, P., Kar, P., Kelley-Hoskins, N., Kertzman, M., Kieda, D., Krause, M., Lang, M.J., Maier, G., Moriarty, P., Nieto, D., Nievas-Rosillo, M., Ong, R.A., Pandel, D., Pohl, M., Prado, R.R., Pueschel, E., Quinn, J., Ragan, K., Reynolds, P.T., Richards, G.T., Roache, E., Sadeh, I., Santander, M., Sembroski, G.H., Weinstein, A., Wilcox, P., Williams, D.A., Williamson, T.J. (2020) 'VERITAS Detection of LS 5039 and HESS J1825-137'. Astroparticle Physics, 117, 102403. doi: https://doi.org/10.1016/j.astropartphys.2019.102403
Abstract
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 8.8σ. The measured flux above 1 TeV is near inferior conjunction and near superior conjunction. The pulsar wind nebula HESS J1825-137 is detected with a statistical significance of 6.7σ and a measured flux above 1 TeV of .
Publisher
Elsevier
Publisher DOI
10.1016/j.astropartphys.2019.102403
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Attribution-NonCommercial-NoDerivs 3.0 Ireland