H.E.S.S. discovery of very high energy γ-ray emission from PKS 0625-354
Abstract. PKS 0625−354 (z = 0.055) was observed with the four High Energy Stereoscopic System (H.E.S.S.) telescopes in 2012 during 5.5 h. The source was detect
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| Hauptverfasser: | , , , , , , , , |
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| Körperschaft: | |
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 February 20
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 476, Heft: 3, Pages: 4187-4198 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty439 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1093/mnras/sty439 Verlag, Volltext: https://academic.oup.com/mnras/article/476/3/4187/4880460 
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| Verfasserangaben: | H.E.S.S. Collaboration, H. Abdalla, G. Cologna, W. Hofmann, F. Jankowsky, M. Mohamed, F. Rieger, S. Schwemmer, S.J. Wagner [und weitere] |
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| 520 | |a Abstract. PKS 0625−354 (z = 0.055) was observed with the four High Energy Stereoscopic System (H.E.S.S.) telescopes in 2012 during 5.5 h. The source was detect | ||
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