Results 11 to 20 of about 34,962 (144)
Periodontitis and atherosclerotic cardiovascular disease: A critical appraisal
Periodontology 2000, EarlyView., 2023 Abstract
In spite of intensive research efforts driving spectacular advances in terms of prevention and treatments, cardiovascular diseases (CVDs) remain a leading health burden, accounting for 32% of all deaths (World Health Organization. “Cardiovascular Diseases (CVDs).” WHO, February 1, 2017, https://www.who.int/news‐room/fact‐sheets/detail ...Maria Clotilde Carra, Hélène Rangé, Giuseppina Caligiuri, Philippe Bouchard +3 morewiley +1 more sourceTumor-infiltrating T cells correlate with NY-ESO-1-specific autoantibodies in ovarian cancer. [PDF]
PLoS ONE, 2008 BACKGROUND: Tumor-infiltrating CD8+ T cells are correlated with prolonged progression-free and overall survival in epithelial ovarian cancer (EOC). A significant fraction of EOC patients mount autoantibody responses to various tumor antigens, however the Katy Milne, Rebecca O Barnes, Adam Girardin, Melanie A Mawer, Nancy J Nesslinger, Alvin Ng, Julie S Nielsen, Robert Sahota, Eric Tran, John R Webb, May Q Wong, Darin A Wick, Andrew Wray, Elissa McMurtrie, Martin Köbel, Steven E Kalloger, C Blake Gilks, Peter H Watson, Brad H Nelson +18 moredoaj +1 more sourceARGO-YBJ: Status and Highlights [PDF]
, 2012 The ARGO-YBJ experiment is in stable data taking since November 2007 at the
YangBaJing Cosmic Ray Laboratory (Tibet, P.R. China, 4300 m a.s.l., 606
g/cm$^2$). ARGO-YBJ is facing open problems in Cosmic Ray (CR) physics in
different ways.Di Sciascio, G.core +4 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 sourcesOlivier Chesneau's work on massive stars [PDF]
, 2015 Olivier Chesneau challenged several fields of observational stellar
astrophysics with bright ideas and an impressive amount of work to make them
real in the span of his career, from his first paper on P Cygni in 2000, up to
his last one on V838 Mon in ...Millour, Florentincore +4 more sourcesMonte Carlo Performance Studies for the Site Selection of the Cherenkov
Telescope Array [PDF]
, 2017 The Cherenkov Telescope Array (CTA) represents the next generation of
ground-based instruments for very-high-energy (VHE) gamma-ray astronomy, aimed
at improving on the sensitivity of current-generation experiments by an order
of magnitude and providing ...Arrabito, L., Bernlöhr, K., Bregeon, J., Cortina, J., Cumani, P., Di Pierro, F., Falceta-Goncalves, D., Hassan, T., Hinton, J., Jogler, T., Lang, R. G., Maier, G., Moralejo, A., Morselli, A., Peixoto, C. J. Todero, Wood, M. +15 morecore +3 more sourcesInvestigations of fast neutron production by 190 GeV/c muon interactions
on different targets [PDF]
, 2001 The production of fast neutrons (1 MeV - 1 GeV) in high energy muon-nucleus
interactions is poorly understood, yet it is fundamental to the understanding
of the background in many underground experiments. The aim of the present
experiment (CERN NA55) was Boehm, F., Chazal, V., Cook, B., Henrikson, H., Jonkmans, G., Mascarenhas, N., Paic, A., Vogel, P., Vuilleumier, J. -L. +8 morecore +2 more sourcesRoute diversity analyses for free-space optical wireless links within turbulent scenarios [PDF]
, 2013 Free-Space Optical (FSO) communications link performance is highly affected when propagating through the time-spatially variable turbulent environment.Anguita, Belmonte, Chatzidiamantis, Gappmair, Ghassemlooy, Grabner, Jeganathan, Jiri Libich, Joaquin Perez, Kaneko, Kashyap, Khalighi, Ko, Lee, Lee, Letzepis, Libich, Moradi, Navidpour, Perez, Popoola, Popoola, Rosenberg, Stanislav Zvanovec, Sujan Rajbhandari, Tsiftsis, Tyson, Walther, Zabih Ghassemlooy, Zhu +29 morecore +2 more sources
