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- Discovery of two candidate pulsar wind nebulae in very-high-energy gamma rays doi link

Auteur(s): Aharonian F., R. Bazer-Bachi A., Boisson C., Borrel V., Boutelier T., M. Chounet L., Coignet G., Degrange B., Djannati-Ataï A., Dubus G., Espigat P., Farnier C., Feinstein F., Fiasson A., Fontaine G., Gallant Y., Giebels B., F. Glicenstein J., Goret P., Henri G., Jacholkowska Agnieszka, Khelifi B., Komin Nukri, Lamanna G., Lemiere A., Lemoine-Goumard M., M. Martin J., Marcowith A., Moulin Emmanuel, Vasileiadis G.

(Article) Publié: Astronomy & Astrophysics, vol. 472 p.489-495 (2007)
Texte intégral en Openaccess : arxiv


Ref HAL: in2p3-00148471_v1
Ref Arxiv: 0705.1605
DOI: 10.1051/0004-6361:20077280
Ref. & Cit.: NASA ADS
Exporter : BibTex | endNote
54 citations
Résumé:

We present the discovery of two very-high-energy gamma-ray sources in an ongoing systematic search for emission above 100 GeV from pulsar wind nebulae in survey data from the H.E.S.S. telescope array. Imaging Atmospheric Cherenkov Telescopes are ideal tools for searching for extended emission from pulsar wind nebulae in the very-high-energy regime. H.E.S.S., with its large field of view of 5 degrees and high sensitivity, gives new prospects for the search for these objects. An ongoing systematic search for very-high-energy emission from energetic pulsars over the region of the Galactic plane between -60 degrees < l < 30 degrees, -2 degrees < b < 2 degrees is performed. For the resulting candidates, the standard H.E.S.S. analysis was applied and a search for multi-wavelength counterparts was performed. We present the discovery of two new candidate gamma-ray pulsar wind nebulae, HESS J1718-385 and HESS J1809-193. H.E.S.S. has proven to be a suitable instrument for pulsar wind nebula searches.