Parsons RD, Holler M, King J, Lefranc V, Moulin E, Poon H, Veh J, Viana A (2016)
Publication Language: English
Publication Type: Conference contribution, Conference Contribution
Publication year: 2016
Publisher: Proceedings of Science (PoS)
Series: Proceedings of Science
Book Volume: 236
Pages Range: 830
Conference Proceedings Title: Proceedings of The 34th International Cosmic Ray Conference - PoS(ICRC2015)
DOI: 10.22323/1.236.0830
The Galactic Centre has been studied with the High Energy Stereoscopic System (H.E.S.S.) for over 10 years, revealing a bright, complex gamma-ray morphology. Besides a strong point-like very-high-energy gamma-ray source coincident with the supermassive black hole Sgr A∗, previous analyses also revealed a diffuse ridge of gamma-ray emission, indicative of a powerful cosmic-ray accelerator in this region. The addition of a fifth telescope with 600 m2 mirror area to the centre of the H.E.S.S. array has increased the energy range accessible, allowing observations to take place down to 100 GeV and potentially below. This wider energy range allows an important overlap in observations with satellite instruments such as the Fermi-LAT gamma-ray telescope. We will present the results of new H.E.S.S observations of the Galactic Centre region and show a detailed analysis of the central source, including comparisons to results at other wavelengths.
APA:
Parsons, R.D., Holler, M., King, J., Lefranc, V., Moulin, E., Poon, H.,... Viana, A. (2016). Sgr A∗ observations with H.E.S.S. II. In Sissa Medialab (Eds.), Proceedings of The 34th International Cosmic Ray Conference - PoS(ICRC2015) (pp. 830). The Hague, NL: Proceedings of Science (PoS).
MLA:
Parsons, Robert Daniel, et al. "Sgr A∗ observations with H.E.S.S. II." Proceedings of the 34th International Cosmic Ray Conference, ICRC 2015, The Hague Ed. Sissa Medialab, Proceedings of Science (PoS), 2016. 830.
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