Results 11 to 20 of about 29,784,966 (285)
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 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 sourcesA Quality Improvement Initiative to Standardize Pneumocystis jirovecii Pneumonia Prophylaxis in Pediatric Patients With Solid Tumors
Pediatric Blood &Cancer, EarlyView.ABSTRACT Background
Pediatric patients with extracranial solid tumors (ST) receiving chemotherapy are at an increased risk for Pneumocystis jirovecii pneumonia (PJP). However, evidence guiding prophylaxis practices in this population is limited. A PJP‐related fatality at our institution highlighted inconsistent prescribing approaches and concerns about Kriti Kumar, Denise M. Connolly, Ellen Kellington, Elyse Zelunka, Karla Kerrigan, Furqan Shaikh, Paul C. Nathan, Meredith S. Irwin, Sarah Cohen‐Gogo +8 morewiley +1 more sourceSickle Cell Disease Is an Inherent Risk for Asthma in a Sibling Comparison Study
Pediatric Blood &Cancer, EarlyView.ABSTRACT Introduction
Sickle cell disease (SCD) and asthma share a complex relationship. Although estimates vary, asthma prevalence in children with SCD is believed to be comparable to or higher than the general population. Determining whether SCD confers an increased risk for asthma remains challenging due to overlapping symptoms and the ...Suhei C. Zuleta De Bernardis, Okeleji Olayinka, Mariam Z. Quraishi, Lakshmi V. Srivaths, Deborah L. Brown, Neethu M. Menon, Ricardo A. Mosquera, Ashwin P. Patel, James M. Stark, Aravind Yadav +9 morewiley +1 more source
