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Serendipitous discovery of the unidentified extended TeV gamma-ray source HESS J1303-631

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posted on 2012-10-24, 08:53 authored by F. Aharonian, A. G. Akhperjanian, K. M. Aye, A. R. Bazer-Bachi, M. Beilicke, W. Benbow, D. Berge, P. Berghaus, K. Bernlohr, C. Boisson, O. Bolz, I. Braun, F. Breitling, A. M. Brown, J. B. Gordo, P. M. Chadwick, L. M. Chounet, R. Cornils, L. Costamante, B. Degrange, A. Djannati-Atai, L. O. Drury, G. Dubus, D. Emmanoulopoulos, P. Espigat, F. Feinstein, P. Fleury, G. Fontaine, Y. Fuchs, S. Funk, Y. A. Gallant, B. Giebels, S. Gillessen, J. F. Glicenstein, P. Goret, C. Hadjichristidis, M. Hauser, G. Heinzelmann, G. Henri, G. Hermann, JA. Hinton, W. Hofmann, M. Holleran, D. Horns, de Jager O. C., B. Khelifi, N. Komin, A. Konopelko, IJ. Latham, Le Gellou R., A. Lemiere, M. Lemoine-Goumard, N. Leroy, T. Lohse, O. Martineau-Huynh, A. Marcowith, C. Masterson, T. J. L. McComb, de Naurois M., S. J. Nolan, A. Noutsos, K. J. Orford, J. L. Osborne, M. Ouchrif, M. Panter, G. Pelletier, S. Pita, G. Puhlhofer, M. Punch, B. C. Raubenheimer, M. Raue, J. Raux, S. M. Rayner, I. Redondo, A. Reimer, O. Reimer, J. Ripken, L. Rob, L. Rolland, G. Rowell, V. Sahakian, L. Sauge, S. Schlenker, R. Schlickeiser, C. Schuster, U. Schwanke, M. Siewert, H. Sol, R. Steenkamp, C. Stegmann, J. P. Tavernet, R. Terrier, C. G. Theoret, M. Tluczykont, van der Walt D. J., G. Vasileiadis, C. Venter, P. Vincent, H. J. Volk, S. J. Wagner
The serendipitous discovery of an unidentified extended TeV $\gamma$-ray source close to the galactic plane named HESS J1303-631 at a significance of 21 standard deviations is reported. The observations were performed between February and June 2004 with the HESS stereoscopic system of Cherenkov telescopes in Namibia. HESS J1303-631 was discovered roughly $0.6\degr$ north of the binary system PSR B1259-63 / SS 2883 , the target object of the initial observation campaign which was also detected at TeV energies in the same field of view. HESS J1303-631 is extended with a width of an assumed intrinsic Gaussian emission profile of $\sigma = (0.16 \pm 0.02)\degr$ and the integral flux above $380\,\mathrm{GeV}$ is compatible with constant emission over the entire observational period of $(17 \pm 3)$% of the Crab Nebula flux. The measured energy spectrum can be described by a power-law $\mathrm{d}N/\mathrm{d}E \sim E^{-\Gamma}$ with a photon index of $\Gamma = 2.44 \pm 0.05_{\mathrm{stat}} \pm 0.2_{\mathrm{syst}}$. Up to now, no counterpart at other wavelengths is identified. Various possible TeV production scenarios are discussed.

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Citation

ASTRONOMY & ASTROPHYSICS, 2005, 439 (3), pp. 1013-1021

Version

  • VoR (Version of Record)

Published in

ASTRONOMY & ASTROPHYSICS

Publisher

EDP Sciences for European Southern Observatory (ESO)

issn

0004-6361

Copyright date

2005

Available date

2012-10-24

Publisher version

http://www.aanda.org/articles/aa/abs/2005/33/aa3195-05/aa3195-05.html

Language

en

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