1
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Albert A, Alfaro R, Alvarez C, Arteaga-Velázquez JC, Avila Rojas D, Ayala Solares HA, Babu R, Belmont-Moreno E, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Chaparro-Amaro O, Cotti U, Cotzomi J, Coutiño de León S, De la Fuente E, Diaz Hernandez R, Dingus BL, DuVernois MA, Durocher M, Díaz-Vélez JC, Ellsworth RW, Engel K, Espinoza C, Fan KL, Fang K, Fernández Alonso M, Fleischhack H, Fraija N, García-González JA, Garfias F, González MM, Goodman JA, Harding JP, Hernandez S, Hinton J, Huang D, Hueyotl-Zahuantitla F, Hüntemeyer P, Iriarte A, Joshi V, Kaufmann S, Lee J, Linnemann JT, Longinotti AL, Luis-Raya G, Malone K, Martinez O, Martínez-Castro J, Matthews JA, Miranda-Romagnoli P, Morales-Soto JA, Moreno E, Mostafá M, Nayerhoda A, Nellen L, Nisa MU, Noriega-Papaqui R, Olivera-Nieto L, Omodei N, Pérez Araujo Y, Pérez-Pérez EG, Rho CD, Rosa-González D, Ruiz-Velasco E, Salazar H, Salazar-Gallegos D, Sandoval A, Schneider M, Serna-Franco J, Smith AJ, Son Y, Springer RW, Tibolla O, Tollefson K, Torres I, Torres-Escobedo R, Turner R, Ureña-Mena F, Varela E, Villaseñor L, Wang X, Watson IJ, Willox E, Yun-Cárcamo S, Zhou H, de León C, Beacom JF, Linden T, Ng KCY, Peter AHG, Zhou B. Discovery of Gamma Rays from the Quiescent Sun with HAWC. Phys Rev Lett 2023; 131:051201. [PMID: 37595214 DOI: 10.1103/physrevlett.131.051201] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/06/2022] [Revised: 01/27/2023] [Accepted: 06/23/2023] [Indexed: 08/20/2023]
Abstract
We report the first detection of a TeV γ-ray flux from the solar disk (6.3σ), based on 6.1 years of data from the High Altitude Water Cherenkov (HAWC) observatory. The 0.5-2.6 TeV spectrum is well fit by a power law, dN/dE=A(E/1 TeV)^{-γ}, with A=(1.6±0.3)×10^{-12} TeV^{-1} cm^{-2} s^{-1} and γ=3.62±0.14. The flux shows a strong indication of anticorrelation with solar activity. These results extend the bright, hard GeV emission from the disk observed with Fermi-LAT, seemingly due to hadronic Galactic cosmic rays showering on nuclei in the solar atmosphere. However, current theoretical models are unable to explain the details of how solar magnetic fields shape these interactions. HAWC's TeV detection thus deepens the mysteries of the solar-disk emission.
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Affiliation(s)
- A Albert
- Physics Division, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
| | - R Alfaro
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - C Alvarez
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, México
| | | | - D Avila Rojas
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - H A Ayala Solares
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - R Babu
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - E Belmont-Moreno
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - C Brisbois
- Department of Physics, University of Maryland, College Park, MD, USA
| | | | - T Capistrán
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - S Casanova
- Instytut Fizyki Jadrowej im Henryka Niewodniczanskiego Polskiej Akademii Nauk, IFJ-PAN, Krakow, Poland
| | - O Chaparro-Amaro
- Centro de Investigaci'on en Computaci'on, Instituto Polit'ecnico Nacional, M'exico City, M'exico
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J Cotzomi
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - S Coutiño de León
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - E De la Fuente
- Departamento de F'isica, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
| | - R Diaz Hernandez
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - B L Dingus
- Physics Division, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
- Department of Physics, University of Maryland, College Park, MD, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - M Durocher
- Physics Division, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
| | - J C Díaz-Vélez
- Departamento de F'isica, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
| | - R W Ellsworth
- Department of Physics, University of Maryland, College Park, MD, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, MD, USA
| | - C Espinoza
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - K L Fan
- Department of Physics, University of Maryland, College Park, MD, USA
| | - K Fang
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - M Fernández Alonso
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - H Fleischhack
- Department of Physics, Catholic University of America, 620 Michigan Avenue NE, Washington, DC 20064
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Center for Research and Exploration in Space Science and Technology, NASA/GSFC, Greenbelt, MD 20771
| | - N Fraija
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J A García-González
- Tecnologico de Monterrey, Escuela de Ingeniería y Ciencias, Avenue Eugenio Garza Sada 2501, Monterrey, N.L., Mexico, 64849
| | - F Garfias
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - M M González
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, MD, USA
| | - J P Harding
- Physics Division, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
| | - S Hernandez
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J Hinton
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - D Huang
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | | | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A Iriarte
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - V Joshi
- Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen, Germany
| | - S Kaufmann
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - J Lee
- University of Seoul, Seoul, Rep. of Korea
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - A L Longinotti
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - G Luis-Raya
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - K Malone
- Space Science and Applications Group, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
| | - O Martinez
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - J Martínez-Castro
- Centro de Investigaci'on en Computaci'on, Instituto Polit'ecnico Nacional, M'exico City, M'exico
| | - J A Matthews
- Dept of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | | | - J A Morales-Soto
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - E Moreno
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - M Mostafá
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - A Nayerhoda
- Instytut Fizyki Jadrowej im Henryka Niewodniczanskiego Polskiej Akademii Nauk, IFJ-PAN, Krakow, Poland
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de Mexico, Ciudad de Mexico, Mexico
| | - M U Nisa
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | | | - L Olivera-Nieto
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - N Omodei
- Department of Physics, Stanford University: Stanford, CA 94305-4060, USA
| | - Y Pérez Araujo
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | | | - C D Rho
- Department of Physics, Sungkyunkwan University, Suwon 16419, South Korea
| | - D Rosa-González
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - E Ruiz-Velasco
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - H Salazar
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - D Salazar-Gallegos
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - A Sandoval
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - M Schneider
- Department of Physics, University of Maryland, College Park, MD, USA
| | - J Serna-Franco
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - A J Smith
- Department of Physics, University of Maryland, College Park, MD, USA
| | - Y Son
- University of Seoul, Seoul, Rep. of Korea
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - O Tibolla
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - I Torres
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - R Torres-Escobedo
- Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, People's Republic of China
| | - R Turner
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - F Ureña-Mena
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - E Varela
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - L Villaseñor
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - X Wang
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - I J Watson
- University of Seoul, Seoul, Rep. of Korea
| | - E Willox
- Department of Physics, University of Maryland, College Park, MD, USA
| | - S Yun-Cárcamo
- Department of Physics, University of Maryland, College Park, MD, USA
| | - H Zhou
- Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, People's Republic of China
| | - C de León
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J F Beacom
- Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, Ohio State University, Columbus, Ohio 43210, USA
- Department of Astronomy, Ohio State University, Columbus, Ohio 43210, USA
| | - T Linden
- The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, SE-10691 Stockholm, Sweden
| | - K C Y Ng
- Department of Physics, The Chinese University of Hong Kong, Sha Tin, Hong Kong, China
| | - A H G Peter
- Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, Ohio State University, Columbus, Ohio 43210, USA
- Department of Astronomy, Ohio State University, Columbus, Ohio 43210, USA
- School of Natural Sciences, Institute for Advanced Study, 1 Einstein Drive, Princeton, NJ 08540, USA
| | - B Zhou
- William H. Miller III Department of Physics and Astronomy, Johns Hopkins University, Baltimore, Maryland 21218, USA
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Scussel A, Marcondes-Braga F, Espinoza C, De Marchi D, Avila M, Duque A, de Paulo A, Mangini S, de Campos I, Seguro L, Gaiotto F, Bacal F. The Role of High-Sensitive Troponin in Identifying Patients with Cardiac Allograft Rejection. J Heart Lung Transplant 2023. [DOI: 10.1016/j.healun.2023.02.1223] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 04/05/2023] Open
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Rocío Yon, Macarena Sepúlveda Tapia, Rosario Carmona, Espinoza C. Mujeres mapuche en la ciudad. Trayectoria de vida y participación política en Santiago de Chile. rev colomb antropol 2022. [DOI: 10.22380/2539472x.2197] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022] Open
Abstract
El texto analiza la trayectoria política de diez mujeres mapuche en la ciudad de Santiago de Chile. Se basa en una investigación cualitativa cuyas principales técnicas metodológicas fueron la observación participante y la entrevista en profundidad. El texto se apoya en los enfoques de los feminismos decoloniales e indígenas para dar cuenta de las distintas tensiones que se expresan en las trayectorias políticas de estas mujeres, vinculadas a cuestiones como el género, la clase y su identidad mapuche urbana. El artículo revela que a pesar de que la participación política de las mujeres indígenas es heterogénea, se caracteriza por la conformación de redes y búsqueda de alternativas, tanto en espacios autónomos como institucionales.
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Olivares-Silva F, De Gregorio N, Espitia-Corredor J, Espinoza C, Vivar R, Silva D, Osorio JM, Lavandero S, Peiró C, Sánchez-Ferrer C, Díaz-Araya G. Resolvin-D1 attenuation of angiotensin II-induced cardiac inflammation in mice is associated with prevention of cardiac remodeling and hypertension. Biochim Biophys Acta Mol Basis Dis 2021; 1867:166241. [PMID: 34400298 DOI: 10.1016/j.bbadis.2021.166241] [Citation(s) in RCA: 12] [Impact Index Per Article: 4.0] [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: 06/13/2021] [Revised: 07/20/2021] [Accepted: 08/02/2021] [Indexed: 12/27/2022]
Abstract
AIMS Despite the broad pharmacological arsenal to treat hypertension, chronic patients may develop irreversible cardiac remodeling and fibrosis. Angiotensin II, the main peptide responsible for the Renin-Angiotensin-Aldosterone-System, has been closely linked to cardiac remodeling, hypertrophy, fibrosis, and hypertension, and some of these effects are induced by inflammatory mediators. Resolvin-D1 (RvD1) elicits potent anti-inflammatory and pro-resolving effects in various pathological models. In this study, we aimed to examine whether RvD1 ameliorates cardiac remodeling and hypertension triggered by angiotensin II. METHODS AND RESULTS Alzet® osmotic mini-pumps filled with angiotensin II (1.5 mg/kg/day) were implanted in male C57BL/6 J mice for 7 or 14 days. RvD1 (3 μg/kg/day, i.p) was administered one day after the surgery and during the complete infusion period. Blood pressure and myocardial functional parameters were assessed by echocardiography. At the end of the experimental procedure, blood and heart tissue were harvested, and plasma and histological parameters were studied. After 7 and 14 days, RvD1 reduced the increase of neutrophil and macrophage infiltration triggered by angiotensin II, and also reduced ICAM-1 and VCAM-1 expression levels. RvD1 also reduced cytokine plasma levels (IL-1β, TNF-α, IL-6, KC, MCP-1), cardiac hypertrophy, interstitial and perivascular fibrosis, and hypertension. CONCLUSIONS This study unveils novel cardioprotective effects of RvD1 in angiotensin II-induced hypertension and cardiac remodeling by attenuating inflammation and provides insights into a potential clinical application.
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Affiliation(s)
- Francisco Olivares-Silva
- Department of Chemical Pharmacology and Toxicology, Faculty of Chemical and Pharmaceutical Sciences, Universidad de Chile, Santiago, Chile; Advanced Center for Chronic Diseases (ACCDiS), Faculty of Chemical and Pharmaceutical Sciences and Faculty of Medicine, Universidad de Chile, Santiago, Chile
| | - Nicole De Gregorio
- Advanced Center for Chronic Diseases (ACCDiS), Faculty of Chemical and Pharmaceutical Sciences and Faculty of Medicine, Universidad de Chile, Santiago, Chile
| | - Jenaro Espitia-Corredor
- Department of Chemical Pharmacology and Toxicology, Faculty of Chemical and Pharmaceutical Sciences, Universidad de Chile, Santiago, Chile; Department of Pharmacology, Faculty of Medicine, Universidad Autónoma de Madrid and Instituto de Investigación Sanitaria Hospital Universitario La Paz (IdiPAZ), Spain
| | - Claudio Espinoza
- Department of Chemical Pharmacology and Toxicology, Faculty of Chemical and Pharmaceutical Sciences, Universidad de Chile, Santiago, Chile
| | - Raúl Vivar
- Pharmacology Program, Biomedical Sciences Institute, Faculty of Medicine, Universidad de Chile, Santiago, Chile
| | - David Silva
- Advanced Center for Chronic Diseases (ACCDiS), Faculty of Chemical and Pharmaceutical Sciences and Faculty of Medicine, Universidad de Chile, Santiago, Chile
| | - José Miguel Osorio
- Department of Chemical Pharmacology and Toxicology, Faculty of Chemical and Pharmaceutical Sciences, Universidad de Chile, Santiago, Chile
| | - Sergio Lavandero
- Advanced Center for Chronic Diseases (ACCDiS), Faculty of Chemical and Pharmaceutical Sciences and Faculty of Medicine, Universidad de Chile, Santiago, Chile; Cardiology Division, Department of Internal Medicine, University of Texas Southwestern Medical Center, Dallas, TX, USA
| | - Concepción Peiró
- Department of Pharmacology, Faculty of Medicine, Universidad Autónoma de Madrid and Instituto de Investigación Sanitaria Hospital Universitario La Paz (IdiPAZ), Spain
| | - Carlos Sánchez-Ferrer
- Department of Pharmacology, Faculty of Medicine, Universidad Autónoma de Madrid and Instituto de Investigación Sanitaria Hospital Universitario La Paz (IdiPAZ), Spain
| | - Guillermo Díaz-Araya
- Department of Chemical Pharmacology and Toxicology, Faculty of Chemical and Pharmaceutical Sciences, Universidad de Chile, Santiago, Chile; Advanced Center for Chronic Diseases (ACCDiS), Faculty of Chemical and Pharmaceutical Sciences and Faculty of Medicine, Universidad de Chile, Santiago, Chile.
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5
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Albert A, Alfaro R, Alvarez C, Angeles Camacho JR, Arteaga-Velázquez JC, Arunbabu KP, Avila Rojas D, Ayala Solares HA, Baghmanyan V, Belmont-Moreno E, BenZvi SY, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Cotti U, Cotzomi J, Coutiño de León S, De la Fuente E, de León C, Dingus BL, DuVernois MA, Díaz-Vélez JC, Ellsworth RW, Engel K, Espinoza C, Fleischhack H, Fraija N, Galván-Gámez A, Garcia D, García-González JA, Garfias F, González MM, Goodman JA, Harding JP, Hernandez S, Hona B, Huang D, Hueyotl-Zahuantitla F, Hüntemeyer P, Iriarte A, Joshi V, Lara A, Lee WH, León Vargas H, Linnemann JT, Longinotti AL, Luis-Raya G, Lundeen J, López-Coto R, Malone K, Marinelli SS, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews JA, Miranda-Romagnoli P, Morales-Soto JA, Moreno E, Nayerhoda A, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Omodei N, Peisker A, Pérez-Pérez EG, 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, Tabachnick E, Tanner M, Tibolla O, Tollefson K, Torres I, Torres-Escobedo R, Weisgarber T, Yodh G, Zepeda A, Zhou H. Constraints on Lorentz Invariance Violation from HAWC Observations of Gamma Rays above 100 TeV. Phys Rev Lett 2020; 124:131101. [PMID: 32302173 DOI: 10.1103/physrevlett.124.131101] [Citation(s) in RCA: 9] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/18/2019] [Revised: 02/07/2020] [Accepted: 03/04/2020] [Indexed: 06/11/2023]
Abstract
Because of the high energies and long distances to the sources, astrophysical observations provide a unique opportunity to test possible signatures of Lorentz invariance violation (LIV). Superluminal LIV enables the decay of photons at high energy. The high altitude water Cherenkov (HAWC) observatory is among the most sensitive gamma-ray instruments currently operating above 10 TeV. HAWC finds evidence of 100 TeV photon emission from at least four astrophysical sources. These observations exclude, for the strongest of the limits set, the LIV energy scale to 2.2×10^{31} eV, over 1800 times the Planck energy and an improvement of 1 to 2 orders of magnitude over previous limits.
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Affiliation(s)
- A Albert
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - R Alfaro
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - C Alvarez
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas 29050, Mexico
| | - J R Angeles Camacho
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | | | - K P Arunbabu
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - H A Ayala Solares
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - V Baghmanyan
- Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 IFJ-PAN, Krakow 31342, Poland
| | - E Belmont-Moreno
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - S Y BenZvi
- Department of Physics & Astronomy, University of Rochester, Rochester, New York 14627, USA
| | - C Brisbois
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | - K S Caballero-Mora
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas 29050, Mexico
| | - T Capistrán
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - S Casanova
- Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 IFJ-PAN, Krakow 31342, Poland
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia 58040, Mexico
| | - J Cotzomi
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla 72570, Mexico
| | - S Coutiño de León
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - E De la Fuente
- Departamento de Física, CUCEI, Universidad de Guadalajara, Guadalajara 44430, Mexico
| | - C de León
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia 58040, Mexico
| | - B L Dingus
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de los Valles, Universidad de Guadalajara, Guadalajara 46600, Mexico
| | - R W Ellsworth
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - C Espinoza
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - H Fleischhack
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - A Galván-Gámez
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - D Garcia
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - J A García-González
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - F Garfias
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - M M González
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - J P Harding
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - S Hernandez
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - B Hona
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | - D Huang
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | | | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | - A Iriarte
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - V Joshi
- Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, 91058 Erlangen, Germany
| | - A Lara
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - W H Lee
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | - A L Longinotti
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - G Luis-Raya
- Universidad Politecnica de Pachuca, Pachuca, Hgo 42083, Mexico
| | - J Lundeen
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | - R López-Coto
- INFN and Universita di Padova, via Marzolo 8, I-35131, Padova, Italy
| | - K Malone
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - S S Marinelli
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | | | - J Martínez-Castro
- Centro de Investigación en Computación, Instituto Politécnico Nacional, México City 07738, Mexico
| | - H Martínez-Huerta
- Instituto de Física de São Carlos, Universidade de São Paulo, São Carlos, Sao Paolo 13566-590, Brasil
| | - J A Matthews
- Dept of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico 87131, USA
| | | | - J A Morales-Soto
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia 58040, Mexico
| | - E Moreno
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla 72570, Mexico
| | - A Nayerhoda
- Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 IFJ-PAN, Krakow 31342, Poland
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de Mexico, Ciudad de Mexico 04510, Mexico
| | - M Newbold
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
| | - M U Nisa
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | | | - N Omodei
- Stanford University, Stanford, California 94305, USA
| | - A Peisker
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | - E G Pérez-Pérez
- Universidad Politecnica de Pachuca, Pachuca, Hgo 42083, Mexico
| | - C D Rho
- Department of Physics & Astronomy, University of Rochester, Rochester, New York 14627, USA
| | - C Rivière
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - D Rosa-González
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - M Rosenberg
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - E Ruiz-Velasco
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - H Salazar
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla 72570, Mexico
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 IFJ-PAN, Krakow 31342, Poland
| | - A Sandoval
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - M Schneider
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - H Schoorlemmer
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - G Sinnis
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - A J Smith
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
| | - P Surajbali
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - E Tabachnick
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - M Tanner
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - O Tibolla
- Universidad Politecnica de Pachuca, Pachuca, Hgo 42083, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | - I Torres
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - R Torres-Escobedo
- Departamento de Física, CUCEI, Universidad de Guadalajara, Guadalajara 44430, Mexico
- Department of Physics and Astronomy, Texas Tech University, Lubbock, Texas 79409-1051, USA
| | - T Weisgarber
- Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA
| | - G Yodh
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697, USA
| | - A Zepeda
- Physics Department, Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City 07360, Mexico
| | - H Zhou
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
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6
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Abeysekara AU, Albert A, Alfaro R, Angeles Camacho JR, Arteaga-Velázquez JC, Arunbabu KP, Avila Rojas D, Ayala Solares HA, Baghmanyan V, Belmont-Moreno E, BenZvi SY, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Cotti U, Cotzomi J, Coutiño de León S, De la Fuente E, de León C, Dichiara S, Dingus BL, DuVernois MA, Díaz-Vélez JC, Ellsworth RW, Engel K, Espinoza C, Fleischhack H, Fraija N, Galván-Gámez A, Garcia D, García-González JA, Garfias F, González MM, Goodman JA, Harding JP, Hernandez S, Hinton J, Hona B, Huang D, Hueyotl-Zahuantitla F, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Kieda D, Lara A, Lee WH, León Vargas H, Linnemann JT, Longinotti AL, Luis-Raya G, Lundeen J, López-Coto R, Malone K, Marinelli SS, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews JA, Miranda-Romagnoli P, Morales-Soto JA, Moreno E, Mostafá M, Nayerhoda A, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Peisker A, Pérez-Pérez EG, Pretz J, Ren Z, Rho CD, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Sinnis G, Smith AJ, Springer RW, Surajbali P, Tabachnick E, Tanner M, Tibolla O, Tollefson K, Torres I, Torres-Escobedo R, Villaseñor L, Weisgarber T, Wood J, Yapici T, Zhang H, Zhou H. Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC. Phys Rev Lett 2020; 124:021102. [PMID: 32004015 DOI: 10.1103/physrevlett.124.021102] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/18/2019] [Revised: 11/21/2019] [Indexed: 06/10/2023]
Abstract
We present the first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov Observatory, a wide field-of-view observatory capable of detecting gamma rays up to a few hundred TeV. Nine sources are observed above 56 TeV, all of which are likely galactic in origin. Three sources continue emitting past 100 TeV, making this the highest-energy gamma-ray source catalog to date. We report the integral flux of each of these objects. We also report spectra for three highest-energy sources and discuss the possibility that they are PeVatrons.
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Affiliation(s)
- A U Abeysekara
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA
| | - A Albert
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
| | - R Alfaro
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J R Angeles Camacho
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | | | - K P Arunbabu
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - H A Ayala Solares
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - V Baghmanyan
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - E Belmont-Moreno
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - S Y BenZvi
- Department of Physics & Astronomy, University of Rochester, Rochester, New York, USA
| | - C Brisbois
- Department of Physics, University of Maryland, College Park, Maryland, 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, IFJ-PAN, Krakow, Poland
| | - 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
| | - E De la Fuente
- Departamento de Física, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
- Department of Physics and Astronomy, Texas Tech University, Lubbock, Texas, USA
| | - C de León
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - S Dichiara
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - B L Dingus
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin, USA
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
- Department of Physics and Astronomy, Texas Tech University, Lubbock, Texas, USA
| | - R W Ellsworth
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - C Espinoza
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - H Fleischhack
- Department of Physics, Michigan Technological University, Houghton, Michigan, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - A Galván-Gámez
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - D Garcia
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J A García-González
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - F Garfias
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - M M González
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - J P Harding
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
| | - S Hernandez
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J Hinton
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - B Hona
- Department of Physics, Michigan Technological University, Houghton, Michigan, USA
| | - D Huang
- Department of Physics, Michigan Technological University, Houghton, Michigan, USA
| | | | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, Michigan, USA
| | - A Iriarte
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - A Jardin-Blicq
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - V Joshi
- Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen, Germany
| | - S Kaufmann
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - D Kieda
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA
| | - A Lara
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - W H Lee
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | - A L Longinotti
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - G Luis-Raya
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - J Lundeen
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | - R López-Coto
- INFN and Universita di Padova, via Marzolo 8, Padova, Italy
| | - K Malone
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - S S Marinelli
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, 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, México City, México
| | - H Martínez-Huerta
- Instituto de Física de São Carlos, Universidade de São Paulo, São Carlos, São Paulo, Brasil
| | - J A Matthews
- Dept of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico, USA
| | | | - J A Morales-Soto
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - E Moreno
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - M Mostafá
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - A Nayerhoda
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de Mexico, Ciudad de Mexico, Mexico
| | - M Newbold
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA
| | - M U Nisa
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | | | - A Peisker
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | | | - J Pretz
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - Z Ren
- Dept of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico, USA
| | - C D Rho
- Department of Physics & Astronomy, University of Rochester, Rochester, New York, USA
| | - C Rivière
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - D Rosa-González
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - M Rosenberg
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - E Ruiz-Velasco
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - A Sandoval
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - M Schneider
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - H Schoorlemmer
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - G Sinnis
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
| | - A J Smith
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA
| | - P Surajbali
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - E Tabachnick
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - M Tanner
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - O Tibolla
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | - I Torres
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - R Torres-Escobedo
- Departamento de Física, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
- Department of Physics and Astronomy, Texas Tech University, Lubbock, Texas, USA
| | - L Villaseñor
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - T Weisgarber
- Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin, USA
| | - J Wood
- NASA Marshall Space Flight Center, Hunstville, Alabama, USA
| | - T Yapici
- Department of Physics & Astronomy, University of Rochester, Rochester, New York, USA
| | - H Zhang
- Department of Physics and Astronomy, Purdue University, West Lafayette, Indiana, USA
| | - H Zhou
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
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7
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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, Belmont-Moreno E, BenZvi SY, 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, Díaz-Vélez JC, Dichiara S, Dingus BL, DuVernois MA, Ellsworth RW, Engel K, Espinoza C, Fang K, Fleischhack H, Fraija N, Galván-Gámez A, García-González JA, Garfias F, González-Muñoz A, González MM, Goodman JA, Hampel-Arias Z, Harding JP, Hernandez S, Hinton J, Hona B, Hueyotl-Zahuantitla F, Hui CM, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Kar P, Kunde GJ, Lauer RJ, Lee WH, León Vargas H, Li H, Linnemann JT, Longinotti AL, Luis-Raya G, López-Coto R, Malone K, Marinelli SS, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Matthews JA, Miranda-Romagnoli P, Moreno E, Mostafá M, Nayerhoda A, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Pretz J, Pérez-Pérez EG, Ren Z, Rho CD, 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 AJ, Springer RW, Surajbali P, Taboada I, Tibolla O, Tollefson K, Torres I, Vianello G, Villaseñor L, Weisgarber T, Werner F, Westerhoff S, Wood J, Yapici T, Yodh G, Zepeda A, Zhang H, Zhou H. Publisher Correction: Very-high-energy particle acceleration powered by the jets of the microquasar SS 433. Nature 2018; 564:E38. [PMID: 30482938 DOI: 10.1038/s41586-018-0688-8] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Abstract
In this Letter, owing to a production error, the penultimate version of the PDF was published. The HTML version was always correct. The PDF has been corrected online.
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Affiliation(s)
- A U Abeysekara
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - A Albert
- Physics and Theoretical Divisions, 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, Mexico
| | - J D Álvarez
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - R Arceo
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico
| | | | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H A Ayala Solares
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - 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
| | - 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, IFJ-PAN, 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
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico.,Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - S Dichiara
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - B L Dingus
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - M A DuVernois
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - 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
| | - C Espinoza
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - K Fang
- Department of Astronomy, University of Maryland, College Park, MD, USA.,Joint Space-Science Institute, University of Maryland, College Park, MD, USA
| | - H Fleischhack
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Galván-Gámez
- 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
| | - A González-Muñoz
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, 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 and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA.,Inter-university Institute for High Energies, Université Libre de Bruxelles, Brussels, Belgium
| | - J P Harding
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - S Hernandez
- 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
- NASA Marshall Space Flight Center, Astrophysics Office, 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, Mexico
| | - P Kar
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - G J Kunde
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - 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
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H Li
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - 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, Mexico
| | | | - 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
| | - 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
| | - A Nayerhoda
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de Mexico, 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
| | | | - J Pretz
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | | | - 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
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, 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
| | - M Seglar Arroyo
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - G Sinnis
- Physics and Theoretical Divisions, 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, 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
| | - G Vianello
- Department of Physics, Stanford University, Stanford, CA, USA
| | - L Villaseñor
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - T Weisgarber
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - F Werner
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - S Westerhoff
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - J Wood
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - T Yapici
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - G Yodh
- Department of Physics and Astronomy, University of California, Irvine, Irvine, CA, USA
| | - A Zepeda
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico.,Physics Department, Centro de Investigación y de Estudios Avanzados del IPN, Mexico City, Mexico
| | - H Zhang
- Department of Physics and Astronomy, Purdue University, West Lafayette, IN, USA
| | - H Zhou
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA.
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Galban S, Van Dort M, Hao H, Espinoza C, Heist K, Nino C, Galban C, Besirli C, Ross B. Development and evaluation of a novel MAPK and PI3K inhibitor. Eur J Cancer 2016. [DOI: 10.1016/s0959-8049(16)32681-8] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022]
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Beltran P, Espinoza C, Hernandez C, Chavez D, Reyna W, Cruz G, Perez Campos E. Ascariasis as cause of intestinal occlusion and concurrent appendicitis. Trop Biomed 2016; 33:833-836. [PMID: 33579082] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 06/12/2023]
Abstract
Intestinal occlusion by ascariasis is a commonly seen socio-economic status low, is associated with poor sanitary hygiene. It is rare to see a case with both intestinal occlusion and appendicitis at the same time, as described in this report.
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Affiliation(s)
| | - C Espinoza
- Department of Anesthesiology IMSS HRO-24
| | | | - D Chavez
- Rural Anesthesiology IMSS HRO-24
| | - W Reyna
- Rural Hospital of Opportunities number 24 Mexican Institute of Social Security (IMSS HRO 24)
- Faculty of Medicine and Surgery Autonomous University Benito Juarez of Oaxaca (UABJO)
| | - G Cruz
- Faculty of Medicine and Surgery Autonomous University Benito Juarez of Oaxaca (UABJO)
| | - E Perez Campos
- Faculty of Medicine and Surgery Autonomous University Benito Juarez of Oaxaca (UABJO)
- Immunology and Biochemistry Unit ITO-UNAM
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Espinoza C, Schlechter R, Herrera D, Torres E, Serrano A, Medina C, Arce-Johnson P. Cisgenesis and intragenesis: new tools for improving crops. Biol Res 2016; 46:323-31. [PMID: 24510134 DOI: 10.4067/s0716-97602013000400003] [Citation(s) in RCA: 47] [Impact Index Per Article: 5.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/28/2013] [Accepted: 11/11/2013] [Indexed: 11/17/2022] Open
Abstract
Genetically Modified Organisms (GMO) could be the answer for many relevant problems affecting crops. However, improving crops through GMO is also often associated with safety concerns, environmental risks and health issues due to the presence of foreign DNA. These limitations have prompted the development of alternative technologies. Recently, cisgenesis and intragenesis have been developed as new tools aimed to modify crops. While cisgenesis involves genetic modification using a complete copy of natural genes with their regulatory elements that belong exclusively to sexually compatible plants, intragenesis refers to the transference of new combinations of genes and regulatory sequences belonging to that particular species. So far, application of cisgenesis and intragenesis as alternatives to conventional transgenesis are limited to a few species, mainly due to the lack of knowledge of the regulatory sequences required. The grape is one of the most cultivated crops worldwide and is the most economically relevant crop in Chile. Its genomic sequence has been completed, making available new sources of information to improve grape traits by genetic manipulation. This review is focused on the current alternatives to transgenesis in plants, including new approaches to develop marker-free crops, their application to economically relevant crops and future perspectives in the area. Also, the identification of grapevine promoters with a wide range of expression profiles is shown. The expression pattern of these genes was analyzed in different tissues and developmental stages, as well as under several stresses and stimuli, giving a broad range of expression patterns, including genes expressed exclusively during ripening, in response to sugars, senescence and biotic stress, among others. Genes with strong and constitutive expression were also identified. Functional analysis using reporter genes has been conducted in order to confirm the promoter's transcription activity, opening new possibilities for developing cisgenic/intragenic grapevines.
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Moreno J, Espinoza C, Simpson R, Petzold G, Nuñez H, Gianelli M. Application of ohmic heating/vacuum impregnation treatments and air drying to develop an apple snack enriched in folic acid. INNOV FOOD SCI EMERG 2016. [DOI: 10.1016/j.ifset.2015.12.014] [Citation(s) in RCA: 23] [Impact Index Per Article: 2.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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Beckord B, Berkowitz R, Espinoza C, Anand N. Systemic thrombolysis: cure for prosthetic mitral valve thrombosis in the comorbid, non-surgical candidate. Case Reports 2014; 2014:bcr-2013-203071. [DOI: 10.1136/bcr-2013-203071] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/04/2022] Open
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Espinoza C, Lomax S, Windsor P. The effect of a topical anesthetic on the sensitivity of calf dehorning wounds. J Dairy Sci 2013; 96:2894-902. [PMID: 23477817 DOI: 10.3168/jds.2012-5954] [Citation(s) in RCA: 30] [Impact Index Per Article: 2.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/17/2012] [Accepted: 01/09/2013] [Indexed: 11/19/2022]
Abstract
The objective was to determine the effect of a topical local anesthetic on the sensitivity of dehorning wounds in calves. Thirty 2-mo-old Holstein-Friesian calves were randomly allocated to sham dehorning control (CON), scoop dehorning without treatment with topical anesthetic (SnoTA), or scoop dehorning with an application of a topical anesthetic (STA). Sensitivity was measured by providing mechanical stimulation to the dehorned wound and peri-wound area using von Frey monofilaments calibrated at 10 and 300 g. Calf responses were categorized as absent, minor, moderate, or severe. Sensitivity measurements were performed before treatment and at various time points up to 24h posttreatment. Sham dehorned calves displayed unchanging absent or minor responses to stimulation. Regardless of whether topical anesthetic was applied, scoop dehorned calves were more likely to display minor, moderate, or severe responses than sham dehorned control calves, and responses tended to be most extreme at 4h postdehorning. Calves in the STA group tended to be less likely to display minor, moderate, or severe responses than calves in the SnoTA group at most time points (exception at 4h postdehorning). Responses were significantly more likely to be less severe in STA calves than in SnoTA calves at 40 min and 1.5h following dehorning. Thus, the use of the topical anesthetic for calves reduced the short-term sensitivity of scoop dehorning wounds.
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Affiliation(s)
- C Espinoza
- The University of Sydney, Private Bag 4003 Narellan, New South Wales 2567, Australia
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Diaz V, Silva C, Antinao J, Espinoza C, Henriquez S, Parra C. Epidemiology of Creutzfeldt-Jacob in Chile. Morbility and Mortality (P03.260). Neurology 2012. [DOI: 10.1212/wnl.78.1_meetingabstracts.p03.260] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022] Open
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Merrill FE, Campos E, Espinoza C, Hogan G, Hollander B, Lopez J, Mariam FG, Morley D, Morris CL, Murray M, Saunders A, Schwartz C, Thompson TN. Magnifying lens for 800 MeV proton radiography. Rev Sci Instrum 2011; 82:103709. [PMID: 22047305 DOI: 10.1063/1.3652974] [Citation(s) in RCA: 3] [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: 05/31/2023]
Abstract
This article describes the design and performance of a magnifying magnetic-lens system designed, built, and commissioned at the Los Alamos National Laboratory (LANL) for 800 MeV flash proton radiography. The technique of flash proton radiography has been developed at LANL to study material properties under dynamic loading conditions through the analysis of time sequences of proton radiographs. The requirements of this growing experimental program have resulted in the need for improvements in spatial radiographic resolution. To meet these needs, a new magnetic lens system, consisting of four permanent magnet quadrupoles, has been developed. This new lens system was designed to reduce the second order chromatic aberrations, the dominant source of image blur in 800 MeV proton radiography, as well as magnifying the image to reduce the blur contribution from the detector and camera systems. The recently commissioned lens system performed as designed, providing nearly a factor of three improvement in radiographic resolution.
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Affiliation(s)
- F E Merrill
- Los Alamos National Laboratory, Los Alamos, New Mexico 87544, USA.
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Abdo AA, Ackermann M, Ajello M, Baldini L, Ballet J, Barbiellini G, Baring MG, Bastieri D, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cecchi C, Çelik Ö, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cognard I, Cohen-Tanugi J, Cominsky LR, Conrad J, Cutini S, Dermer CD, de Angelis A, de Palma F, Digel SW, do Couto e Silva E, Drell PS, Dubois R, Dumora D, Espinoza C, Farnier C, Favuzzi C, Fegan SJ, Focke WB, Fortin P, Frailis M, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giavitto G, Giebels B, Giglietto N, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Hanabata Y, Harding AK, Hayashida M, Hays E, Hughes RE, Jackson MS, Jóhannesson G, Johnson AS, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kataoka J, Katsuta J, Kawai N, Kerr M, Knödlseder J, Kocian ML, Kramer M, Kuss M, Lande J, Latronico L, Lemoine-Goumard M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Lyne AG, Madejski GM, Makeev A, Mazziotta MN, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Nolan PL, Norris JP, Noutsos A, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Paneque D, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piron F, Porter TA, Rainò S, Rando R, Razzano M, Reimer A, Reimer O, Reposeur T, Rochester LS, Rodriguez AY, Romani RW, Roth M, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Parkinson PMS, Scargle JD, Sgrò C, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Stappers BW, Stecker FW, Strickman MS, Suson DJ, Tajima H, Takahashi H, Takahashi T, Tanaka T, Thayer JB, Thayer JG, Theureau G, Thompson DJ, Tibaldo L, Tibolla O, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Vasileiou V, Venter C, Vilchez N, Vitale V, Waite AP, Wang P, Winer BL, Wood KS, Yamazaki R, Ylinen T, Ziegler M. Gamma-Ray Emission from the Shell of Supernova Remnant W44 Revealed by the Fermi LAT. Science 2010; 327:1103-6. [PMID: 20056857 DOI: 10.1126/science.1182787] [Citation(s) in RCA: 206] [Impact Index Per Article: 14.7] [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)
- A. A. Abdo
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - M. Ackermann
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Ajello
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - L. Baldini
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - J. Ballet
- Laboratoire Astrophysique Instrumentation Modélisation, Commissariat à l’Énergie Atomique (CEA)–Institut de Recherche sur les Lois Fondamentales de l’Univers (IRFU)/CNRS/Université Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - G. Barbiellini
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I–34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I–34127 Trieste, Italy
| | - M. G. Baring
- Rice University, Department of Physics and Astronomy, MS–108, Post Office Box 1892, Houston, TX 77251, USA
| | - D. Bastieri
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I–35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I–35131 Padova, Italy
| | - B. M. Baughman
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - K. Bechtol
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. Bellazzini
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - B. Berenji
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. D. Blandford
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. D. Bloom
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. Bonamente
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - A. W. Borgland
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. Bregeon
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - A. Brez
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - M. Brigida
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - P. Bruel
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - T. H. Burnett
- Department of Physics, University of Washington, Seattle, WA 98195–1560, USA
| | - S. Buson
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I–35131 Padova, Italy
| | - G. A. Caliandro
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - R. A. Cameron
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. A. Caraveo
- Istituto di Astrofisica Spaziale e Fisica Cosmica, Istituto Nazionale di Astrofisica (INAF), I–20133 Milano, Italy
| | - J. M. Casandjian
- Laboratoire Astrophysique Instrumentation Modélisation, Commissariat à l’Énergie Atomique (CEA)–Institut de Recherche sur les Lois Fondamentales de l’Univers (IRFU)/CNRS/Université Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - C. Cecchi
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - Ö. Çelik
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Center for Research and Exploration in Space Science and Technology (CRESST), NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- University of Maryland, Baltimore County, Baltimore, MD 21250, USA
| | - A. Chekhtman
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
- George Mason University, Fairfax, VA 22030, USA
| | - C. C. Cheung
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - J. Chiang
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Ciprini
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - R. Claus
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - I. Cognard
- Laboratoire de Physique et Chemie de l'Environnement (LPCE), LPCE UMR 6115 CNRS, F–45071 Orléans Cedex 02, France, and Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/Institut National des Sciences de l’Univers (INSU), F–18330 Nançay, France
| | - J. Cohen-Tanugi
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - L. R. Cominsky
- Department of Physics and Astronomy, Sonoma State University, Rohnert Park, CA 94928–3609, USA
| | - J. Conrad
- Department of Physics, Stockholm University, AlbaNova, SE–106 91 Stockholm, Sweden
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE–106 91 Stockholm, Sweden
| | - S. Cutini
- Agenzia Spaziale Italiana (ASI) Science Data Center, I–00044 Frascati (Roma), Italy
| | - C. D. Dermer
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - A. de Angelis
- Dipartimento di Fisica, Università di Udine and Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Gruppo Collegato di Udine, I–33100 Udine, Italy
| | - F. de Palma
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - S. W. Digel
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. do Couto e Silva
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. S. Drell
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. Dubois
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - D. Dumora
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - C. Espinoza
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
| | - C. Farnier
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - C. Favuzzi
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - S. J. Fegan
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - W. B. Focke
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Fortin
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - M. Frailis
- Dipartimento di Fisica, Università di Udine and Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Gruppo Collegato di Udine, I–33100 Udine, Italy
| | - Y. Fukazawa
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - S. Funk
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Fusco
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - F. Gargano
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - D. Gasparrini
- Agenzia Spaziale Italiana (ASI) Science Data Center, I–00044 Frascati (Roma), Italy
| | - N. Gehrels
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- University of Maryland, College Park, MD 20742, USA
| | - S. Germani
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - G. Giavitto
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, and Università di Trieste, I–34127 Trieste, Italy
| | - B. Giebels
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - N. Giglietto
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - F. Giordano
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - T. Glanzman
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - G. Godfrey
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - I. A. Grenier
- Laboratoire Astrophysique Instrumentation Modélisation, Commissariat à l’Énergie Atomique (CEA)–Institut de Recherche sur les Lois Fondamentales de l’Univers (IRFU)/CNRS/Université Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - M.-H. Grondin
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - J. E. Grove
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - L. Guillemot
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - S. Guiriec
- University of Alabama in Huntsville, Huntsville, AL 35899, USA
| | - Y. Hanabata
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - A. K. Harding
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - M. Hayashida
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. Hays
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - R. E. Hughes
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - M. S. Jackson
- Department of Physics, Stockholm University, AlbaNova, SE–106 91 Stockholm, Sweden
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE–106 91 Stockholm, Sweden
- Department of Physics, Royal Institute of Technology (KTH), AlbaNova, SE–106 91 Stockholm, Sweden
| | - G. Jóhannesson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. S. Johnson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. J. Johnson
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- University of Maryland, College Park, MD 20742, USA
| | - W. N. Johnson
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - T. Kamae
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - H. Katagiri
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - J. Kataoka
- Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152–8551, Japan
- Waseda University, 1-104 Totsukamachi, Shinjuku-ku, Tokyo 169–8050, Japan
| | - J. Katsuta
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229–8510, Japan
- Department of Physics, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113–0033, Japan
| | - N. Kawai
- Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152–8551, Japan
- Cosmic Radiation Laboratory, Institute of Physical and Chemical Research (RIKEN), Wako, Saitama 351–0198, Japan
| | - M. Kerr
- Department of Physics, University of Washington, Seattle, WA 98195–1560, USA
| | - J. Knödlseder
- Centre d'Étude Spatiale des Rayonnements, CNRS/Université Paul Sabatier (UPS), BP 44346, F–30128 Toulouse Cedex 4, France
| | - M. L. Kocian
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Kramer
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
- Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
| | - M. Kuss
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - J. Lande
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - L. Latronico
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - M. Lemoine-Goumard
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - F. Longo
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I–34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I–34127 Trieste, Italy
| | - F. Loparco
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - B. Lott
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - M. N. Lovellette
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - P. Lubrano
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - A. G. Lyne
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
| | - G. M. Madejski
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Makeev
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
- George Mason University, Fairfax, VA 22030, USA
| | - M. N. Mazziotta
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - J. E. McEnery
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - C. Meurer
- Department of Physics and Astronomy, Sonoma State University, Rohnert Park, CA 94928–3609, USA
- Department of Physics, Stockholm University, AlbaNova, SE–106 91 Stockholm, Sweden
| | - P. F. Michelson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - W. Mitthumsiri
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. Mizuno
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - C. Monte
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - M. E. Monzani
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Morselli
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma “Tor Vergata,” I–00133 Roma, Italy
| | - I. V. Moskalenko
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Murgia
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. Nakamori
- Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152–8551, Japan
| | - P. L. Nolan
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. P. Norris
- Department of Physics and Astronomy, University of Denver, Denver, CO 80208, USA
| | - A. Noutsos
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
| | - E. Nuss
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - T. Ohsugi
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - N. Omodei
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - E. Orlando
- Max-Planck Institut für Extraterrestrische Physik, 85748 Garching, Germany
| | - J. F. Ormes
- Department of Physics and Astronomy, University of Denver, Denver, CO 80208, USA
| | - D. Paneque
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - D. Parent
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - V. Pelassa
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - M. Pepe
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - M. Pesce-Rollins
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - F. Piron
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - T. A. Porter
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - S. Rainò
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - R. Rando
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I–35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I–35131 Padova, Italy
| | - M. Razzano
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - A. Reimer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A–6020 Innsbruck, Austria
| | - O. Reimer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A–6020 Innsbruck, Austria
| | - T. Reposeur
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - L. S. Rochester
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Y. Rodriguez
- Institut de Ciencies de l'Espai (IEEC-CSIC), Campus UAB, 08193 Barcelona, Spain
| | - R. W. Romani
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Roth
- Department of Physics, University of Washington, Seattle, WA 98195–1560, USA
| | - F. Ryde
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE–106 91 Stockholm, Sweden
- Department of Physics, Royal Institute of Technology (KTH), AlbaNova, SE–106 91 Stockholm, Sweden
| | - H. F.-W. Sadrozinski
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - D. Sanchez
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - A. Sander
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - P. M. Saz Parkinson
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - J. D. Scargle
- Space Sciences Division, NASA Ames Research Center, Moffett Field, CA 94035–1000, USA
| | - C. Sgrò
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - E. J. Siskind
- NYCB Real-Time Computing Incorporated, Lattingtown, NY 11560–1025, USA
| | - D. A. Smith
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - P. D. Smith
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - G. Spandre
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - P. Spinelli
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - B. W. Stappers
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
| | - F. W. Stecker
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - M. S. Strickman
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - D. J. Suson
- Department of Chemistry and Physics, Purdue University Calumet, Hammond, IN 46323–2094, USA
| | - H. Tajima
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - H. Takahashi
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - T. Takahashi
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229–8510, Japan
| | - T. Tanaka
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. B. Thayer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. G. Thayer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - G. Theureau
- Laboratoire de Physique et Chemie de l'Environnement (LPCE), LPCE UMR 6115 CNRS, F–45071 Orléans Cedex 02, France, and Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/Institut National des Sciences de l’Univers (INSU), F–18330 Nançay, France
| | - D. J. Thompson
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - L. Tibaldo
- Laboratoire Astrophysique Instrumentation Modélisation, Commissariat à l’Énergie Atomique (CEA)–Institut de Recherche sur les Lois Fondamentales de l’Univers (IRFU)/CNRS/Université Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I–35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I–35131 Padova, Italy
| | - O. Tibolla
- Max-Planck-Institut für Kernphysik, D–69029 Heidelberg, Germany
| | - D. F. Torres
- Institut de Ciencies de l'Espai (IEEC-CSIC), Campus UAB, 08193 Barcelona, Spain
- Institució Catalana de Recerca i Estudis Avançats (ICREA), 08010 Barcelona, Spain
| | - G. Tosti
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - A. Tramacere
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Consorzio Interuniversitario per la Fisica Spaziale (CIFS), I–10133 Torino, Italy
| | - Y. Uchiyama
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. L. Usher
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - V. Vasileiou
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Center for Research and Exploration in Space Science and Technology (CRESST), NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- University of Maryland, Baltimore County, Baltimore, MD 21250, USA
| | - C. Venter
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- North-West University, Potchefstroom Campus, Potchefstroom 2520, South Africa
| | - N. Vilchez
- Centre d'Étude Spatiale des Rayonnements, CNRS/Université Paul Sabatier (UPS), BP 44346, F–30128 Toulouse Cedex 4, France
| | - V. Vitale
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma “Tor Vergata,” I–00133 Roma, Italy
- Dipartimento di Fisica, Università di Roma “Tor Vergata,” I–00133 Roma, Italy
| | - A. P. Waite
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Wang
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - B. L. Winer
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - K. S. Wood
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - R. Yamazaki
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - T. Ylinen
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE–106 91 Stockholm, Sweden
- Department of Physics, Royal Institute of Technology (KTH), AlbaNova, SE–106 91 Stockholm, Sweden
- School of Pure and Applied Natural Sciences, University of Kalmar, SE–391 82 Kalmar, Sweden
| | - M. Ziegler
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
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Artigas L, Otero E, Paranhos R, Gómez M, Piccini C, Costagliola M, Silva R, Suárez P, Gallardo V, Hernández-Becerril D, Chistoserdov A, Vieira R, Perez- Cenci M, Ternon J, Beker B, Thyssen M, Dionisi H, Do Rosario Marinho-Jaussaud I, Gonzalez A, Hurtado C, Parra J, Alonso C, Hozbor C, Peressutti S, Negri R, Espinoza C, Cardoso A, Martins O, Covacevich F, Berón C, Salerno G. Towards a Latin American and Caribbean international census of marine microbes (LACar ? ICoMM): overview and discussion on some current research directions. REV BIOL TROP 2007. [DOI: 10.15517/rbt.v56i0.5587] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022] Open
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Espinoza C, Medina C, Somerville S, Arce-Johnson P. Senescence-associated genes induced during compatible viral interactions with grapevine and Arabidopsis. J Exp Bot 2007; 58:3197-212. [PMID: 17761729 DOI: 10.1093/jxb/erm165] [Citation(s) in RCA: 75] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/17/2023]
Abstract
The senescence process is the last stage in leaf development and is characterized by dramatic changes in cellular metabolism and the degeneration of cellular structures. Several reports of senescence-associated genes (SAGs) have appeared, and an overlap in some of the genes induced during senescence and pathogen infections has been observed. For example, the enhanced expression of SAGs in response to diseases caused by fungi, bacteria, and viruses that trigger the hypersensitive response (HR) or during infections induced by virulent fungi and bacteria that elicit necrotic symptoms has been observed. The present work broadens the search for SAGs induced during compatible viral interactions with both the model plant Arabidopsis thaliana and a commercially important grapevine cultivar. The transcript profiles of Arabidopsis ecotype Uk-4 infected with tobacco mosaic virus strain Cg (TMV-Cg) and Vitis vinifera cv. Carménère infected with grapevine leafroll-associated virus strain 3 (GLRaV-3) were analysed using microarray slides of the reference species Arabidopsis. A large number of SAGs exhibited altered expression during these two compatible interactions. Among the SAGs were genes that encode proteins such as proteases, lipases, proteins involved in the mobilization of nutrients and minerals, transporters, transcription factors, proteins related to translation and antioxidant enzymes, among others. Thus, part of the plant's response to virus infection appears to be the activation of the senescence programme. Finally, it was demonstrated that several virus-induced genes are also expressed at elevated levels during natural senescence in healthy plants.
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Affiliation(s)
- C Espinoza
- Departamento de Genética Molecular y Microbiología, Facultad de Ciencias Biológicas, Pontificia Universidad Católica de Chile, Alameda 340, Santiago de Chile, Casilla 114-D, Chile
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Espinoza C, Vega A, Medina C, Schlauch K, Cramer G, Arce-Johnson P. Gene expression associated with compatible viral diseases in grapevine cultivars. Funct Integr Genomics 2006; 7:95-110. [PMID: 16775684 DOI: 10.1007/s10142-006-0031-6] [Citation(s) in RCA: 54] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/16/2005] [Revised: 04/11/2006] [Accepted: 04/14/2006] [Indexed: 12/20/2022]
Abstract
Viral diseases affect grapevine cultures without inducing any resistance response. Thus, these plants develop systemic diseases and are chronically infected. Molecular events associated with viral compatible infections responsible for disease establishment and symptoms development are poorly understood. In this study, we surveyed viral infection in grapevines at a transcriptional level. Gene expression in the Vitis vinifera red wine cultivars Carménère and Cabernet-Sauvignon naturally infected with GLRaV-3 were evaluated using a genome-wide expression profiling with the Vitis vinifera GeneChip from Affymetrix. We describe numerous genes that are induced or repressed in viral infected grapevines leaves. Changes in gene expression involved a wide spectrum of biological functions, including processes of translation and protein targeting, metabolism, transport, and cell defense. Considering cellular localization, the membrane and endomembrane systems appeared with the highest number of induced genes, while chloroplastic genes were mostly repressed. As most induced genes associated with the membranous system are involved in transport, the possible effect of virus in this process is discussed. Responses of both cultivars are analyzed and the results are compared with published data from other species. This is the first study of global gene profiling in grapevine in response to viral infections using DNA microarray.
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Affiliation(s)
- C Espinoza
- Departamento de Genética Molecular y Microbiología, Facultad de Ciencias Biológicas, Pontificia Universidad Católica de Chile, Casilla 114-D, Alameda 340, Santiago, Chile.
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Troncoso R, Espinoza C, Sánchez-Estrada A, Tiznado M, García HS. Analysis of the isothiocyanates present in cabbage leaves extract and their potential application to control Alternaria rot in bell peppers. Food Res Int 2005. [DOI: 10.1016/j.foodres.2005.02.004] [Citation(s) in RCA: 43] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/25/2022]
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22
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Espinoza C, Camaño A, Díaz R. Spatial and temporal comparison of copper bioaccumulation in the mussel Aulacomya ater (Molina) from Jorgillo location (23 degrees 45'S; 79 degrees 27'W) and Dichato location (36 degrees 32'S; 71 degrees 56'W), Chile. Bull Environ Contam Toxicol 2004; 73:1049-1056. [PMID: 15674719 DOI: 10.1007/s00128-004-0531-9] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/24/2023]
Affiliation(s)
- C Espinoza
- Laboratorio de Ecotoxicología, Instituto de Investigación Pesquera, 8 Región S.A., Av. Casilla 350, Talcahuano, Chile
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23
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Espinoza C, Strauss F, Devoto. Acute signaling pathways of the human corpus luteum are dependent on protein kinase A/C activation. Effect of GnRH antagonist. Fertil Steril 2004. [DOI: 10.1016/j.fertnstert.2004.07.843] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/26/2022]
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24
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Repo-Carrasco R, Espinoza C, Jacobsen SE. Nutritional Value and Use of the Andean Crops Quinoa (Chenopodium quinoa) and Kañiwa (Chenopodium pallidicaule). Food Reviews International 2003. [DOI: 10.1081/fri-120018884] [Citation(s) in RCA: 364] [Impact Index Per Article: 17.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
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Kerut EK, Given MB, McIlwain E, Allen G, Espinoza C, Giles TD. Echocardiographic texture analysis using the wavelet transform: differentiation of early heart muscle disease. Ultrasound Med Biol 2000; 26:1445-1453. [PMID: 11179619 DOI: 10.1016/s0301-5629(00)00289-1] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
Abstract
Echocardiographic quantitation of myocardial texture for diagnosis of early cardiomyopathy (CMP) remains problematic. Conventional statistical methods are limited, contributed by a small image region-of-interest (ROI) and difficulty in discrimination from noise. This study was performed to evaluate the 2-D Haar wavelet decomposition method as a tool to identify textural changes in a rat model of early CMP, focusing on changes that occur before development of M-mode structural abnormalities. Early diabetic CMP, ethanol CMP and diabetic-ethanol CMP rat models were evaluated. Echocardiography was performed on two groups of rats. Group I (5 week cohort, n = 4 per subgroup) included controls, rats on 12% ethanol, a diabetic subgroup, and diabetic rats on 4% ethanol. Group II (10 week cohort, n = 5 per subgroup) included the same categories as group I with an additional subgroup taking 4% ethanol was also studied. M-mode left ventricular measurements were comparable in all subgroups of group I. However, diabetic rats in group II had an increased left ventricular dimension (LVD) compared to all others and an increased septal dimension (IVSD) and posterior wall dimension (PWD) were noted in the 4% and 12% ethanol groups. End-diastolic digital images of all rats in the parasternal short axis view, at the papillary muscle level, were downloaded to a computer. A 16 x 16 (ROI) was selected from the anterior interventricular septum. Although standard statistical methods could not differentiate any of the groups, calculation of textural energy and normalized textural energy with the 2-D Haar wavelet decomposition method found at 5 weeks increased normalized texture energy in diabetics compared to all others. At 10 weeks increased texture energy was noted in diabetics. Diabetic-ethanol rats at both 5 and 10 weeks revealed a blunted textural energy compared to diabetic rats. In a rat model of diabetic cardiomyopathy, the 2-D wavelet decomposition method identified textural energy changes before development of echocardiographic structural changes. Ethanol-associated blunting of textural changes in diabetic rats was also noted. This method for quantitation of ventricular texture may be relevant for diagnosis of early cardiomyopathy.
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Affiliation(s)
- E K Kerut
- Cardiovascular Research Laboratory, Division of Cardiology, Louisiana State University Health Sciences Center, New Orleans, LA, USA.
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26
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Atkins R, Benbow W, Berley D, Chen ML, Coyne DG, Delay RS, Dingus BL, Dorfan DE, Ellsworth RW, Espinoza C, Evans D, Falcone A, Fleysher L, Fleysher R, Gisler G, Goodman JA, Haines TJ, Hoffman CM, Hugenberger S, Kelley LA, Leonor I, McConnell M, McCullough JF, McEnery JE, Miller RS, Mincer AI, Morales MF, Murray MM, Nemethy P, Ryan JM, Schneider M, Shen B, Shoup A, Sinnis C, Smith AJ, Sullivan GW, Thompson TN, Tumer T, Wang K, Wascko MO, Westerhoff S, Williams DA, Yang T, Yodh GB. TeV Observations of Markarian 501 with the Milagrito Water Cerenkov Detector. Astrophys J 1999; 525:L25-L28. [PMID: 10511505 DOI: 10.1086/312332] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
Abstract
The Milagrito water Cerenkov detector near Los Alamos, New Mexico, was operated as a sky monitor at energies of a few TeV between 1997 February and 1998 May, including the period of the strong, long-lasting 1997 flare of Markarian 501. Milagrito served as a test run for the full Milagro detector. An event excess with a significance of 3.7 sigma from Markarian 501 was observed, in agreement with expectations.
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Espinoza C, Manito N, Roca J, Castells E, Mauri J, Ribas M, Claret G. Reversibility of pulmonary hypertension in patients evaluated for orthotopic heart transplantation: importance in the postoperative morbidity and mortality. Transplant Proc 1999; 31:2503-4. [PMID: 10500689 DOI: 10.1016/s0041-1345(99)00436-4] [Citation(s) in RCA: 29] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/22/2022]
Affiliation(s)
- C Espinoza
- Princeps d'Espanya Hospital, Barcelona, Spain.
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Espinoza C, Manito N, Castells E, Roca J, Rodriguez R, Octavio de Toledo MC, Calbet JM, Fontanillas C, Saura E, Miralles A, Granados J, Benito M, Mauri F, Ramón JM, Obi C, Quiles C, Claret G. Pretransplant risk factors of early mortality after orthotopic heart transplantation. Transplant Proc 1999; 31:2507-8. [PMID: 10500691 DOI: 10.1016/s0041-1345(99)00438-8] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/18/2022]
Affiliation(s)
- C Espinoza
- Princeps d'Espanya Hospital, Barcelona, Spain
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Miralles A, Espinoza C, Rodriguez R, Flajsig I, Saura E, Calbet JM, Granados J, Benito M, Castells E. Reduction aortoplasty: readaptation technique in great vessel mismatches in heart transplantation. Transplant Proc 1999; 31:2501-2. [PMID: 10500688 DOI: 10.1016/s0041-1345(99)00435-2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Affiliation(s)
- A Miralles
- Department of Cardiac Surgery, Ciutat Sanitària i Universitària de Bellvitge, Barcelona, Spain
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Castells E, Espinoza C, Calbet JM, Octavio de Toledo MC, Saura E, Benito M, Granados J, Manito N, Miralles A, Roca J, Rodriguez R, Rullan C, Esplugas E. Surgical extracardiac thoracic complications in heart transplantation. Transplant Proc 1999; 31:2511-2. [PMID: 10500693 DOI: 10.1016/s0041-1345(99)00440-6] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022]
Affiliation(s)
- E Castells
- Department of Cardiac Surgery, Anesthesiology and Cardiology, Hospitalet de Llobregat, Barcelona, Spain
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Manito N, Perez JL, Roca J, Castells E, Niubó J, Garcia A, Ribas M, Saura E, Rufí G, Gomez-Hospital JA, Espinoza C, Esplugas E. Usefulness of quantitative cytomegalovirus antigenemia determinations in heart transplantation. Transplant Proc 1999; 31:2526-7. [PMID: 10500700 DOI: 10.1016/s0041-1345(99)00447-9] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/17/2022]
Affiliation(s)
- N Manito
- Servicio de Cardiología, Ciudad Sanitaria y Universitaria de Bellvitge, Barcelona, Spain
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Espinoza C, Manito N, Castells E, Rodriguez R, Octavio de Toledo MC, Calbet JM, Fontanillas C, Saura E, Miralles A, Granados J, Benito M, Roca J, Mauri F, Ramon JM, Obi C, Quiles C, Claret G. Perioperative mortality risk factors after orthotopic heart transplantation. Transplant Proc 1999; 31:2509-10. [PMID: 10500692 DOI: 10.1016/s0041-1345(99)00439-x] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/26/2022]
Affiliation(s)
- C Espinoza
- Princeps d'Espanya Hospital, Barcelona, Spain
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33
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Chen L, Marmey P, Taylor NJ, Brizard JP, Espinoza C, D'Cruz P, Huet H, Zhang S, de Kochko A, Beachy RN, Fauquet CM. Expression and inheritance of multiple transgenes in rice plants. Nat Biotechnol 1998; 16:1060-4. [PMID: 9831036 DOI: 10.1038/3511] [Citation(s) in RCA: 78] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
Abstract
The ability to control integration, inheritance, and expression of multiple transgenes is a prerequisite for manipulating biosynthetic pathways and complex agronomic characteristics in plants. One hundred and twenty-five independent transgenic rice plants were regenerated after cobombarding embryogenic tissues with a mixture of 14 different pUC-based plasmids. Eighty-five percent of the R0 plants contained more than two, and 17% more than nine, of the target genes. Plants containing multiple transgenes displayed normal morphologies and 63% set viable seed. Multigene cotransformation efficiency was correlated with the ratio in which the plasmids were mixed with respect to the selectable marker. All target genes had an equal chance of integration, indicating that the nature of the coding region had no effect on the efficiency of integration. Three plant lines containing 11, 10, and 9 transgenes, respectively, were analyzed for patterns of integration and inheritance until the R3 generation. Integration of multiple transgenes occurred at either one or two genetic loci, with inheritance conforming to a 3:1 Mendelian ratio. Coexpression of four marker genes was investigated until the R2 generation.
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Affiliation(s)
- L Chen
- International Laboratory for Tropical Agricultural Biotechnology, (ORSTOM-TSRI), Division of Plant Biology, The Scripps Research Institute, La Jolla, CA 92037, USA
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Calbet JM, Obi C, Rodríguez R, Espinoza C, Benito M, Granados J, Fontanillas C, Miralles A, Saura E, Castells E. [Aneurysms of the left ventricle. Surgical treatment]. Rev Esp Cardiol 1998; 51 Suppl 3:80-5. [PMID: 9717408] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/08/2023]
Abstract
Left ventricular aneurysm as a complication of myocardial infarction is observed in 10% of patients. In recent years, all surgical teams have observed a significant decrease of this complication. There is no doubt that this is due to the current medical treatment in the acute phase of myocardial infarction. Surgical treatment is considered only when the ventricular aneurysm presents complications such as congestive heart failure, thromboembolism, malignant ventricular arrhythmias or angina. In this review, we comment on the principle surgical procedures reported up to now. The indication of surgery is based on good functional results and long-term survival.
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Affiliation(s)
- J M Calbet
- Servicio de Cirugía Cardíaca, Ciudad Sanitaria y Universitaria de Bellvitge, Hospital Príncipes de España, Barcelona
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Díaz-Véliz G, Alarcón T, Espinoza C, Dussaubat N, Mora S. Ketanserin and anxiety levels: influence of gender, estrous cycle, ovariectomy and ovarian hormones in female rats. Pharmacol Biochem Behav 1997; 58:637-42. [PMID: 9329052 DOI: 10.1016/s0091-3057(97)90004-6] [Citation(s) in RCA: 91] [Impact Index Per Article: 3.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 02/05/2023]
Abstract
The influence of gender, estrous cycle, ovariectomy and ovarian hormones on the behavioral effects of the 5-HT2 receptor antagonist, ketanserin (KET), was studied. Intact males, female rats in the four stages of the estrous cycle and ovariectomized (OVX) female rats 14 days after surgery were used. The OVX rats received progesterone [PROG, 25 mg/kg, subcutaneously (SC)] and/or estradiol benzoate (EB, 10 micrograms/kg, SC). KET (3 mg/kg, SC) was injected 30 min before testing. All the animals were subjected to the following behavioral tests: exploration of an elevated plus-maze and retention of a passive-avoidance response. KET enhanced the exploration of the open arms in diestrous female rats but inhibited this behavior during the other stages of the cycle and in OVX rats injected either with oil or EB. This dose of KET was ineffective in males and in OVX rats injected with PROG. Furthermore, KET inhibited the retention of the passive avoidance response in males, in diestrous and metestrous female rats and in OVX rats injected with oil. In estrous females and in OVX rats injected with EB, KET enhanced the passive-avoidance response. These results demonstrate that the sensitivity to KET differs with the gender, estrous cycle and hormonal treatment and suggest that central serotonergic activity is influenced by the hormonal status of the animal.
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Affiliation(s)
- G Díaz-Véliz
- Unidad de Farmacología, Facultad de Medicina, Universidad de Chile, Santiago, Chile
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Toro H, Espinoza C, Ponce V, Rojas V, Morales MA, Kaleta EF. Infectious Bronchitis: Effect of Viral Doses and Routes on Specific Lacrimal and Serum Antibody Responses in Chickens. Avian Dis 1997. [DOI: 10.2307/1592193] [Citation(s) in RCA: 24] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
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Toro H, Espinoza C, Ponce V, Rojas V, Morales MA, Kaleta EF. Infectious bronchitis: effect of viral doses and routes on specific lacrimal and serum antibody responses in chickens. Avian Dis 1997; 41:379-87. [PMID: 9201403] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/04/2023]
Abstract
An enzyme-linked immunosorbent assay was used to measure the effect of various infectious bronchitis virus (IBV) (strain H-120) vaccine doses and routes of immunization on specific lacrimal and serum antibody responses. The results of the first trial showed that the maximum dose, 10(6) median embryo infective doses (EID50s), delivered by the ocular route elicited both a systemic and a local antibody response in the vaccinated chickens. Lower doses of vaccinal virus, 10(4) (median dose) and 10(2) (minimum dose) EID50 delivered by the same route did not induce a detectable systemic antibody response. A significant increase of IBV-specific lacrimal IgA was elicited by both the maximum and the median vaccine doses. The low vaccine dose (10(2) EID50) did not induce a detectable increase of lacrimal IgA. In a second trial approximately the same vaccine dose was administered to different chicken groups by ocular instillation, drinking water, spray, and cloaca. The results showed that all routes of vaccination tested, including the cloacal route, resulted in an increase of specific serum antibodies. Higher IgG levels were detected throughout the experimental period after vaccination by the ocular route as compared with vaccination via the drinking water. All routes of vaccination tested resulted in an increase of specific IgA in lacrimal fluid. The vaccine application methods spray, ocular instillation, and drinking water induced similar lacrimal IgA responses.
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Affiliation(s)
- H Toro
- Faculty of Veterinary Sciences, University of Chile, Santiago, Chile
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Levine OS, Ortiz E, Contreras R, Lagos R, Vial P, Misraji A, Ferreccio C, Espinoza C, Adlerstein L, Herrera P. Cost-benefit analysis for the use of Haemophilus influenzae type b conjugate vaccine in Santiago, Chile. Am J Epidemiol 1993; 137:1221-8. [PMID: 8322763 DOI: 10.1093/oxfordjournals.aje.a116624] [Citation(s) in RCA: 33] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/29/2023] Open
Abstract
Cost-benefit analyses can be integral to the evaluation of interventions in developing countries. The authors compare the potential benefits to the Chilean Ministry of Health, in terms of treatment costs averted, by prevention of Haemophilus influenzae type b (HIB) invasive disease, with the costs of adding HIB conjugate vaccine to the diphtheria-tetanus-pertussis (DTP) immunization routinely administered to infants. In their basecase model, over a 10-year period (1991-2000), vaccination against HIB will prevent 1,229 cases of HIB invasive disease, including 713 cases of meningitis, 107 of whom would suffer severe, long-term sequelae, and between 29 and 116 deaths. Assuming a cost of US$1 for a full three-dose regimen of vaccine, the benefit/cost ratio of 1.66, with a net discounted savings of over $403,225, illustrates that HIB vaccine can be cost-beneficial. Sensitivity analyses which alter each of the variables in the analysis indicate that if the true incidence of HIB disease is twice the published rate, then three doses of vaccine remains cost-beneficial at US#3.
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Affiliation(s)
- O S Levine
- Center for Vaccine Development, University of Maryland School of Medicine, Baltimore 21201
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Abstract
A five-generation white family with multiple endocrine neoplasia type 2A had six affected members. Two, a mother and her daughter, had interscapular cutaneous pruritic lesions resembling macular/lichen amyloidosis. In the daughter, light microscopy showed homogeneous aggregates in the papillary dermis. Crystal violet staining showed metachromasia and indicated that the deposits were amyloid. This is the fourth family with familial medullary thyroid carcinoma with cutaneous amyloidosis and as such it allowed comparative analysis. Genetic heterogeneity, a contiguous gene, and pleiotropy were considered. It appears that multiple endocrine neoplasia type 2A/familial medullary thyroid carcinoma with cutaneous amyloidosis represents the phenotypic variability of the expression of a pleiotropic gene. The condition is one of the predominantly ectodermal autosomal dominant phakomatoses and is most likely a paracrinopathy.
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Affiliation(s)
- B G Kousseff
- Department of Pediatrics, University of South Florida, Tampa 33612-4799
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Medel M, Espinoza C, Zipper J, Prager R. Preliminary observations on the effects of copper, zinc and polyethylene I. U. F. Bs. on the uterine motility of the rabbit. Contraception 1972; 5:203-13. [PMID: 4568274 DOI: 10.1016/0010-7824(72)90046-7] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/11/2023]
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