Issue |
A&A
Volume 499, Number 3, June I 2009
|
|
---|---|---|
Page(s) | 723 - 728 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/200811357 | |
Published online | 29 April 2009 |
Detection of very high energy radiation from HESS J1908+063 confirms the Milagro unidentified source MGRO J1908+06
1
Max-Planck-Institut für Kernphysik, PO Box 103980, 69029 Heidelberg, Germany
2
Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
3
Yerevan Physics Institute, 2 Alikhanian Brothers St., 375036 Yerevan, Armenia
4
Universität Erlangen-Nürnberg, Physikalisches Institut, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany
5
University of Durham, Department of Physics, South Road, Durham DH1 3LE, UK
6
Centre d'Étude Spatiale des Rayonnements, CNRS/UPS, 9 av. du Colonel Roche, BP 4346, 31029 Toulouse Cedex 4, France
7
Astroparticule et Cosmologie (APC), CNRS, Université Paris 7 Denis Diderot, 10 rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France (UMR 7164, CNRS, Université Paris VII, CEA, Observatoire de Paris, France) e-mail: emma@apc.univ-paris7.fr e-mail: djannati@apc.univ-paris7.fr
8
Landessternwarte, Universität Heidelberg, Königstuhl, 69117 Heidelberg, Germany
9
Institut für Physik, Humboldt-Universität zu Berlin, Newtonstr. 15, 12489 Berlin, Germany
10
LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, 5 place Jules Janssen, 92190 Meudon, France
11
IRFU/DSM/CEA, CE Saclay, 91191 Gif-sur-Yvette, Cedex, France
12
Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland
13
Unit for Space Physics, North-West University, Potchefstroom 2520, South Africa
14
Laboratoire d'Astrophysique de Grenoble, INSU/CNRS, Université Joseph Fourier, BP 53, 38041 Grenoble Cedex 9, France
15
LPNHE, Université Pierre et Marie Curie Paris 6, Université Denis Diderot Paris 7, CNRS/IN2P3, 4 place Jussieu, 75252 Paris Cedex 5, France
16
Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/IN2P3, 91128 Palaiseau, France
17
Laboratoire d'Annecy-le-Vieux de Physique des Particules, CNRS/IN2P3, 9 chemin de Bellevue, BP 110, 74941 Annecy-le-Vieux Cedex, France
18
Instytut Fizyki Jądrowej PAN, ul. Radzikowskiego 152, 31-342 Kraków, Poland
19
Laboratoire de Physique Théorique et Astroparticules, CNRS/IN2P3, Université Montpellier II, CC 70, Place Eugène Bataillon, 34095 Montpellier Cedex 5, France
20
Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, 22761 Hamburg, Germany
21
School of Physics & Astronomy, University of Leeds, Leeds LS2 9JT, UK
22
Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, 72076 Tübingen, Germany
23
Toruń Centre for Astronomy, Nicolaus Copernicus University, ul. Gagarina 11, 87-100 Toruń, Poland
24
Institute of Particle and Nuclear Physics, Charles University, V Holesovickach 2, 18000 Prague 8, Czech Republic
25
European Associated Laboratory for Gamma-Ray Astronomy, jointly supported by CNRS and MPG
26
Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul. Orla 171, 30-244 Kraków, Poland
27
Stanford University, HEPL & KIPAC, Stanford, CA 94305-4085, USA
28
School of Chemistry & Physics, University of Adelaide, Adelaide 5005, Australia
29
Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum, 44780 Bochum, Germany
30
University of Namibia, Private Bag 13301, Windhoek, Namibia
Received:
16
November
2008
Accepted:
16
April
2009
Aims. Detection of a γ-ray source above 300 GeV is reported, confirming the unidentified source MGRO J1908+06, discovered by the Milagro collaboration at a median energy of 20 TeV.
Methods. The source was observed during 27 h as part of the extension of the HESS Galactic plane survey to longitudes >30°.
Results. HESS J1908+063 is detected at a significance level of 10.9σ with an integral flux above 1 TeV of (3.76 ± ± )10-12 ph cm-2 s-1, and a spectral photon index Γ = 2.10±± 0.2. The positions and fluxes of HESS J1908+063 and MGRO J1908+06 are in good agreement. Possible counterparts at other wavelengths and the origin of the γ-ray emission are discussed. The nearby unidentified GeV source, GRO J1908+0556 (GeV) which also remains unidentified and the new Fermi pulsar 0FGL J1907.5+0617, may be connected to the TeV source.
Key words: gamma rays: observations
© ESO, 2009
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