Results 11 to 20 of about 29,978,210 (287)
Observation 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 sourcesFermi LAT observations of cosmic-ray electrons from 7 GeV to 1 TeV [PDF]
, 2010 We present the results of our analysis of cosmic-ray electrons using about 8
million electron candidates detected in the first 12 months on-orbit by the
Fermi Large Area Telescope.1, 1, 11, 11, 13, 13, 13, 13, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 22, 22, 22, 22, 22, 23, 24, 25, 25, 25, 27, 27, 27, 28, 38, 38, 38, 38, 40, 42, 42, *, 49, 50, 53, 54, 55, 22, 6, 6, 6, 8, 8, 8, 8, 8, 4, 9, A. A. Moiseev24, A. Brez3, A. Chekhtman26, A. de Angelis33, A. Drlica Wagner1, A. K. Harding23, A. Makeev26, A. Morselli10, A. N. Cillis29, A. Okumura45, A. P. Waite1, A. Reimer47, A. S. Johnson1, A. Sander9, A. Tramacere1, A. W. Borgland1, A. W. Strong46, B. Berenji1, B. L. Winer9, B. Lott37, B. M. Baughman9, BONAMENTE, EMANUELE, C. C. Cheung26, C. D. Dermer26, C. Favuzzi15, C. Monte15, C. Sgrò3, CECCHI, Claudia, D. Bastieri7, D. F. Torres19, D. Fabiani3, D. Gaggero3, D. Gasparrini35, D. Grasso3, D. Hadasch40, D. Horan17, D. J. Suson51, D. J. Thompson23, D. Paneque1, D. Parent26, D. Sanchez17, E. Charles1, E. D. Bloom1, E. do Couto e. Silva1, E. Hays23, E. J. Siskind48, E. Moretti5, E. Nuss30, E. Orlando46, E. Rapposelli3, E. Wallace18, F. Bellardi3, F. Belli10, F. de Palma15, F. Gargano16, F. Giordano15, F. Longo5, F. Loparco15, F. Piron30, G. A. Caliandro19, G. Barbiellini5, G. Busetto7, G. Di Bernardo3, G. Godfrey1, G. Jóhannesson1, G. Spandre3, H. F. W. Sadrozinski2, H. Katagiri34, H. Tajima1, H. Takahashi44, I. A. Grenier4, I. V. Moskalenko1, J. B. Thayer1, J. Ballet4, J. Bregeon3, J. Chiang1, J. Cohen Tanugi30, J. Conrad31, J. E. Grove26, J. E. McEnery23, J. F. Ormes43, J. G. Thayer1, J. H. Panetta1, J. Kataoka41, J. Knödlseder14, J. Lande1, J. M. Casandjian4, J. Mehault30, J. P. Norris43, J. R. Bogart1, J. Ripken31, J. Vandenbroucke1, K. Bechtol1, K. S. Wood26, L. Baldini3, L. Latronico3, L. S. Rochester1, L. Tibaldo7, M. Ackermann1, M. Ajello1, M. Brigida15, M. Ceccanti3, M. DeKlotz32, M. E. Monzani1, M. Giroletti36, M. Gustafsson7, M. H. Grondin37, M. Hayashida1, M. Kerr18, M. Kuss3, M. Lemoine Goumard37, M. Llena Garde31, M. Minuti3, M. N. Lovellette26, M. N. Mazziotta16, M. Naumann Godo4, M. Ozaki45, M. Pepe12, M. Pesce Rollins3, M. Pinchera3, M. Razzano3, M. Roth18, M. S. Strickman26, M. Turri1, M. Ziegler2, N. Gehrels23, N. Giglietto15, N. Omodei1, N. Saggini3, N. Vilchez14, O. Reimer47, O. Tibolla52, Ö. Çelik23, P. A. Caraveo20, P. Bruel17, P. Carlson21, P. D. Smith9, P. F. Michelson1, P. Fortin17, P. Fusco15, P. Giommi35, P. L. Nolan1, P. Lubrano12, P. S. Drell1, P. Spinelli15, P. Wang1, R. A. Cameron1, R. Bellazzini3, R. Buehler1, R. Claus1, R. Corbet23, R. D. Blandford1, R. Dubois1, R. E. Hughes9, R. P. Johnson2, R. Rando7, R. W. Romani1, S. Buson7, S. Carrigan8, S. Ciprini13, S. Funk1, S. Germani12, S. Guiriec39, S. J. Fegan17, S. Murgia1, S. Profumo2, S. Rainò15, S. Ritz2, S. W. Digel1, T. A. Porter1, T. E. Stephens23, T. Glanzman1, T. H. Burnett18, T. J. Brandt14, T. Kamae1, T. L. Usher1, T. Mizuno34, T. Nakamori41, T. Ohsugi44, T. Reposeur37, T. Takahashi45, T. Tanaka1, T. Ylinen21, TOSTI, Gino, V. Pelassa30, V. Petrosian1, V. Vasileiou24, V. Vitale10, W. B. Atwood2, W. Mitthumsiri1, W. N. Johnson26, Y. Fukazawa34, Y. Uchiyama1, Z. Yang31, Ł. Stawarz45, † +246 morecore +4 more sourcesBiohydrogenation of 22:6n-3 by Butyrivibrio proteoclasticus P18 [PDF]
, 2016 Background: Rumen microbes metabolize 22:6n-3. However, pathways of 22:6n-3 biohydrogenation and ruminal microbes involved in this process are not known.AA AbuGhazaleh, B Vlaeminck, Bruno Vlaeminck, CE Polan, CG Harfoot, CG Harfoot, D Paillard, F Destaillats, G Dobson, H Sakurama, I Wasowska, Jeyamalar Jeyanathan, KJ Shingfield, KJ Shingfield, KJ Shingfield, Marlene Escobar, MR Maia, MRG Maia, P Kairenius, QT Yu, RG Ackman, RJ Forster, RJ Wallace, RL Wolff, Robert John Wallace, SA Huws, TC Jenkins, Veerle Fievez, WJ Hunter, WW Christie, YJ Kim +30 morecore +2 more sourcesUpdated Post-WMAP Benchmarks for Supersymmetry
, 2003 We update a previously-proposed set of supersymmetric benchmark scenarios,
taking into account the precise constraints on the cold dark matter density
obtained by combining WMAP and other cosmological data, as well as the LEP and
b -> s gamma constraints.148, 22, 25, A. De Roeck, Allanach, Baer, Baer, Belanger, Carena, Collaboration], Collaboration], Drees, Drees, Ellis, Ellis, Ellis, Ellis, F. Gianotti, Feng, Heinemeyer, Hinchliffe, J. Ellis, K. A. Olive, Kane, L. Pape, Lahanas, M. Battaglia, Maiani, Pierce, See +29 morecore +1 more sourceReconclining phi radiative decays with other data for a0(980), fo(980),
pi-pi -> KK and pi-pi -> eta-eta
, 2006 Data for phi -> gamma (eta-pizero) are analysed using the KK loop model and
compared with parameters of a0(980) derived from Crystal Barrel data. The
eta-pi mass spectrum agrees closely and the absolute normalisation lies just
within errors. However, BES (PDG), 15, 175, 19, 22, 25, 26, 327, 33, 353, 36, 438, 440, 449, 462, 472, 509, 536, 537, 598, 603, 607, 64, 78, 87, Achasov, Achasov, Achasov, Achasov, Anisovich, Anisovich, Au, Bolgione, Bugg, Bugg, Bugg, Bugg, Close, D.V. Bugg, Dalitz, Jamin, Lindenbaum, Marco, Martin, Moxhay, Nicola, Oller, Oller, Oller, Oller, Palomar, Zou +51 morecore +1 more sourceA catch‐22: Interleukin‐22 and cancer [PDF]
European Journal of Immunology, 2018 AbstractBarrier surfaces of multicellular organisms are in constant contact with the environment and infractions to the integrity of epithelial surfaces is likely a frequent event. Interestingly, components of the immune system, that can be activated by environmental compounds such as the microbiota or nutrients, are interspersed among epithelial cells Pedro Hernandez, Konrad Gronke, Andreas Diefenbach +2 moreopenaire +2 more sourcesDexamethasone for Chemotherapy‐Induced Nausea and Vomiting Prevention in Pediatric Patients: International Consensus
Pediatric Blood &Cancer, EarlyView.ABSTRACT Background
An international Delphi panel of experts developed consensus statements to delineate the circumstances where the risks of dexamethasone as an antiemetic do and do not outweigh its benefits. Procedure
Experts in supportive care of pediatric patients were invited to participate.Negar Shavandi, Paula D. Robinson, Shana Jacobs, L. Lee Dupuis, the International Pediatric Dexamethasone Panel, Sameer Bakhshi, Tiene Bauters, Eva Brack, Simone Cesaro, Claire Fosbrook, Jason Freedman, Tamara MacDonald, Eloise Neumann, Venkatraman Radhakrishnan, Rod Rassekh, Florian Slimano, Johnathan Soggee, Joel Thompson, Marianne van de Wetering, Milena Villarroel, Jasper Wong +20 morewiley +1 more sourceReal‐World Pediatric Blinatumomab Administration: Access to Outpatient Care Delivery and Impact of a Hospital‐Dispensed Model
Pediatric Blood &Cancer, EarlyView.ABSTRACT
Blinatumomab has been shown to be highly effective for patients with pediatric B‐ALL and has recently become standard of care therapy. Due to its past use in the clinical trial setting, there is limited information available about real‐world administration.Katelyn Oranges, Kelly A. Duffy, Sara McDonough, Evelyn Kurpiewski, R. Jennifer Randall, Allison Barz Leahy, Haley M. Newman, Joyce P. Lee, Stephen P. Hunger, Anne F. Reilly, David T. Teachey, Susan R. Rheingold, Daniel J. Zheng +12 morewiley +1 more source
