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Abeysekara A, Albert A, Alfaro R, Alvarez C, Álvarez J, Arceo R, Arteaga-Velázquez J, Avila Rojas D, Ayala Solares H, Belmont-Moreno E, BenZvi S, Braun J, Brisbois C, Caballero-Mora K, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Diaz Hernandez R, Dichiara S, Dingus B, DuVernois M, Ellsworth R, Engel K, Enríquez-Rivera O, Fleischhack H, Fraija N, Galván-Gámez A, García-González J, González Muñoz A, González M, Hampel-Arias Z, Harding J, Hernandez S, Hona B, Hueyotl-Zahuantitla F, Hui C, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Lara A, Lee W, León Vargas H, Linnemann J, Longinotti A, Luis-Raya G, Luna-García R, López-Coto R, Malone K, Marinelli S, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews J, Miranda-Romagnoli P, Moreno E, Mostafá M, Nellen L, Newbold M, Nisa M, Noriega-Papaqui R, Pelayo R, Pretz J, Pérez-Pérez E, Ren Z, Rho C, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Seglar Arroyo M, Sinnis G, Smith A, Springer R, Surajbali P, Taboada I, Tibolla O, Torres I, Villaseñor L, Weisgarber T, Westerhoff S, Wood J, Yapici T, Yodh G, Zepeda A, Zhou H. Constraining the
p¯/p
ratio in TeV cosmic rays with observations of the Moon shadow by HAWC. Int J Clin Exp Med 2018. [DOI: 10.1103/physrevd.97.102005] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Abeysekara AU, Albert A, Alfaro R, Alvarez C, Álvarez JD, Arceo R, Arteaga-Velázquez JC, Avila Rojas D, Ayala Solares HA, Barber AS, Bautista-Elivar N, Becerril A, Belmont-Moreno E, BenZvi SY, Berley D, Bernal A, Braun J, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Dingus BL, DuVernois MA, Díaz-Vélez JC, Ellsworth RW, Engel K, Enríquez-Rivera O, Fiorino DW, Fraija N, García-González JA, Garfias F, Gerhardt M, González Muñoz A, González MM, Goodman JA, Hampel-Arias Z, Harding JP, Hernández S, Hernández-Almada A, Hinton J, Hona B, Hui CM, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Kieda D, Lara A, Lauer RJ, Lee WH, Lennarz D, Vargas HL, Linnemann JT, Longinotti AL, Luis Raya G, Luna-García R, López-Coto R, Malone K, Marinelli SS, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews JA, Miranda-Romagnoli P, Moreno E, Mostafá M, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Pelayo R, Pretz J, Pérez-Pérez EG, Ren Z, Rho CD, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salazar H, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Sinnis G, Smith AJ, Springer RW, Surajbali P, Taboada I, Tibolla O, Tollefson K, Torres I, Ukwatta TN, Vianello G, Weisgarber T, Westerhoff S, Wisher IG, Wood J, Yapici T, Yodh G, Younk PW, Zepeda A, Zhou H, Guo F, Hahn J, Li H, Zhang H. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth. Science 2018; 358:911-914. [PMID: 29146808 DOI: 10.1126/science.aan4880] [Citation(s) in RCA: 211] [Impact Index Per Article: 35.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/20/2017] [Accepted: 10/09/2017] [Indexed: 11/02/2022]
Abstract
The unexpectedly high flux of cosmic-ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary production. We report the detection, using the High-Altitude Water Cherenkov Observatory (HAWC), of extended tera-electron volt gamma-ray emission coincident with the locations of two nearby middle-aged pulsars (Geminga and PSR B0656+14). The HAWC observations demonstrate that these pulsars are indeed local sources of accelerated leptons, but the measured tera-electron volt emission profile constrains the diffusion of particles away from these sources to be much slower than previously assumed. We demonstrate that the leptons emitted by these objects are therefore unlikely to be the origin of the excess positrons, which may have a more exotic origin.
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Affiliation(s)
- A U Abeysekara
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - A Albert
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - R Alfaro
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - C Alvarez
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - J D Álvarez
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - R Arceo
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | | | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H A Ayala Solares
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A S Barber
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | | | - A Becerril
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - E Belmont-Moreno
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - S Y BenZvi
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - D Berley
- Department of Physics, University of Maryland, College Park, MD, USA
| | - A Bernal
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J Braun
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - C Brisbois
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | | | - T Capistrán
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - S Casanova
- Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland.,Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - M Castillo
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J Cotzomi
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - S Coutiño de León
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - C De León
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - E De la Fuente
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico
| | - B L Dingus
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico
| | - R W Ellsworth
- School of Physics, Astronomy, and Computational Sciences, George Mason University, Fairfax, VA, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, MD, USA
| | - O Enríquez-Rivera
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - D W Fiorino
- Department of Physics, University of Maryland, College Park, MD, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J A García-González
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - F Garfias
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Gerhardt
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A González Muñoz
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M M González
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, MD, USA
| | - Z Hampel-Arias
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J P Harding
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - S Hernández
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Hernández-Almada
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J Hinton
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - B Hona
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - C M Hui
- Astrophysics Office, NASA Marshall Space Flight Center Huntsville, AL, USA
| | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A Iriarte
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Jardin-Blicq
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - V Joshi
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - S Kaufmann
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - D Kieda
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - A Lara
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - R J Lauer
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - W H Lee
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - D Lennarz
- School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, USA
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - A L Longinotti
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - G Luis Raya
- Universidad Politecnica de Pachuca, Pachuca, Hidalgo, Mexico
| | - R Luna-García
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - R López-Coto
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany.
| | - K Malone
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - S S Marinelli
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - O Martinez
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | | | - J Martínez-Castro
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - H Martínez-Huerta
- Physics Department, Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City, Mexico
| | - J A Matthews
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | | | - E Moreno
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - M Mostafá
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Newbold
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - M U Nisa
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | | | - R Pelayo
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - J Pretz
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - E G Pérez-Pérez
- Universidad Politecnica de Pachuca, Pachuca, Hidalgo, Mexico
| | - Z Ren
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - C D Rho
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - C Rivière
- Department of Physics, University of Maryland, College Park, MD, USA
| | - D Rosa-González
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - M Rosenberg
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - E Ruiz-Velasco
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H Salazar
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland.
| | - A Sandoval
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Schneider
- Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - H Schoorlemmer
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - G Sinnis
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - A J Smith
- Department of Physics, University of Maryland, College Park, MD, USA
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - P Surajbali
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - I Taboada
- School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, USA
| | - O Tibolla
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - I Torres
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - T N Ukwatta
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - G Vianello
- Hansen Experimental Physics Laboratory Stanford University, Stanford, CA, USA
| | - T Weisgarber
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - S Westerhoff
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - I G Wisher
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J Wood
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - T Yapici
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - G Yodh
- Department of Physics and Astronomy, University of California, Irvine, Irvine, CA, USA
| | - P W Younk
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - A Zepeda
- Physics Department, Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City, Mexico.,Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - H Zhou
- Los Alamos National Laboratory, Los Alamos, NM, USA.
| | - F Guo
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - J Hahn
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - H Li
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - H Zhang
- Los Alamos National Laboratory, Los Alamos, NM, USA
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3
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Alfaro R, Alvarez C, Álvarez J, Arceo R, Arteaga-Velázquez J, Avila Rojas D, Ayala Solares H, Barber A, Becerril A, Belmont-Moreno E, BenZvi S, Brisbois C, Caballero-Mora K, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Diaz Hernandez R, Dichiara S, Dingus B, DuVernois M, Díaz-Vélez J, Ellsworth R, Enriquez-Rivera O, Fiorino D, Fleischhack H, Fraija N, García-González J, González Muñoz A, González M, Goodman J, Hampel-Arias Z, Harding J, Hernandez-Almada A, Hinton J, Hueyotl-Zahuantitla F, Hui C, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Lara A, Lauer R, Lennarz D, León Vargas H, Linnemann J, Longinotti A, Luis Raya G, Luna-García R, López-Cámara D, López-Coto R, Malone K, Marinelli S, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews J, Miranda-Romagnoli P, Moreno E, Mostafá M, Nellen L, Newbold M, Nisa M, Noriega-Papaqui R, Pelayo R, Pretz J, Pérez-Pérez E, Ren Z, Rho C, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Sinnis G, Smith A, Springer R, Surajbali P, Taboada I, Tibolla O, Tollefson K, Torres I, Ukwatta T, Villaseñor L, Weisgarber T, Westerhoff S, Wood J, Yapici T, Zepeda A, Zhou H. All-particle cosmic ray energy spectrum measured by the HAWC experiment from 10 to 500 TeV. Int J Clin Exp Med 2017. [DOI: 10.1103/physrevd.96.122001] [Citation(s) in RCA: 42] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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4
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Aleksić J, Ansoldi S, Antonelli LA, Antoranz P, Babic A, Bangale P, Barrio JA, González JB, Bednarek W, Bernardini E, Biasuzzi B, Biland A, Blanch O, Bonnefoy S, Bonnoli G, Borracci F, Bretz T, Carmona E, Carosi A, Colin P, Colombo E, Contreras JL, Cortina J, Covino S, Da Vela P, Dazzi F, De Angelis A, De Caneva G, De Lotto B, Wilhelmi EDO, Mendez CD, Prester DD, Dorner D, Doro M, Einecke S, Eisenacher D, Elsaesser D, Fonseca MV, Font L, Frantzen K, Fruck C, Galindo D, López RJG, Garczarczyk M, Terrats DG, Gaug M, Godinović N, Muñoz AG, Gozzini SR, Hadasch D, Hanabata Y, Hayashida M, Herrera J, Hildebrand D, Hose J, Hrupec D, Idec W, Kadenius V, Kellermann H, Kodani K, Konno Y, Krause J, Kubo H, Kushida J, La Barbera A, Lelas D, Lewandowska N, Lindfors E, Lombardi S, Longo F, López M, López-Coto R, López-Oramas A, Lorenz E, Lozano I, Makariev M, Mallot K, Maneva G, Mankuzhiyil N, Mannheim K, Maraschi L, Marcote B, Mariotti M, Martínez M, Mazin D, Menzel U, Miranda JM, Mirzoyan R, Moralejo A, Munar-Adrover P, Nakajima D, Niedzwiecki A, Nilsson K, Nishijima K, Noda K, Orito R, Overkemping A, Paiano S, Palatiello M, Paneque D, Paoletti R, Paredes JM, Paredes-Fortuny X, Persic M, Poutanen J, Moroni PGP, Prandini E, Puljak I, Reinthal R, Rhode W, Ribó M, Rico J, Garcia JR, Rügamer S, Saito T, Saito K, Satalecka K, Scalzotto V, Scapin V, Schultz C, Schweizer T, Shore SN, Sillanpää A, Sitarek J, Snidaric I, Sobczynska D, Spanier F, Stamatescu V, Stamerra A, Steinbring T, Storz J, Strzys M, Takalo L, Takami H, Tavecchio F, Temnikov P, Terzić T, Tescaro D, Teshima M, Thaele J, Tibolla O, Torres DF, Toyama T, Treves A, Uellenbeck M, Vogler P, Zanin R, Kadler M, Schulz R, Ros E, Bach U, Krauß F, Wilms J. Black hole lightning due to particle acceleration at subhorizon scales. Science 2014; 346:1080-4. [DOI: 10.1126/science.1256183] [Citation(s) in RCA: 100] [Impact Index Per Article: 10.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Affiliation(s)
- J. Aleksić
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | - S. Ansoldi
- Università di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy
| | - L. A. Antonelli
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | - P. Antoranz
- Università di Siena and INFN Pisa, I-53100 Siena, Italy
| | - A. Babic
- Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia
| | - P. Bangale
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | | | - J. Becerra González
- Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
- Present address: NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA, and Department of Physics and Department of Astronomy, University of Maryland, College Park, MD 20742, USA
| | | | - E. Bernardini
- Deutsches Elektronen-Synchrotron, D-15738 Zeuthen, Germany
| | - B. Biasuzzi
- Università di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy
| | - A. Biland
- ETH Zurich, CH-8093 Zurich, Switzerland
| | - O. Blanch
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | - S. Bonnefoy
- Universidad Complutense, E-28040 Madrid, Spain
| | - G. Bonnoli
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | - F. Borracci
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - T. Bretz
- Universität Würzburg, D-97074 Würzburg, Germany
- Present address: Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland
| | - E. Carmona
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, E-28040 Madrid, Spain
| | - A. Carosi
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | - P. Colin
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - E. Colombo
- Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
| | | | - J. Cortina
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | - S. Covino
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | - P. Da Vela
- Università di Siena and INFN Pisa, I-53100 Siena, Italy
| | - F. Dazzi
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - A. De Angelis
- Università di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy
| | - G. De Caneva
- Deutsches Elektronen-Synchrotron, D-15738 Zeuthen, Germany
| | - B. De Lotto
- Università di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy
| | | | - C. Delgado Mendez
- Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, E-28040 Madrid, Spain
| | - D. Dominis Prester
- Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia
| | - D. Dorner
- Universität Würzburg, D-97074 Würzburg, Germany
| | - M. Doro
- Università di Padova and INFN, I-35131 Padova, Italy
| | - S. Einecke
- Technische Universität Dortmund, D-44221 Dortmund, Germany
| | | | | | | | - L. Font
- Unitat de Física de les Radiacions, Departament de Física, and Centro de Estudios e Investigación Espaciales-Institut d’Estudis Espacials de Catalunya, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain
| | - K. Frantzen
- Technische Universität Dortmund, D-44221 Dortmund, Germany
| | - C. Fruck
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - D. Galindo
- Universitat de Barcelona, Institut de Ciències del Cosmos, Institut d’Estudis Espacials de Catalunya-Universitat de Barcelona, E-08028 Barcelona, Spain
| | - R. J. García López
- Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
| | - M. Garczarczyk
- Deutsches Elektronen-Synchrotron, D-15738 Zeuthen, Germany
| | - D. Garrido Terrats
- Unitat de Física de les Radiacions, Departament de Física, and Centro de Estudios e Investigación Espaciales-Institut d’Estudis Espacials de Catalunya, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain
| | - M. Gaug
- Unitat de Física de les Radiacions, Departament de Física, and Centro de Estudios e Investigación Espaciales-Institut d’Estudis Espacials de Catalunya, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain
| | - N. Godinović
- Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia
| | - A. González Muñoz
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | - S. R. Gozzini
- Deutsches Elektronen-Synchrotron, D-15738 Zeuthen, Germany
| | - D. Hadasch
- Institute of Space Sciences, E-08193 Barcelona, Spain
- Present address: Institut für Astro- und Teilchenphysik, Leopold-Franzens-Universität Innsbruck, A-6020 Innsbruck, Austria
| | - Y. Hanabata
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - M. Hayashida
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - J. Herrera
- Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
| | | | - J. Hose
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - D. Hrupec
- Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia
| | - W. Idec
- University of Łódz', PL-90236 Lodz, Poland
| | - V. Kadenius
- Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland
| | - H. Kellermann
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - K. Kodani
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - Y. Konno
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - J. Krause
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - H. Kubo
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - J. Kushida
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - A. La Barbera
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | - D. Lelas
- Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia
| | | | - E. Lindfors
- Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland
- Present address: Finnish Centre for Astronomy with ESO (FINCA), Turku, Finland
| | - S. Lombardi
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | - F. Longo
- Università di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy
| | - M. López
- Universidad Complutense, E-28040 Madrid, Spain
| | - R. López-Coto
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | - A. López-Oramas
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | | | - I. Lozano
- Universidad Complutense, E-28040 Madrid, Spain
| | - M. Makariev
- Institute for Nuclear Research and Nuclear Energy, BG-1784 Sofia, Bulgaria
| | - K. Mallot
- Deutsches Elektronen-Synchrotron, D-15738 Zeuthen, Germany
| | - G. Maneva
- Institute for Nuclear Research and Nuclear Energy, BG-1784 Sofia, Bulgaria
| | - N. Mankuzhiyil
- Università di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy
- Present address: Astrophysics Science Division, Bhabha Atomic Research Centre, Mumbai 400085, India
| | - K. Mannheim
- Universität Würzburg, D-97074 Würzburg, Germany
| | - L. Maraschi
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | - B. Marcote
- Universitat de Barcelona, Institut de Ciències del Cosmos, Institut d’Estudis Espacials de Catalunya-Universitat de Barcelona, E-08028 Barcelona, Spain
| | - M. Mariotti
- Università di Padova and INFN, I-35131 Padova, Italy
| | - M. Martínez
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | - D. Mazin
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - U. Menzel
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - J. M. Miranda
- Università di Siena and INFN Pisa, I-53100 Siena, Italy
| | - R. Mirzoyan
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - A. Moralejo
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | - P. Munar-Adrover
- Universitat de Barcelona, Institut de Ciències del Cosmos, Institut d’Estudis Espacials de Catalunya-Universitat de Barcelona, E-08028 Barcelona, Spain
| | - D. Nakajima
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | | | - K. Nilsson
- Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland
- Present address: Finnish Centre for Astronomy with ESO (FINCA), Turku, Finland
| | - K. Nishijima
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - K. Noda
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - R. Orito
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - A. Overkemping
- Technische Universität Dortmund, D-44221 Dortmund, Germany
| | - S. Paiano
- Università di Padova and INFN, I-35131 Padova, Italy
| | - M. Palatiello
- Università di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy
| | - D. Paneque
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - R. Paoletti
- Università di Siena and INFN Pisa, I-53100 Siena, Italy
| | - J. M. Paredes
- Universitat de Barcelona, Institut de Ciències del Cosmos, Institut d’Estudis Espacials de Catalunya-Universitat de Barcelona, E-08028 Barcelona, Spain
| | - X. Paredes-Fortuny
- Universitat de Barcelona, Institut de Ciències del Cosmos, Institut d’Estudis Espacials de Catalunya-Universitat de Barcelona, E-08028 Barcelona, Spain
| | - M. Persic
- Università di Udine and Istituto Nazionale di Fisica Nucleare (INFN) Trieste, I-33100 Udine, Italy, and Istituto Nazionale di Astrofisica (INAF)-Trieste, I-34127 Trieste, Italy
| | - J. Poutanen
- Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland
| | | | | | - I. Puljak
- Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia
| | - R. Reinthal
- Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland
| | - W. Rhode
- Technische Universität Dortmund, D-44221 Dortmund, Germany
| | - M. Ribó
- Universitat de Barcelona, Institut de Ciències del Cosmos, Institut d’Estudis Espacials de Catalunya-Universitat de Barcelona, E-08028 Barcelona, Spain
| | - J. Rico
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | | | - S. Rügamer
- Universität Würzburg, D-97074 Würzburg, Germany
| | - T. Saito
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - K. Saito
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | | | - V. Scalzotto
- Università di Padova and INFN, I-35131 Padova, Italy
| | - V. Scapin
- Universidad Complutense, E-28040 Madrid, Spain
| | - C. Schultz
- Università di Padova and INFN, I-35131 Padova, Italy
| | - T. Schweizer
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - S. N. Shore
- Università di Pisa and INFN Pisa, I-56126 Pisa, Italy
| | - A. Sillanpää
- Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland
| | - J. Sitarek
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
| | - I. Snidaric
- Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia
| | | | - F. Spanier
- Universität Würzburg, D-97074 Würzburg, Germany
| | - V. Stamatescu
- Institut de Física d’Altes Energies, Campus UAB, E-08193 Bellaterra, Spain
- Present address: School of Chemistry and Physics, University of Adelaide, Adelaide 5005, Australia
| | - A. Stamerra
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | | | - J. Storz
- Universität Würzburg, D-97074 Würzburg, Germany
| | - M. Strzys
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - L. Takalo
- Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland
| | - H. Takami
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - F. Tavecchio
- INAF National Institute for Astrophysics, I-00136 Rome, Italy
| | - P. Temnikov
- Institute for Nuclear Research and Nuclear Energy, BG-1784 Sofia, Bulgaria
| | - T. Terzić
- Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia
| | - D. Tescaro
- Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
| | - M. Teshima
- Max-Planck-Institut für Physik, D-80805 München, Germany
- Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan
| | - J. Thaele
- Technische Universität Dortmund, D-44221 Dortmund, Germany
| | - O. Tibolla
- Universität Würzburg, D-97074 Würzburg, Germany
| | - D. F. Torres
- ICREA and Institute of Space Sciences, E-08193 Barcelona, Spain
| | - T. Toyama
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - A. Treves
- Università dell’Insubria and INFN Milano Bicocca, Como, I-22100 Como, Italy
| | - M. Uellenbeck
- Technische Universität Dortmund, D-44221 Dortmund, Germany
| | - P. Vogler
- ETH Zurich, CH-8093 Zurich, Switzerland
| | - R. Zanin
- Universitat de Barcelona, Institut de Ciències del Cosmos, Institut d’Estudis Espacials de Catalunya-Universitat de Barcelona, E-08028 Barcelona, Spain
| | - M. Kadler
- Universität Würzburg, D-97074 Würzburg, Germany
| | - R. Schulz
- Universität Würzburg, D-97074 Würzburg, Germany
- Dr. Remeis-Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen-Nürnberg, ECAP, D-96049 Bamberg, Germany
| | - E. Ros
- Max-Planck-Institut für Radioastronomie, D-53121 Bonn, Germany
- Observatori Astronòmic, Universitat de València, E-46980 Paterna, València, Spain
- Departament d’Astronomia i Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - U. Bach
- Max-Planck-Institut für Radioastronomie, D-53121 Bonn, Germany
| | - F. Krauß
- Universität Würzburg, D-97074 Würzburg, Germany
- Dr. Remeis-Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen-Nürnberg, ECAP, D-96049 Bamberg, Germany
| | - J. Wilms
- Dr. Remeis-Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen-Nürnberg, ECAP, D-96049 Bamberg, Germany
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Escolano Serrano S, Ruiz Alcántara I, Alfonso Diego J, González Muñoz A, Gastaldo Simeón E. [Late-onset Group B Streptococcus disease in twins delivered by caesarean section]. An Pediatr (Barc) 2014; 82:e95-7. [PMID: 24588958 DOI: 10.1016/j.anpedi.2013.12.015] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/01/2013] [Revised: 12/16/2013] [Accepted: 12/20/2013] [Indexed: 10/25/2022] Open
Abstract
Group B Streptococcus (GBS) is a commensal pathogen of the gut microflora with a well-established role in the aetiology of early and late onset GBS infections in the newborn. The incidence of early onset infections by vertical transmission has been drastically reduced in recent decades with the use of intravenous intrapartum prophylaxis. Progress in risk factor detection and prophylaxis of late-onset infection has however remained static. The ongoing modifications and improvements of the guidelines regarding prophylaxis, risk factors and prevention of the early-onset GBS disease have not addressed late-onset GBS infection in detail. The following cases illustrate the presence of grey areas in current guidelines and in the knowledge of the pathogenesis of late-onset disease.
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Affiliation(s)
- S Escolano Serrano
- Departamento de Pediatría, Hospital Universitario la Ribera, Alcira, Valencia, España.
| | - I Ruiz Alcántara
- Departamento de Pediatría, Hospital Universitario la Ribera, Alcira, Valencia, España
| | - J Alfonso Diego
- Departamento de Pediatría, Hospital Universitario la Ribera, Alcira, Valencia, España
| | - A González Muñoz
- Departamento de Pediatría, Hospital Universitario la Ribera, Alcira, Valencia, España
| | - E Gastaldo Simeón
- Departamento de Pediatría, Hospital Universitario la Ribera, Alcira, Valencia, España
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6
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Abstract
The evolution of the surface roughness during the anodic dissolution of polycrystalline Ni was investigated by means of ex situ AFM in acid phosphate solutions. To characterize the time and spatial scaling behavior of surface roughness, the interface width and the power spectral density of the surface at different dissolution stages were analyzed in terms of dynamic scaling theories. The time dependence of global surface roughness, W(L,t), shows an unstable behavior characterized by a continuous increase without saturation following the relation W approximately t(beta), where beta > 0.5. The unstable behavior results from the development of wide grooves that originates a surface consisting of mounds. Two scaling regimes at scales shorter and larger than the mound dimensions (l(c)) were observed. For l < l(c), we found alpha approximately 1 consistent with mounds exhibiting smooth (faceted) walls, whereas an anomalous scaling behavior with a proper local roughness exponents (alpha(loc) < 1) dominates at l > l(c). The introduction of nitrite in the solution, a common additive used in phosphating baths, leads to some changes in the scaling behavior as a consequence of different generated chemical surface conditions during dissolution. The different dissolution rates of the exposed crystal orientations and surface diffusion of adatoms were identified as the physical processes that govern the interface dynamic for this system.
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Affiliation(s)
- A G Muñoz
- Institute of Thin Films and Interfaces (ISG 3), Research Centre Juelich, D-52425 Juelich, Germany.
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7
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Muñoz AG, Benitez G, Vela ME, Salvarezza RC. Influence of the adsorption of N species on the anodic dissolution of Ni. Langmuir 2004; 20:2361-2368. [PMID: 15835697 DOI: 10.1021/la0359225] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/24/2023]
Abstract
The dissolution and passivation of Ni in nitrite-containing acid solutions are investigated by Auger spectroscopy, atomic force microscopy, and conventional electrochemical techniques. The dissolution/ passivation of the Ni surface is consistent with a competition between adsorbed OH- and nitrogen-containing species with a potential-dependent surface coverage. Nitrogen-containing species hinder the passivation of the Ni surface, shifting the formation of the complex nickel hydroxide/oxide film to more positive potential values. The dynamics of the dissolving interface, followed by atomic force microscopy, reflect first the competition of adsorbed species, leading to the development of protrusions and cavities, and finally the formation of the passive film that promotes surface smoothening by a preferential dissolution of the protrusion tips under ohmic control.
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Affiliation(s)
- A G Muñoz
- Instituto de Ingeniería Electroquímica y Corrosión, Departamento de Ingeniería Química, Universidad Nacional del Sur, 8000 Bahia Blanca, Argentina.
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