Abstract
The serendipitous discovery of an unidentified extended TeV γ-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° 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 σ = (0.16 ± 0.02)° and the integral flux above 380 GeV is compatible with constant emission over the entire observational period of (17 ± 3)% of the Crab Nebula flux. The measured energy spectrum can be described by a power-law dN/dE ∼ E-Γ with a photon index of Γ = 2.44 ±0.05stat ± 0.2syst. Up to now, no counterpart at other wavelengths is identified. Various possible TeV production scenarios are discussed.
| Original language | English |
|---|---|
| Pages (from-to) | 1013-1021 |
| Number of pages | 9 |
| Journal | Astronomy and Astrophysics |
| Volume | 439 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - 1 Sept 2005 |
| Externally published | Yes |
Keywords
- Galaxy: disk
- Gamma rays: observations
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