%0 Journal Article
%T PSR J1907+0602: A Radio-Faint Gamma-Ray Pulsar Powering a Bright TeV Pulsar Wind Nebula
%+ Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112))
%+ Laboratoire Leprince-Ringuet (LLR)
%+ Laboratoire de physique et chimie de l'environnement (LPCE)
%+ Unité Scientifique de la Station de Nançay (USN)
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%+ Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG)
%+ Centre d'étude spatiale des rayonnements (CESR)
%A A. Abdo, A.
%A Ackermann, Markus
%A Ajello, Marco
%A Baldini, Luca
%A Ballet, Jean
%A Barbiellini, Guido
%A Bastieri, D.
%A M. Baughman, B.
%A Bechtol, K.
%A Bellazzini, R.
%A Berenji, B.
%A D. Blandford, R.
%A D. Bloom, E.
%A Bonamente, E.
%A W. Borgland, A.
%A Bregeon, J.
%A Brez, A.
%A Brigida, M.
%A Bruel, Pascal
%A H. Burnett, T.
%A Buson, S.
%A A. Caliandro, G.
%A A. Cameron, R.
%A Camilo, F.
%A Caraveo, P. A.
%A M. Casandjian, J.
%A Cecchi, C.
%A Çelik, Ö.
%A Chekhtman, A.
%A C. Cheung, C.
%A Chiang, J.
%A Ciprini, S.
%A Claus, R.
%A Cognard, Ismaël
%A Cohen-Tanugi, J.
%A R. Cominsky, L.
%A Conrad, J.
%A Cutini, S.
%A de Angelis, A.
%A de Palma, F.
%A W. Digel, S.
%A L. Dingus, B.
%A Dormody, M.
%A Do Couto E Silva, E.
%A S. Drell, P.
%A Dubois, R.
%A Dumora, D.
%A Farnier, C.
%A Favuzzi, C.
%A J. Fegan, S.
%A B. Focke, W.
%A Fortin, P.
%A Frailis, M.
%A C. C. Freire, P.
%A Fukazawa, Y.
%A Funk, S.
%A Fusco, P.
%A Gargano, F.
%A Gasparrini, D.
%A Gehrels, N.
%A Germani, S.
%A Giavitto, G.
%A Giebels, B.
%A Giglietto, N.
%A Giordano, F.
%A Glanzman, T.
%A Godfrey, G.
%A A. Grenier, I.
%A Grondin, M.-H.
%A E. Grove, J.
%A Guillemot, L.
%A Guiriec, S.
%A Hanabata, Y.
%A K. Harding, A.
%A Hays, E.
%A E. Hughes, R.
%A S. Jackson, M.
%A Jóhannesson, G.
%A S. Johnson, A.
%A J. Johnson, T.
%A N. Johnson, W.
%A Johnston, S.
%A Kamae, T.
%A Katagiri, H.
%A Kataoka, J.
%A Kawai, N.
%A Kerr, M.
%A Knödlseder, Jürgen
%A L. Kocian, M.
%A Kuss, M.
%A Lande, J.
%A Latronico, L.
%A Lemoine-Goumard, M.
%A Longo, F.
%A Loparco, F.
%A Lott, B.
%A N. Lovellette, M.
%A Lubrano, P.
%A Makeev, A.
%A Marelli, M.
%A N. Mazziotta, M.
%A E. Mcenery, J.
%A Meurer, C.
%A F. Michelson, P.
%A Mitthumsiri, W.
%A Mizuno, T.
%A A. Moiseev, A.
%A Monte, C.
%A E. Monzani, M.
%A Morselli, A.
%A V. Moskalenko, I.
%A Murgia, S.
%A L. Nolan, P.
%A P. Norris, J.
%A Nuss, E.
%A Ohsugi, T.
%A Omodei, N.
%A Orlando, E.
%A F. Ormes, J.
%A Paneque, D.
%A Parent, D.
%A Pelassa, V.
%A Pepe, M.
%A Pesce-Rollins, M.
%A Piron, F.
%A Porter, T.A.
%A Rainò, S.
%A Rando, R.
%A S. Ray, P.
%A Razzano, M.
%A Reimer, A.
%A Reimer, O.
%A Reposeur, T.
%A Ritz, S.
%A S. E. Roberts, M.
%A S. Rochester, L.
%A Y. Rodriguez, A.
%A W. Ro'Mani, R.
%A Roth, M.
%A Ryde, F.
%A F.-W. Sadrozinski, H.
%A Sanchez, D.
%A Sander, A.
%A M. Saz Parkinson, P.
%A D. Scargle, J.
%A Sgrò, C.
%A J. Siskind, E.
%A Smith, David Stanley
%A D. Smith, P.
%A Spandre, G.
%A Spinelli, P.
%A S. Strickman, M.
%A J. Suson, D.
%A Tajima, H.
%A Takahashi, H.
%A Tanaka, T.
%A B. Thayer, J.
%A G. Thayer, J.
%A Theureau, G.
%A J. Thompson, D.
%A Tibaldo, L.
%A Tibolla, O.
%A F. Torres, D.
%A Tosti, G.
%A Tramacere, A.
%A Uchiyama, Y.
%A L. Usher, T.
%A van Etten, A.
%A Vasileiou, V.
%A Venter, C.
%A Vilchez, N.
%A Vitale, V.
%A P. Waite, A.
%A Wang, P.
%A Watters, K.
%A L. Winer, B.
%A T. Wolff, M.
%A S. Wood, K.
%A Ylinen, T.
%A Ziegler, M.
%< avec comité de lecture
%@ 0004-637X
%J The Astrophysical Journal
%I American Astronomical Society
%V 711
%P 64-74
%8 2010-03-01
%D 2010
%Z 1001.0792
%R 10.1088/0004-637X/711/1/64
%K gamma rays: general
%K pulsars: general
%K pulsars: individual (PSR J1907+0602)
%K supernovae: individual (SNR G40.5-0.5)
%Z Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Journal articles
%X We present multiwavelength studies of the 106.6 ms gamma-ray pulsar PSR J1907+06 near the TeV source MGRO J1908+06. Timing observations with Fermi result in a precise position determination for the pulsar of R.A. = 19h07m547(2), decl. = +06:02:16(2) placing the pulsar firmly within the TeV source extent, suggesting the TeV source is the pulsar wind nebula of PSR J1907+0602. Pulsed gamma-ray emission is clearly visible at energies from 100 MeV to above 10 GeV. The phase-averaged power-law index in the energy range E > 0.1 GeV is = 1.76 \pm 0.05 with an exponential cutoff energy E_{c} = 3.6 \pm 0.5 GeV. We present the energy-dependent gamma-ray pulsed light curve as well as limits on off-pulse emission associated with the TeV source. We also report the detection of very faint (flux density of ~3.4 microJy) radio pulsations with the Arecibo telescope at 1.5 GHz having a dispersion measure DM = 82.1 \pm 1.1 cm^{-3}pc. This indicates a distance of 3.2 \pm 0.6 kpc and a pseudo-luminosity of L_{1400} ~ 0.035 mJy kpc^2. A Chandra ACIS observation revealed an absorbed, possibly extended, compact <(4 arcsec) X-ray source with significant non-thermal emission at R.A. = 19h07m54.76, decl. = +06:02:14.6 with a flux of 2.3^{+0.6}_{-1.4} X 10^{-14} erg cm^{-2} s^{-1}. From archival ASCA observations, we place upper limits on any arcminute scale 2--10 keV X-ray emission of ~ 1 X 10^{-13} erg cm^{-2} s^{-1}. The implied distance to the pulsar is compatible with that of the supernova remnant G40.5-0.5, located on the far side of the TeV nebula from PSR J1907+0602, and the S74 molecular cloud on the nearer side which we discuss as potential birth sites.
%G English
%Z Fermi-LAT
%2 https://hal.in2p3.fr/in2p3-00461061/document
%2 https://hal.in2p3.fr/in2p3-00461061/file/1001.0792.pdf
%L in2p3-00461061
%U https://hal.in2p3.fr/in2p3-00461061
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