Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/37555
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Type: Journal article
Title: Very high energy gamma rays from the direction of Sagittarius A*
Author: Aharonian, F.
Akhperjanian, A.
Aye, K.
Bazer-Bachi, A.
Beilicke, M.
Benbow, W.
Berge, D.
Berghaus, P.
Bernlohr, K.
Bolz, O.
Boisson, C.
Borgmeier, C.
Breitling, F.
Brown, A.
Bussons Gordo, J.
Chadwick, P.
Chitnis, V.
Chounet, L.
Cornils, R.
Costamante, L.
et al.
Citation: Astronomy and Astrophysics: a European journal, 2004; 425(1):L13-L17
Publisher: E D P Sciences
Issue Date: 2004
ISSN: 0004-6361
1432-0746
Statement of
Responsibility: 
F. Aharonian...G. Rowell...et al.
Abstract: We report the detection of a point-like source of very high energy (VHE) γ-rays coincident within 1′ of Sgr A*, obtained with the HESS array of Cherenkov telescopes. The γ-rays exhibit a power-law energy spectrum with a spectral index of -2.2 ± 0.09 × 0.15 and a flux above the 165 GeV threshold of (1.82 ± 0.22) × 10-7 m-2 s-1. The measured flux and spectrum differ substantially from recent results reported in particular by the CANGAROO collaboration.
Rights: © The European Southern Observatory 2004
DOI: 10.1051/0004-6361:200400055
Published version: http://dx.doi.org/10.1051/0004-6361:200400055
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Physics publications

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