Please use this identifier to cite or link to this item:
Title: Discovery of two candidate pulsar wind nebulae in very-high-energy gamma rays
Authors: Aharonian, F.
Benbow, W.
Berge, D.
Bernlöhr, K.
Bolz, O.
Braun, I.
Bühler, R.
Carrigan, S.
Costamante, L.
Domainko, W.
Egberts, K.
Beilicke, M.
Cornils, R.
Heinzelmann, G.
Holleran, M.
Raue, M.
Ripken, J.
Bernlöhr, K.
Funk, S.
Orford, K. J.
Füßling, M.
Dubus, G.
Kerschhaggl, M.
Lohse, T.
Schlenker, S.
Schwanke, U.
De Jager OC
Boisson, C.
Martin, J. M.
Sol, H.
Brion, E.
Glicenstein, J. F.
Fontaine, G.
Osborne, J. L.
Goret, P.
Moulin, E.
Rolland, L.
Brown, A. M.
Raubenheimer, B. C.
Chadwick, P. M.
Dickinson, H. J.
Hadjichristidis, C.
Latham, I. J.
Giebels, B.
Le Gallou R
McComb, T. J. L.
Rayner, S. M.
Nolan, S. J.
Spangler, D.
Ward, M.
Tam, P. H.
Büsching, I.
Venter, C.
Chounet, L. -. M.
Komin, N.
Degrange, B.
Khélifi, B.
Lemoine-Goumard, M.
Superina, G.
Tluczykont, M.
Wagner, S. J.
Coignet, G.
Boutelier, T.
Lamanna, G.
Ranchon, S.
Rosier-Lees, S.
Vialle, J. P.
Marcowith, A.
Djannati-Ataï, A.
Espigat, P.
Lemière, A.
Maurin, G.
Pita, S.
Henri, G.
Farnier, C.
Punch, M.
Terrier, R.
Aharonian, F.
Drury, L. O.
Moulin, E.
Behera, B.
Emmanoulopoulos, D.
Häuser, M.
Hinton, J. A.
Pelletier, G.
Pedaletti, G.
Pühlhofer, G.
Feinstein, F.
Schwemmer, S.
Fiasson, A.
Gallant, Y. A.
Förster, A.
Jacholkowska, A.
Vasileiadis, G.
Glück, B.
Khélifi, B.
Stegmann, C.
Petrucci, P. -. O.
Saugé, L.
Hoffmann, A.
Horns, D.
Funk, S.
Kendziorra, E.
Akhperjanian, A. G.
Santangelo, A.
Schwarzburg, S.
Martineau-Huynh, O.
De Naurois M
Kosack, K.
Tavernet, J. -. P.
Vincent, P.
Nedbal, D.
Rob, L.
Ruppel, J.
Sahakian, V.
Häuser, D.
Schlickeiser, R.
Schröder, R.
Shalchi, A.
Steenkamp, R.
Masterson, C.
Costamante, L.
Masterson, C.
Tluczykont, M.
Berge, D.
Bazer-Bachi, A. R.
Hinton, J. A.
Rowell, G.
Hermann, G.
Tluczykont, M.
Hinton, J. A.
Hofmann, W.
Panter, M.
Hoppe, S.
Rowell, G.
Van Eldik C
Noutsos, A.
Volk, H. J.
Borrel, V.
Marcowith, A.
Olive, J. -. P.
First Published: Sep-2007
Publisher: EDP Sciences for European Southern Observatory (ESO)
Citation: Astronomy & Astrophysics, 2007, 472 (2), pp. 489-495
Abstract: Context.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 HESS telescope array. Aims.Imaging Atmospheric Cherenkov Telescopes are ideal tools for searching for extended emission from pulsar wind nebulae in the very-high-energy regime. HESS, with its large field of view of 5$^{\circ}$ and high sensitivity, gives new prospects for the search for these objects. Methods.An ongoing systematic search for very-high-energy emission from energetic pulsars over the region of the Galactic plane between $-60^\circ < l < 30^\circ$, $-2^\circ < b < 2^\circ$ is performed. For the resulting candidates, the standard HESS analysis was applied and a search for multi-wavelength counterparts was performed. Results. We present the discovery of two new candidate $\gamma$-ray pulsar wind nebulae, HESS J1718-385 and HESS J1809-193. Conclusions.HESS has proven to be a suitable instrument for pulsar wind nebula searches.
DOI Link: 10.1051/0004-6361:20077280
ISSN: 0004-6361
eISSN: 1432-0746
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2007 ESO. Reproduced with permission from Astronomy & Astrophysics, © ESO.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

Files in This Item:
File Description SizeFormat 
aa7280-07.pdfPublished (publisher PDF)1.41 MBAdobe PDFView/Open

Items in LRA are protected by copyright, with all rights reserved, unless otherwise indicated.