Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/50827
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dc.contributor.author | Aharonian, F. | - |
dc.contributor.author | Akhperjanian, A. | - |
dc.contributor.author | Barres de Almaida, U. | - |
dc.contributor.author | Bazer-Bachi, A. | - |
dc.contributor.author | Behera, B. | - |
dc.contributor.author | Beilicke, M. | - |
dc.contributor.author | Benbow, W. | - |
dc.contributor.author | Bernlohr, K. | - |
dc.contributor.author | Boisson, C. | - |
dc.contributor.author | Bolz, O. | - |
dc.contributor.author | Borrel, V. | - |
dc.contributor.author | Braun, I. | - |
dc.contributor.author | Brion, E. | - |
dc.contributor.author | Brown, A. | - |
dc.contributor.author | Buhler, R. | - |
dc.contributor.author | Bulik, T. | - |
dc.contributor.author | Busching, I. | - |
dc.contributor.author | Boutelier, T. | - |
dc.contributor.author | Carrigan, S. | - |
dc.contributor.author | Chadwick, P. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2008 | - |
dc.identifier.citation | Astronomy and Astrophysics: a European journal, 2008; 484(2):435-440 | - |
dc.identifier.issn | 0004-6361 | - |
dc.identifier.issn | 1432-0746 | - |
dc.identifier.uri | http://hdl.handle.net/2440/50827 | - |
dc.description.abstract | The HESS experiment, an array of four Imaging Atmospheric Cherenkov Telescopes with high sensitivity and large field-of-view, has been used to search for emitters of very-high-energy (VHE, >100 GeV) γ-rays along the Galactic plane, covering the region 30° < l < 60°, 280° < l < 330°, and −3° < b < 3°. In this continuation of the HESS Galactic Plane Scan, a new extended VHE γ-ray source was discovered at α2000=19h12m49s, δ2000=+10◦09°06'' (HESS J1912+101). Its integral flux between 1–10 TeV is ∼10% of the Crab Nebula flux in the same energy range. The measured energy spectrum can be described by a power law dN/dE ∼ E−Γ with a photon index Γ = 2.7 ± 0.2stat ± 0.3sys. HESS J1912+101 is plausibly associated with the high spin-down luminosity pulsar PSR J1913+1011. We also discuss associations with an as yet unconfirmed SNR candidate proposed from low frequency radio observation and/or with molecular clouds found in ¹³CO data. | - |
dc.description.statementofresponsibility | F. Aharonian ... G. Rowell ... et al. | - |
dc.language.iso | en | - |
dc.publisher | EDP Sciences | - |
dc.rights | © ESO 2008. Article published by EDP Sciences | - |
dc.source.uri | http://dx.doi.org/10.1051/0004-6361:20078715 | - |
dc.subject | ISM: supernova remnants | - |
dc.subject | gamma rays: observations | - |
dc.title | Discovery of very-high-energy γ-ray emission from the vicinity of PSR J1913+1011 with HESS | - |
dc.title.alternative | Discovery of very-high-energy gamma-ray emission from the vicinity of PSR J1913+1011 with HESS | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1051/0004-6361:20078715 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Rowell, G. [0000-0002-9516-1581] | - |
Appears in Collections: | Aurora harvest Chemistry and Physics publications |
Files in This Item:
File | Description | Size | Format | |
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hdl_50827.pdf | Published version | 2.03 MB | Adobe PDF | View/Open |
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