Results 11 to 20 of about 47,761,508 (79)
Identification of the TeV Gamma-ray Source ARGO J2031+4157 with the
Cygnus Cocoon [PDF]
, 2014 The extended TeV gamma-ray source ARGO J2031+4157 (or MGRO J2031+41) is
positionally consistent with the Cygnus Cocoon discovered by $Fermi$-LAT at GeV
energies in the Cygnus superbubble.15, 16, 16, 16, 18, 18, 19, 2, 2, 2, 2, 2, 21, 4, 4, 4, 4, 4, 4, 4, 4, 8, 8, 8, A. Budano6, A. D’Amone3, A. F. Yuan9, A. Surdo4, and G. Zizzi20
(The ARGO-YBJ Collaboration), B. Bartoli1, B. D’Ettorre Piazzoli1, B. Z. Dai11, C. C. Ning9, C. F. Feng12, C. Liu5, C. Vigorito18, C. Y. Wu5, D. Martello3, Danzengluobu9, F. R. Zhu13, F. Ruggieri6, F. Shi5, G. Di Sciascio8, G. Liguori14, G. Mancarella3, G. Marsella3, H. H. He5, H. J. Li9, H. Lu5, H. M. Zhang5, H. R. Wu5, H. Wang5, H. Y. Jia13, Haibing Hu9, Hongbo Hu5, I. De Mitri3, J. Liu11, J. Zhao5, L. L. Ma5, L. Perrone3, L. Xue12, L. Zhang11, Labaciren9, M. Iacovacci1, M. Panareo3, M. Y. Liu9, M. Zha5, Mari SM, P. Bernardini3, P. Branchini6, P. Camarri7, P. Creti4, P. Montini6, P. Pistilli6, P. R. Shen5, P. Salvini15, P. Vallania17, Q. B. Gou5, Q. Q. Zhu5, Q. Y. Yang11, R. Cardarelli8, R. Iuppa7, R. Santonico7, S. Catalanotti1, S. Mastroianni2, S. Vernetto17, S. W. Cui10, S. Z. Chen5, T. Di Girolamo1, T. L. Chen9, X. C. Yang11, X. D. Sheng5, X. H. Ma5, X. J. Bi5, X. X. Zhou13, X. Y. Zhang12, Y. H. Tan5, Y. Q. Guo5, Y. Zhang5, Z. Cao5, Z. G. Yao5, Zhaoyang Feng5, Zhaxiciren9, Zhaxisangzhu9, Zhenyong Feng13 +104 morecore +3 more sourcesFermi Large Area Telescope Observations of the Crab Pulsar and Nebula [PDF]
, 2009 We report on gamma-ray observations of the Crab Pulsar and Nebula using 8
months of survey data with the Fermi Large Area Telescope (LAT). The high
quality light curve obtained using the ephemeris provided by the Nancay and
Jodrell Bank radio telescopes ...10, 10, 10, 10, 12, 13, 13, 13, 15, 15, 15, 15, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 63, 2, 2, 24, 25, 24, 25, 24, 40, 26, 26, 30, 30, 62, 34, 34, 34, 34, 34, 34, 63, 34, 63, 34, 64, 39, 40, 40, 40, 46, 48, 53, 53, 54, 54, 61, 58, 59, 6, 60, 63, A. A. Abdo1, A. A. Moiseev23, A. Brez7, A. Chekhtman1, A. de Angelis31, A. de Luca32, A. G. Lyne35, A. K. Harding23, A. Makeev1, A. Morselli49, A. Noutsos35, A. P. Waite3, A. Reimer3, A. S. Johnson3, A. Sander42, A. Tramacere3, A. Van Etten3, A. W. Borgland3, A. Y. Rodriguez20, B. Berenji3, B. Giebels18, B. L. Winer42, B. Lott33, B. W. Stappers35, BONAMENTE, EMANUELE, C. C. Cheung1, C. D. Dermer1, C. Espinoza35, C. Farnier28, C. Favuzzi16, C. Meurer6, C. Monte16, C. Sgrò7, CECCHI, Claudia, D. A. Smith33, D. Bastieri12, D. Dumora33, D. F. Torres20, D. Gasparrini38, D. J. Suson57, D. J. Thompson23, D. Paneque3, D. Parent33, D. Sanchez18, E. C. Ferrara23, E. D. Bloom3, E. do Couto e. Silva3, E. Hays23, E. J. Siskind56, E. Moretti9, E. Nuss28, E. Orlando51, E. Wallace19, F. Camilo21, F. de Palma16, F. Gargano17, F. Giordano16, F. Kuehn42, F. Longo9, F. Loparco16, F. Piron28, F. Ryde6, G. A. Caliandro20, G. Barbiellini9, G. Giavitto9, G. Godfrey3, G. Jóhannesson3, G. Spandre7, G. Theureau27, H. F. W. Sadrozinski4, H. Katagiri37, H. Tajima3, H. Takahashi37, I. A. Grenier8, I. Cognard27, I. V. Moskalenko3, J. B. Thayer3, J. Ballet8, J. Bregeon7, J. Chiang3, J. Cohen Tanugi28, J. Conrad6, J. D. Scargle55, J. E. Grove1, J. E. McEnery23, J. F. Ormes50, J. G. Thayer3, J. H. Panetta3, J. Kataoka44, J. Knödlseder47, J. Lande3, J. M. Casandjian8, J. P. Norris50, K. Bechtol3, K. S. Wood1, K. Watters3, L. Baldini7, L. Guillemot33, L. Latronico7, L. R. Cominsky29, L. S. Rochester3, L. Tibaldo8, M. Ackermann3, M. Ajello3, M. Axelsson5, M. Brigida16, M. E. Monzani3, M. Frailis31, M. G. Baring11, M. H. Grondin33, M. Hayashida3, M. Kerr19, M. Kramer35, M. Kuss7, M. L. Kocian3, M. Lemoine Goumard33, M. Marelli22, M. N. Lovellette1, M. N. Mazziotta17, M. Ozaki52, M. Pepe14, M. Pesce Rollins7, M. Pierbattista8, M. Razzano7, M. Roth19, M. S. Strickman1, M. Ziegler4, N. Gehrels23, N. Giglietto16, N. Kawai45, N. Omodei7, N. Vilchez47, O. Reimer3, Ö. Çelik23, P. A. Caraveo22, P. Bruel18, P. C. C. Freire36, P. D. Smith42, P. F. Michelson3, P. Fusco16, P. L. Nolan3, P. Lubrano14, P. M. Saz Parkinson4, P. S. Drell3, P. S. Ray1, P. Spinelli16, P. Wang3, P. Weltevrede35, R. A. Cameron3, R. Bellazzini7, R. Claus3, R. D. Blandford3, R. Dubois3, R. E. Hughes42, R. P. Johnson4, R. Rando12, R. W. Romani3, S. Ciprini15, S. E. Thorsett4, S. Funk3, S. Germani14, S. Guiriec41, S. H. Lee3, S. J. Fegan18, S. Johnston43, S. Murgia3, S. Rainò16, S. Ritz4, S. W. Digel3, T. A. Porter4, T. Glanzman3, T. H. Burnett19, T. J. Johnson23, T. Kamae3, T. L. Usher3, T. Mizuno37, T. Nakamori45, T. Ohsugi37, T. Reposeur33, T. Tanaka3, T. Ylinen6, TOSTI, Gino, V. Pelassa28, V. Vasileiou23, V. Vitale49, W. B. Atwood4, W. B. Focke3, W. Mitthumsiri3, W. N. Johnson1, Y. Fukazawa37, Y. Hanabata37, Y. Uchiyama3 +243 morecore +7 more sourcesObservation of the TeV gamma-ray source MGRO J1908+06 with ARGO-YBJ [PDF]
, 2012 The extended gamma ray source MGRO J1908+06, discovered by the Milagro air
shower detector in 2007, has been observed for about 4 years by the ARGO-YBJ
experiment at TeV energies, with a statistical significance of 6.2 standard
deviations.00133 Roma, 00133 Roma, 00146 Roma, 00146 Roma, 100049 Beijing, 10125 Torino, 10125 Torino, 10133 Torino, 11, 11, 11, 11, 16, 18, 18, 18, 19, 19, 2, 2, 2, 2, 2, 2 North Cuihu Rd., 22, 22, 22, 22, 23, 250100 Jinan, 27100 Pavia, 27100 Pavia, 4, 4, 4, 4, 4, 40127 Bologna, 610031 Chengdu, 650091 Kunming, 7, 7, 7, 73100 Lecce, 73100 Lecce, 8, 80126 Napoli, 80126 Napoli, 850000 Lhasa, 90128 Palermo, 90146 Palermo, 95125 Catania, A. Budano8, A. F. Yuan12, A. K. Calabrese Melcarne9, A. Pagliaro16, A. Surdo4, and G. Zizzi9(The Argo-YBJ Collaboration)1 Dipartimento di Fisica dell’Universit`a di Napoli “Federico II, B. Bartoli1, B. D’Ettorre Piazzoli1, B. Panico10, B. Wang5, B. Xu21, B. Z. Dai14, C. Bleve3, C. C. Ning12, C. Cattaneo7, C. F. Feng20, C. Liu5, C. Q. Liu14, C. Stanescu8, C. Vigorito18, C. Y. Wu5, China13 Hebei Normal University, China14 Yunnan University, China15 Dipartimento di Fisica, China21 Southwest Jiaotong University, China22 Dipartimento di Fisica dell’Universit`a “Roma Tre, China6 Dipartimento di Fisica Nucleare e Teorica dell’Universit`a di Pavia, Chinese Academy of Sciences, Complesso Universitario di Monte Sant’Angelo, corso Fiume 4, D. Martello3, Danzengluobu12, E. Giroletti6, Edificio 18, F. Galeazzi8, F. R. Zhu21, F. Ruggieri8, F. Shi5, G. Di Sciascio11, G. D’Al´ı Staiti15, G. Liguori6, G. Mancarella3, G. Marsella4, H. H. He5, H. J. Li12, H. Lu5, H. M. Zhang5, H. R. Wu5, H. Wang5, H. Y. Jia21, Haibing Hu12, Hebei, Hongbo Hu5, I. Bolognino6, I. De Mitri3, I. James8, Institute of High Energy Physics, Italy, Italy10 Dipartimento di Fisica dell’Universit`a di Roma “Tor Vergata, Italy11 Istituto Nazionale di Fisica Nucleare, Italy12 Tibet University, Italy16 Istituto Nazionale di Fisica Nucleare, Italy17 Osservatorio Astrofisico di Torino dell’Istituto Nazionale di Astrofisica, Italy18 Istituto Nazionale di Fisica Nucleare, Italy19 Dipartimento di Fisica dell’Universit`a di Torino, Italy2 Istituto Nazionale di Fisica Nucleare, Italy20 Shandong University, Italy23 Istituto di Astrofisica Spaziale e Fisica Cosmica dell’Istituto Nazionale di Astrofisica, Italy3 Dipartimento di Matematica e Fisica “Ennio De Giorgi, Italy4 Istituto Nazionale di Fisica Nucleare, Italy5 Key Laboratory of Particle Astrophysics, Italy7 Istituto Nazionale di Fisica Nucleare, Italy8 Istituto Nazionale di Fisica Nucleare, Italy9 Istituto Nazionale di Fisica Nucleare-CNAF, J. Liu14, J. Y. Li20, Jianli Zhang5, Jilong Zhang5, L. Perrone4, L. Xue20, L. Zhang14, Labaciren12, M. Dattoli17, M. Iacovacci1, M. Panareo4, M. Y. Liu12, M. Zha5, Mari SM, P. Bernardini3, P. Branchini8, P. Camarri10, P. Creti4, P. Montini8, P. Pistilli8, P. R. Shen5, P. Salvini7, P. Vallania17, P. Zhang14, P.O. Box 918, Q. B. Gou5, Q. Huang21, Q. Q. Zhu5, Q. Y. Yang14, R. Cardarelli11, R. Iuppa10, R. Santonico10, S. Catalanotti1, S. Mastroianni2, S. Vernetto17, S. W. Cui13, S. Z. Chen5, Sezione di Catania, Sezione di Lecce, Sezione di Napoli, Sezione di Pavia, Sezione di Roma Tor Vergata, Sezione di Roma Tre, Sezione di Torino, Shandong, Shijiazhuang 050016, Sichuan, T. Di Girolamo1, T. L. Chen12, Universit`a degli Studi di Palermo, via Bassi 6, via Bassi 6, via Cinthia, via Cinthia, via della Ricerca Scientifica 1, via della Vasca Navale 84, via La Malfa 153, via P. Giuria 1, via P. Giuria 1, via per Arnesano, via per Arnesano, Viale A. Doria 6, Viale Berti-Pichat 6/2, Viale delle Scienze, X. B. Qu20, X. C. Yang14, X. D. Sheng5, X. H. Ding12, X. H. Ma5, X. J. Bi5, X. X. Li5, X. X. Zhou21, X. Y. Zhang20, Xizang, Y. Chen5, Y. H. Tan5, Y. Q. Guo5, Y. X. Yan14, Y. Zhang5, Yunnan, Z. Cao5, Z. G. Yao5, Zhaoyang Feng5, Zhaxiciren12, Zhaxisangzhu12, Zhenyong Feng21, ” Complesso Universitario di Monte Sant’Angelo, ” Universit`a del Salento, ” via della Ricerca Scientifica 1, ” via della Vasca Navale 84 +215 morecore +3 more sourcesVector and axial-vector couplings of D and D* mesons in 2+1 flavor
Lattice QCD [PDF]
, 2013 Using the axial-vector coupling and the electromagnetic form factors of the D
and D* mesons in 2+1 flavor Lattice QCD, we compute the D*D\pi, DD\rho and
D*D*\rho coupling constants, which play an important role in describing the
charm hadron interactions Can, K. U., Erkol, G., Oka, M., Ozpineci, A., Takahashi, T. T. +4 morecore +2 more sourcesSpectral analysis of 50 GRBs detected by HETE-2 [PDF]
, 2003 FREGATE, the gamma-ray detector of HETE-2 is entirely dedicated to the study
of GRBs. Its main characteristic is its broad energy range, from 7 keV to 400
keV. This energy range can be further extended down to 2 keV using the data
from the WXM, the X-ray Barraud, C., team, the HETE-2core +3 more sources
