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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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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3
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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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4
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Arensman E, Larkin C, McCarthy J, Leitao S, Corcoran P, Williamson E, McAuliffe C, Perry IJ, Griffin E, Cassidy EM, Bradley C, Kapur N, Kinahan J, Cleary A, Foster T, Gallagher J, Malone K, Ramos Costa AP, Greiner BA. Psychosocial, psychiatric and work-related risk factors associated with suicide in Ireland: optimised methodological approach of a case-control psychological autopsy study. BMC Psychiatry 2019; 19:275. [PMID: 31492119 PMCID: PMC6728991 DOI: 10.1186/s12888-019-2249-6] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 03/02/2019] [Accepted: 08/20/2019] [Indexed: 01/19/2023] Open
Abstract
BACKGROUND Suicide has profound effects on families and communities, but is a statistically rare event. Psychological autopsies using a case-control design allow researchers to examine risk factors for suicide, using a variety of sources to detail the psychological and social characteristics of decedents and to compare them to controls. The Suicide Support and Information System Case Control study (SSIS-ACE) aimed to compare psychosocial, psychiatric and work-related risk factors across three groups of subjects: suicide decedents, patients presenting to hospital with a high-risk self-harm episode, and general practice controls. METHODS The study design includes two inter-related studies; one main case-control study: comparing suicide cases to general practice (GP) controls, and one comparative study: comparing suicide cases to patients presenting with high-risk self-harm. Consecutive cases of suicide and probable suicide are identified through coroners' registration of deaths in the defined region (Cork City and County, Ireland) and are frequency-matched for age group and gender with GP patient controls recruited from the same GP practice as the deceased. Data sources for suicide cases include coroners' records, interviews with health care professionals and proxy informants; data sources for GP controls and for high-risk self-harm controls include interviews with control, with proxy informants and with health care professionals. Interviews are semi-structured and consist of quantitative and qualitative parts. The quantitative parts include a range of validated questionnaires addressing psychiatric, psychosocial and occupational factors. The study adopts several methodological innovations, including accessing multiple data sources for suicide cases and controls simultaneously, recruiting proxy informants to examine consistency across sources. CONCLUSIONS The study allows for the investigation of consistency across different data sources and contributes to the methodological advancement of psychological autopsy research. The study will also inform clinical and public health practice. The comparison between suicide cases and controls will allow investigation of risk and protective factors for suicide more generally, while the comparison with high-risk self-harm patients will help to identify the factors associated specifically with a fatal outcome to a self-harm episode. A further enhancement is the particular focus on specific work-related risk factors for suicide.
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Affiliation(s)
- E. Arensman
- 0000000123318773grid.7872.aNational Suicide Research Foundation and School of Public Health, College of Medicine and Health, University College Cork, Western Gateway Building, Cork, Ireland
| | - C. Larkin
- 0000 0001 0742 0364grid.168645.8Department of Emergency Medicine, University of Massachusetts Medical School, Worcester, 01655 USA
| | | | - S. Leitao
- 0000 0004 0617 6269grid.411916.aSchool of Public Health, College of Medicine and Health and National Perinatal Epidemiology Centre, Department of Obstetrics and Gynaecology, Cork University Hospital Maternity Hospital, Wilton, Cork, Ireland
| | - P. Corcoran
- 0000000123318773grid.7872.aNational Suicide Research Foundation and School of Public Health, University College Cork, Western Gateway Building, Cork, Ireland
| | - E. Williamson
- 0000000123318773grid.7872.aNational Suicide Research Foundation, University College Cork, Western Gateway Building, Cork, Ireland
| | - C. McAuliffe
- St. Patrick’s Mental Health Services, Cork, Ireland
| | - I. J. Perry
- 0000000123318773grid.7872.aSchool of Public Health, College of Medicine and Health, University College Cork, Western Gateway Building, Cork, Ireland
| | - E. Griffin
- 0000000123318773grid.7872.aNational Suicide Research Foundation, University College Cork, Western Gateway Building, Cork, Ireland
| | - E. M. Cassidy
- Department of Psychiatry and Neurobehavioural Science, University College Cork, Liaison Psychiatry Service, Cork University Hospital, Cork, Ireland
| | - C. Bradley
- 0000000123318773grid.7872.aDepartment of General Practice, University College Cork, Western Gateway Building, Cork, Ireland
| | - N. Kapur
- 0000 0004 0430 6955grid.450837.dCentre for Mental Health and Safety, University of Manchester and Greater Manchester Mental Health NHS Foundation Trust, Manchester, UK
| | - J. Kinahan
- 0000 0004 0575 9497grid.411785.eNorth Lee Psychiatric Services, Mercy University Hospital, Cork, Ireland
| | - A. Cleary
- 0000 0001 0768 2743grid.7886.1Geary Institute for Public Policy, University College Dublin, Dublin, Ireland
| | - T. Foster
- Consultant Psychiatrist, Omagh and Fermanagh, Northern Ireland
| | - J. Gallagher
- 0000000123318773grid.7872.aSchool of Public Health, University College Cork, Cork, Ireland
| | - K. Malone
- 0000 0001 0768 2743grid.7886.1School of Medicine, University College Dublin, Dublin, Ireland
| | - A. P. Ramos Costa
- 0000000123318773grid.7872.aSchool of Public Health and National Suicide Research Foundation, University College Cork, Cork, Ireland
| | - B. A. Greiner
- 0000000123318773grid.7872.aSchool of Public Health, College of Medicine and Health, University College Cork, Cork, Ireland
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5
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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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Malone S, Eapen L, C.E., Kendal W, MacRae R, Perry G, Malone K, Bowen J, Craig J, Grimes S, Morgan S. Results of a Phase III Trial of Optimal Sequencing of Dose Escalated Radiation (XRT) and 6 Months Androgen Deprivation Therapy (ADT) in Prostate Cancer. Int J Radiat Oncol Biol Phys 2018. [DOI: 10.1016/j.ijrobp.2018.06.064] [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: 11/26/2022]
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7
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Abeysekara A, Albert A, Alfaro R, Alvarez C, Álvarez J, Arceo R, Arteaga-Velázquez J, Avila Rojas D, Ayala Solares H, Belmont-Moreno E, BenZvi S, Braun J, Brisbois C, Caballero-Mora K, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Diaz Hernandez R, Dichiara S, Dingus B, DuVernois M, Ellsworth R, Engel K, Enríquez-Rivera O, Fleischhack H, Fraija N, Galván-Gámez A, García-González J, González Muñoz A, González M, Hampel-Arias Z, Harding J, Hernandez S, Hona B, Hueyotl-Zahuantitla F, Hui C, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Lara A, Lee W, León Vargas H, Linnemann J, Longinotti A, Luis-Raya G, Luna-García R, López-Coto R, Malone K, Marinelli S, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews J, Miranda-Romagnoli P, Moreno E, Mostafá M, Nellen L, Newbold M, Nisa M, Noriega-Papaqui R, Pelayo R, Pretz J, Pérez-Pérez E, Ren Z, Rho C, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Seglar Arroyo M, Sinnis G, Smith A, Springer R, Surajbali P, Taboada I, Tibolla O, Torres I, Villaseñor L, Weisgarber T, Westerhoff S, Wood J, Yapici T, Yodh G, Zepeda A, Zhou H. Constraining the
p¯/p
ratio in TeV cosmic rays with observations of the Moon shadow by HAWC. Int J Clin Exp Med 2018. [DOI: 10.1103/physrevd.97.102005] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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8
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Abeysekara AU, Albert A, Alfaro R, Alvarez C, Álvarez JD, Arceo R, Arteaga-Velázquez JC, Avila Rojas D, Ayala Solares HA, Barber AS, Bautista-Elivar N, Becerril A, Belmont-Moreno E, BenZvi SY, Berley D, Bernal A, Braun J, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Dingus BL, DuVernois MA, Díaz-Vélez JC, Ellsworth RW, Engel K, Enríquez-Rivera O, Fiorino DW, Fraija N, García-González JA, Garfias F, Gerhardt M, González Muñoz A, González MM, Goodman JA, Hampel-Arias Z, Harding JP, Hernández S, Hernández-Almada A, Hinton J, Hona B, Hui CM, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Kieda D, Lara A, Lauer RJ, Lee WH, Lennarz D, Vargas HL, Linnemann JT, Longinotti AL, Luis Raya G, Luna-García R, López-Coto R, Malone K, Marinelli SS, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews JA, Miranda-Romagnoli P, Moreno E, Mostafá M, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Pelayo R, Pretz J, Pérez-Pérez EG, Ren Z, Rho CD, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salazar H, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Sinnis G, Smith AJ, Springer RW, Surajbali P, Taboada I, Tibolla O, Tollefson K, Torres I, Ukwatta TN, Vianello G, Weisgarber T, Westerhoff S, Wisher IG, Wood J, Yapici T, Yodh G, Younk PW, Zepeda A, Zhou H, Guo F, Hahn J, Li H, Zhang H. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth. Science 2018; 358:911-914. [PMID: 29146808 DOI: 10.1126/science.aan4880] [Citation(s) in RCA: 211] [Impact Index Per Article: 35.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/20/2017] [Accepted: 10/09/2017] [Indexed: 11/02/2022]
Abstract
The unexpectedly high flux of cosmic-ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary production. We report the detection, using the High-Altitude Water Cherenkov Observatory (HAWC), of extended tera-electron volt gamma-ray emission coincident with the locations of two nearby middle-aged pulsars (Geminga and PSR B0656+14). The HAWC observations demonstrate that these pulsars are indeed local sources of accelerated leptons, but the measured tera-electron volt emission profile constrains the diffusion of particles away from these sources to be much slower than previously assumed. We demonstrate that the leptons emitted by these objects are therefore unlikely to be the origin of the excess positrons, which may have a more exotic origin.
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Affiliation(s)
- A U Abeysekara
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - A Albert
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - R Alfaro
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - C Alvarez
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - J D Álvarez
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - R Arceo
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | | | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H A Ayala Solares
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A S Barber
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | | | - A Becerril
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - E Belmont-Moreno
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - S Y BenZvi
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - D Berley
- Department of Physics, University of Maryland, College Park, MD, USA
| | - A Bernal
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J Braun
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - C Brisbois
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | | | - T Capistrán
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - S Casanova
- Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland.,Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - M Castillo
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J Cotzomi
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - S Coutiño de León
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - C De León
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - E De la Fuente
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico
| | - B L Dingus
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico
| | - R W Ellsworth
- School of Physics, Astronomy, and Computational Sciences, George Mason University, Fairfax, VA, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, MD, USA
| | - O Enríquez-Rivera
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - D W Fiorino
- Department of Physics, University of Maryland, College Park, MD, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J A García-González
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - F Garfias
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Gerhardt
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A González Muñoz
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M M González
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, MD, USA
| | - Z Hampel-Arias
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J P Harding
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - S Hernández
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Hernández-Almada
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J Hinton
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - B Hona
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - C M Hui
- Astrophysics Office, NASA Marshall Space Flight Center Huntsville, AL, USA
| | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A Iriarte
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Jardin-Blicq
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - V Joshi
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - S Kaufmann
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - D Kieda
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - A Lara
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - R J Lauer
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - W H Lee
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - D Lennarz
- School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, USA
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - A L Longinotti
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - G Luis Raya
- Universidad Politecnica de Pachuca, Pachuca, Hidalgo, Mexico
| | - R Luna-García
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - R López-Coto
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany.
| | - K Malone
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - S S Marinelli
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - O Martinez
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | | | - J Martínez-Castro
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - H Martínez-Huerta
- Physics Department, Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City, Mexico
| | - J A Matthews
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | | | - E Moreno
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - M Mostafá
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Newbold
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - M U Nisa
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | | | - R Pelayo
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - J Pretz
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - E G Pérez-Pérez
- Universidad Politecnica de Pachuca, Pachuca, Hidalgo, Mexico
| | - Z Ren
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - C D Rho
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - C Rivière
- Department of Physics, University of Maryland, College Park, MD, USA
| | - D Rosa-González
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - M Rosenberg
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - E Ruiz-Velasco
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H Salazar
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland.
| | - A Sandoval
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Schneider
- Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - H Schoorlemmer
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - G Sinnis
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - A J Smith
- Department of Physics, University of Maryland, College Park, MD, USA
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - P Surajbali
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - I Taboada
- School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, USA
| | - O Tibolla
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - I Torres
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - T N Ukwatta
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - G Vianello
- Hansen Experimental Physics Laboratory Stanford University, Stanford, CA, USA
| | - T Weisgarber
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - S Westerhoff
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - I G Wisher
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J Wood
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - T Yapici
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - G Yodh
- Department of Physics and Astronomy, University of California, Irvine, Irvine, CA, USA
| | - P W Younk
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - A Zepeda
- Physics Department, Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City, Mexico.,Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - H Zhou
- Los Alamos National Laboratory, Los Alamos, NM, USA.
| | - F Guo
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - J Hahn
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - H Li
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - H Zhang
- Los Alamos National Laboratory, Los Alamos, NM, USA
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9
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Zia A, Russell J, Sarode R, Veeram S, Josephs S, Malone K. Markers of Coagulation Activation, Inflammation and Fibrinolysis as Predictors of Poor Outcomes After Pediatric Venous Thromboembolism: A Systematic Review and Meta-Analysis. J Vasc Surg Venous Lymphat Disord 2018. [DOI: 10.1016/j.jvsv.2017.12.007] [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: 11/27/2022]
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10
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Alfaro R, Alvarez C, Álvarez J, Arceo R, Arteaga-Velázquez J, Avila Rojas D, Ayala Solares H, Barber A, Becerril A, Belmont-Moreno E, BenZvi S, Brisbois C, Caballero-Mora K, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Diaz Hernandez R, Dichiara S, Dingus B, DuVernois M, Díaz-Vélez J, Ellsworth R, Enriquez-Rivera O, Fiorino D, Fleischhack H, Fraija N, García-González J, González Muñoz A, González M, Goodman J, Hampel-Arias Z, Harding J, Hernandez-Almada A, Hinton J, Hueyotl-Zahuantitla F, Hui C, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Lara A, Lauer R, Lennarz D, León Vargas H, Linnemann J, Longinotti A, Luis Raya G, Luna-García R, López-Cámara D, López-Coto R, Malone K, Marinelli S, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews J, Miranda-Romagnoli P, Moreno E, Mostafá M, Nellen L, Newbold M, Nisa M, Noriega-Papaqui R, Pelayo R, Pretz J, Pérez-Pérez E, Ren Z, Rho C, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Sinnis G, Smith A, Springer R, Surajbali P, Taboada I, Tibolla O, Tollefson K, Torres I, Ukwatta T, Villaseñor L, Weisgarber T, Westerhoff S, Wood J, Yapici T, Zepeda A, Zhou H. All-particle cosmic ray energy spectrum measured by the HAWC experiment from 10 to 500 TeV. Int J Clin Exp Med 2017. [DOI: 10.1103/physrevd.96.122001] [Citation(s) in RCA: 42] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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11
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Affiliation(s)
- D Smith
- Department of Endocrinology, St Vincent's University Hospital, Elm Park, Dublin 4, Ireland.
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12
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Gilhooley J, Bolger M, Charles A, Cleary E, Lane A, Malone K. Young, Male and Feeling Suicidal in Ireland: Is Help or Harm Just One Click Away? Ir Med J 2015; 108:307-308. [PMID: 26817288] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 06/05/2023]
Abstract
Reports suggest an association between internet use and the elevated risk of suicide and self harm. This study examined the resources a suicidal person might find when searching the internet 'front page' for help. Voluntary suicide help websites accounted for 7/12 front page hits. The National Suicide Research Foundation (NSRF) and the National Office for Suicide Prevention (NOSP), a blog and a newspaper article made up the remainder. Sites were difficult to navigate and highly variable in content. Phone credit was required in many cases in order to contact helplines; opening hours and locations were limited. Most statutory websites referred help-seekers to the voluntary sector, mainly the Samaritans. Information on fundraising and volunteering competed with other sources of help. Of concern, the front page also included links to methods to complete suicide. Irish professional medical bodies offered very limited advice. Our findings suggest that online information is variable and potentially harmful. There is an opportunity for all agencies and providers to generate a co-ordinated internet front page tailored for at-risk groups.
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Parvathaiah H, Daly C, Macsuibhne S, Ni chorcorain A, Guerandel A, Malone K. Development of E-learning Module On Delirium for Non-consultant Hospital Doctors Using the Delphi Method. Eur Psychiatry 2015. [DOI: 10.1016/s0924-9338(15)30782-3] [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] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 10/23/2022] Open
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14
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O’ Connor K, Brennan D, O’ Loughlin K, Wilson L, Pillay D, Clarke M, Casey P, Malone K, Lane A. Attitudes towards patients with mental illness in Irish medical students. Ir J Med Sci 2013; 182:679-85. [DOI: 10.1007/s11845-013-0955-5] [Citation(s) in RCA: 10] [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] [Received: 11/20/2012] [Accepted: 04/11/2013] [Indexed: 12/19/2022]
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Samiee S, Beaton L, Eapen L, E C, Ferrarotto C, Grimes S, Malone K, Wilkins R, Malone S. Dicentric Chromosome Assay: A Potential In Vitro Biomarker for Radiosensitivity. Int J Radiat Oncol Biol Phys 2012. [DOI: 10.1016/j.ijrobp.2012.07.1807] [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: 11/17/2022]
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16
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Haridass A, Vandervoort E, Szanto J, Sinclair J, Gratton J, Malone K, Malone S. Customized Head Cushions Reduce Patient Movement During Intracranial Radiosurgery. Int J Radiat Oncol Biol Phys 2012. [DOI: 10.1016/j.ijrobp.2012.07.1922] [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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17
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Malone S, Eapen L, C. E, Kendal W, MacRae R, D'Amico A, Perry G, Bowen J, Malone K, Grimes S. Preliminary Results of a Randomized Trial of Optimal Timing of Dose Escalated (76 Gy) Radiation and 6 months ADT in Prostate Cancer. Int J Radiat Oncol Biol Phys 2012. [DOI: 10.1016/j.ijrobp.2012.07.956] [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: 11/25/2022]
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18
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Malone S, Croke J, Belanger E, Malone K, Avruch L, Malone C, Morash C, Li Y, Nyiri B. PD-0121 USE OF PRE-OP MRI AND “3D PROSTATE CANCER MAPS” TO IMPROVE CTV DEFINITION FOR POST-OPERATIVE RADIATION. Radiother Oncol 2012. [DOI: 10.1016/s0167-8140(12)70460-7] [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: 10/28/2022]
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19
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Croke J, Nyri B, Li Y, Avruch L, Belanger E, Morash C, Kayser C, Malone K, Malone S. PO-0674 POST-OP PROSTATE RADIOTHERAPY: THE CASE OF THE MISSING TARGET, MYSTERY SOLVED. Radiother Oncol 2012. [DOI: 10.1016/s0167-8140(12)71007-1] [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: 10/28/2022]
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20
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Junqueira MJ, Morrow M, Reiner AS, Malone K, Lynch C, Bernstein JL. Patient and tumor characteristics associated with contralateral breast cancer in a nested population-based case-control study. J Clin Oncol 2011. [DOI: 10.1200/jco.2011.29.15_suppl.1014] [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: 11/20/2022] Open
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21
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Lyne J, Quinlivan L, Byrne CA, Malone K, Walsh C. Sleep hygiene use in a psychiatry outpatient setting. Ir Med J 2011; 104:49-50. [PMID: 21465876] [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] [Subscribe] [Scholar Register] [Indexed: 05/30/2023]
Abstract
Non-pharmacological measures are recommended prior to use of hypnotics in the latest NICE guidance. This study investigated if non-pharmacological measures are utilised prior to hypnotic prescribing in a general adult psychiatry outpatient setting, and further reviewed patient's sleep quality following implementation of sleep hygiene education. Interviews were conducted with 85 patients, and poor adherence with NICE guidance was found among the 74 (87%) patients previously prescribed a hypnotic. Just five (6.8%) patients recalled use of non-pharmacological measures prior to hypnotic prescription, 47 (63.5%) indicated non-pharmacological measures had not been discussed, while a further 22 (29.7%) could not remember. Improvement in Pittsburgh Sleep Quality Index scores following implementation of sleep hygiene education was also noted (P = 0.03). These findings suggest that increased awareness of sleep hygiene education for clinicians may be beneficial.
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Affiliation(s)
- J Lyne
- Department of Psychiatry, St Vincent's University Hospital, Elm Park, Dublin 4.
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Gallagher D, Guerandel A, Malone K, Barry M, Barry P. Complex visual hallucinations in a psychologically normal patient. Ir Med J 2007; 100:571-572. [PMID: 17955718] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 05/25/2023]
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23
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Malone K, Beck K, Blakeslee J, Martin L. Practicing Physician Assistant Awareness of ATP III Cholesterol Guidelines. JAAPA 2007. [DOI: 10.1097/01720610-200707000-00077] [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: 11/25/2022]
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24
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Mac Suibhne S, Guerandel A, Malone K. 21st century psychiatry teaching for 21st century doctors: how modern teaching methods may improve patient care. Ir Med J 2007; 100:484-6. [PMID: 17671997] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 05/16/2023]
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25
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Bernstein J, Bernstein L, Langholz B, Thomas D, Stovall M, Capanu M, Thompson WD, Olson J, Malone K, Lynch C, Anton-Culver H, Shore R, Boice J, Begg C, Wolitzer A, Gatti R, Rosenstein B, Borrenson-Dale AL, Concannon P, Haile R. The Interaction of Radiation, the Atm Gene and Breast Cancer. Am J Epidemiol 2006. [DOI: 10.1093/aje/163.suppl_11.s251-a] [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: 11/14/2022] Open
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26
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Affiliation(s)
- D Smith
- Department of Endocrinology, St Vincent's University Hospital, Elm Park, Dublin 4, Ireland.
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Xu F, Sahni H, Settnek S, Gupta A, Phillips J, Zhang D, Beasley J, De Coronado S, Wagner U, Rosso K, Malone K, Singer D, Marks C, Tarnowski B, Buetow K. Mouse models of human cancer web-based resources. AMIA Annu Symp Proc 2003; 2003:1056. [PMID: 14728559 PMCID: PMC1480011] [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] [Subscribe] [Scholar Register] [Indexed: 04/28/2023]
Abstract
The Mouse Models of Human Cancers Consortium (MMHCC) is a collaborative program designed to derive and characterize mouse models of human malignancies. To enhance information and resource exchange among the MMHCC investigators and other cancer research scientists, the NCI Center for Bioinformatics (NCICB, http://ncicb.nci.nih.gov/) has developed web-based resources that are freely available to the cancer research community. These resources include a website (http://emice.nci.nih.gov) and databases for cancer models (http://cancermodels.nci.nih.gov) and cancer images (http://cancerimages.nci.nih.gov).
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Affiliation(s)
- F Xu
- Center for Bioinformatics, National Cancer Institute, Rockville, Maryland, USA
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Hamajima N, Hirose K, Tajima K, Rohan T, Calle EE, Heath CW, Coates RJ, Liff JM, Talamini R, Chantarakul N, Koetsawang S, Rachawat D, Morabia A, Schuman L, Stewart W, Szklo M, Bain C, Schofield F, Siskind V, Band P, Coldman AJ, Gallagher RP, Hislop TG, Yang P, Kolonel LM, Nomura AMY, Hu J, Johnson KC, Mao Y, De Sanjosé S, Lee N, Marchbanks P, Ory HW, Peterson HB, Wilson HG, Wingo PA, Ebeling K, Kunde D, Nishan P, Hopper JL, Colditz G, Gajalanski V, Martin N, Pardthaisong T, Silpisornkosol S, Theetranont C, Boosiri B, Chutivongse S, Jimakorn P, Virutamasen P, Wongsrichanalai C, Ewertz M, Adami HO, Bergkvist L, Magnusson C, Persson I, Chang-Claude J, Paul C, Skegg DCG, Spears GFS, Boyle P, Evstifeeva T, Daling JR, Hutchinson WB, Malone K, Noonan EA, Stanford JL, Thomas DB, Weiss NS, White E, Andrieu N, Brêmond A, Clavel F, Gairard B, Lansac J, Piana L, Renaud R, Izquierdo A, Viladiu P, Cuevas HR, Ontiveros P, Palet A, Salazar SB, Aristizabel N, Cuadros A, Tryggvadottir L, Tulinius H, Bachelot A, Lê MG, Peto J, Franceschi S, Lubin F, Modan B, Ron E, Wax Y, Friedman GD, Hiatt RA, Levi F, Bishop T, Kosmelj K, Primic-Zakelj M, Ravnihar B, Stare J, Beeson WL, Fraser G, Bullbrook RD, Cuzick J, Duffy SW, Fentiman IS, Hayward JL, Wang DY, McMichael AJ, McPherson K, Hanson RL, Leske MC, Mahoney MC, Nasca PC, Varma AO, Weinstein AL, Moller TR, Olsson H, Ranstam J, Goldbohm RA, van den Brandt PA, Apelo RA, Baens J, de la Cruz JR, Javier B, Lacaya LB, Ngelangel CA, La Vecchia C, Negri E, Marubini E, Ferraroni M, Gerber M, Richardson S, Segala C, Gatei D, Kenya P, Kungu A, Mati JG, Brinton LA, Hoover R, Schairer C, Spirtas R, Lee HP, Rookus MA, van Leeuwen FE, Schoenberg JA, McCredie M, Gammon MD, Clarke EA, Jones L, Neil A, Vessey M, Yeates D, Appleby P, Banks E, Beral V, Bull D, Crossley B, Goodill A, Green J, Hermon C, Key T, Langston N, Lewis C, Reeves G, Collins R, Doll R, Peto R, Mabuchi K, Preston D, Hannaford P, Kay C, Rosero-Bixby L, Gao YT, Jin F, Yuan JM, Wei HY, Yun T, Zhiheng C, Berry G, Cooper Booth J, Jelihovsky T, MacLennan R, Shearman R, Wang QS, Baines CJ, Miller AB, Wall C, Lund E, Stalsberg H, Shu XO, Zheng W, Katsouyanni K, Trichopoulou A, Trichopoulos D, Dabancens A, Martinez L, Molina R, Salas O, Alexander FE, Anderson K, Folsom AR, Hulka BS, Bernstein L, Enger S, Haile RW, Paganini-Hill A, Pike MC, Ross RK, Ursin G, Yu MC, Longnecker MP, Newcomb P, Bergkvist L, Kalache A, Farley TMM, Holck S, Meirik O. Alcohol, tobacco and breast cancer--collaborative reanalysis of individual data from 53 epidemiological studies, including 58,515 women with breast cancer and 95,067 women without the disease. Br J Cancer 2002; 87:1234-45. [PMID: 12439712 PMCID: PMC2562507 DOI: 10.1038/sj.bjc.6600596] [Citation(s) in RCA: 675] [Impact Index Per Article: 30.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/12/2002] [Revised: 08/08/2002] [Accepted: 08/23/2002] [Indexed: 12/11/2022] Open
Abstract
Alcohol and tobacco consumption are closely correlated and published results on their association with breast cancer have not always allowed adequately for confounding between these exposures. Over 80% of the relevant information worldwide on alcohol and tobacco consumption and breast cancer were collated, checked and analysed centrally. Analyses included 58,515 women with invasive breast cancer and 95,067 controls from 53 studies. Relative risks of breast cancer were estimated, after stratifying by study, age, parity and, where appropriate, women's age when their first child was born and consumption of alcohol and tobacco. The average consumption of alcohol reported by controls from developed countries was 6.0 g per day, i.e. about half a unit/drink of alcohol per day, and was greater in ever-smokers than never-smokers, (8.4 g per day and 5.0 g per day, respectively). Compared with women who reported drinking no alcohol, the relative risk of breast cancer was 1.32 (1.19-1.45, P<0.00001) for an intake of 35-44 g per day alcohol, and 1.46 (1.33-1.61, P<0.00001) for >/=45 g per day alcohol. The relative risk of breast cancer increased by 7.1% (95% CI 5.5-8.7%; P<0.00001) for each additional 10 g per day intake of alcohol, i.e. for each extra unit or drink of alcohol consumed on a daily basis. This increase was the same in ever-smokers and never-smokers (7.1% per 10 g per day, P<0.00001, in each group). By contrast, the relationship between smoking and breast cancer was substantially confounded by the effect of alcohol. When analyses were restricted to 22 255 women with breast cancer and 40 832 controls who reported drinking no alcohol, smoking was not associated with breast cancer (compared to never-smokers, relative risk for ever-smokers=1.03, 95% CI 0.98-1.07, and for current smokers=0.99, 0.92-1.05). The results for alcohol and for tobacco did not vary substantially across studies, study designs, or according to 15 personal characteristics of the women; nor were the findings materially confounded by any of these factors. If the observed relationship for alcohol is causal, these results suggest that about 4% of the breast cancers in developed countries are attributable to alcohol. In developing countries, where alcohol consumption among controls averaged only 0.4 g per day, alcohol would have a negligible effect on the incidence of breast cancer. In conclusion, smoking has little or no independent effect on the risk of developing breast cancer; the effect of alcohol on breast cancer needs to be interpreted in the context of its beneficial effects, in moderation, on cardiovascular disease and its harmful effects on cirrhosis and cancers of the mouth, larynx, oesophagus and liver.
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Affiliation(s)
- N Hamajima
- Cancer Research UK Epidemiology Unit, Gibson Building, Radcliffe Infirmary, Woodstock Road, Oxford OX2 6HE, UK
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Malone K, Weaver S, Taylor D, Cheng H, Sarathy KP, Mills G. Formation Kinetics of Small Gold Crystallites in Photoresponsive Polymer Gels. J Phys Chem B 2002. [DOI: 10.1021/jp020176i] [Citation(s) in RCA: 36] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
Affiliation(s)
- K. Malone
- Department of Chemistry, Auburn University, Auburn, Alabama 36849
| | - S. Weaver
- Department of Chemistry, Auburn University, Auburn, Alabama 36849
| | - D. Taylor
- Department of Chemistry, Auburn University, Auburn, Alabama 36849
| | - H. Cheng
- Department of Chemistry, Auburn University, Auburn, Alabama 36849
| | - K. P. Sarathy
- Department of Chemistry, Auburn University, Auburn, Alabama 36849
| | - G. Mills
- Department of Chemistry, Auburn University, Auburn, Alabama 36849
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Landsman MJ, Groza V, Tyler M, Malone K. Outcomes of family-centered residential treatment. Child Welfare 2001; 80:351-379. [PMID: 11380046] [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] [Grants] [Subscribe] [Scholar Register] [Indexed: 05/23/2023]
Abstract
This article describes a family-centered residential treatment model and presents results from a quasiexperimental study examining its effectiveness in achieving permanency outcomes for children. Greater postdischarge stability was achieved for participants in the family-centered program than in the agency's standard residential treatment service. Implications for child welfare policy and practice are highlighted.
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Affiliation(s)
- M J Landsman
- National Resource Center for Family Centered Practice, University of Iowa, Iowa City 52242-5000, USA
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31
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Lateef F, Storrow AB, Malone K, Liu T, Gibler BW. Comparison of a 6-hour and 9-hour protocol for evaluation of moderate-to-low risk chest pain patients in an emergency department diagnostic unit. Singapore Med J 2001; 42:52-6. [PMID: 11358190] [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: 04/16/2023]
Abstract
OBJECTIVE To compare the 30-day outcomes of patients enrolled in a 6-hour and 9-hour emergency department (ED)-based chest pain centre (CPC) protocol. METHODS All patients with the chief complaint of chest pain, who were older than 25 years, or with cocaine usage within 96 hours of initial presentation, were eligible for enrolment. Exclusion criteria included acute ST-segment elevation or depression >1 mm in 2 contiguous leads, history of coronary artery disease (CAD), haemodynamic instability or clinical syndromes consistent with unstable angina. Outcomes included ED disposition and cardiac events at 30 days (defined as acute myocardial infarction (AMI), percutaneous trans-luminal coronary angiography (PTCA), coronary artery bypass graft surgery (CABG),ventricular tachycardia or fibrillation (VT/VF) arrest, congestive heart failure (CHF) admission or cardiac-related death). The 9-hour protocol consisted of ST-segment monitoring,serial CK-MB draws at 0, 3,6 and 9 hours as well as a graded exercise test (GXT) prior to ED disposition. The 6-hour protocol eliminated the 9-hour serum marker determination, included cardiac Troponin-I (cTn-I) and allowed a GXT, 3 hours earlier. Follow-up was obtained by medical record review, phone contact, letter and also review of national and state death registries. RESULTS The 9-hour protocol (October 1991-December 1997) included 2,133 patients and the 6-hour protocol (January 1998- August 1998) had 184 patients enrolled. The 6-hour protocol was not different from the 9-hour one in terms of percentage admissions (9-hour: 310, 14.5%; 6-hour: 33, 17.9%; p=0.213), Coronary Care Unit admission (9-hour: 59, 2.8%; 6-hour: 5, 2.7%; p=0.303) or 30-day cardiac events (9-hour: 38, 1.9%; 6-hour: 2, 1.3%; p=0.605). CONCLUSION The 6-hour CPC strategy is an effective and safe evaluation method for patients at low to moderate risk for acute coronary syndromes.
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Affiliation(s)
- F Lateef
- Department of Emergency Medicine, Singapore General Hospital.
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Bowen D, McTiernan A, Burke W, Powers D, Pruski J, Durfy S, Gralow J, Malone K. Participation in breast cancer risk counseling among women with a family history. Cancer Epidemiol Biomarkers Prev 1999; 8:581-5. [PMID: 10428194] [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: 02/13/2023] Open
Abstract
Recent scientific breakthroughs in the genetics of breast cancer may have had effects on women's perceptions of risk and subsequent worry about breast cancer. Here, we present the rates of interest in counseling among women identified from diverse sources, their levels of cancer worry and perceived risk, and predictors of their agreement to participate in breast cancer risk counseling. Women were identified through breast cancer cases and through media offers. They completed a telephone survey and were ultimately either entered or not entered into a counseling trial. Overall, almost half (46%) of cases who were approached responded to the contact letter asking for information about potentially interested relatives. A total of 588 women responded to the brief media solicitations over a 15-week period. Participants recruited from media contacts reported slightly but significantly higher levels of worry about getting cancer, compared to case-recruited participants. Cancer worry negatively and significantly predicted entry into the counseling project. The results presented here may have implications for recruiting women in the general population with a family history of breast cancer for counseling about their risk for the disease.
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Affiliation(s)
- D Bowen
- Fred Hutchinson Cancer Research Center, Seattle, Washington 98109-1024, USA.
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Malone K, Sohocki MM, Sullivan LS, Daiger SP. Identifying and mapping novel retinal-expressed ESTs from humans. Mol Vis 1999; 5:5. [PMID: 10228186 PMCID: PMC2583080] [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] [Grants] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/12/2023] Open
Abstract
PURPOSE The goal of this study was to develop efficient methods to identify tissue-specific expressed sequence tags (ESTs) and to map their locations in the human genome. Through a combination of database analysis and laboratory investigation, unique retina-specific ESTs were identified and mapped as candidate genes for inherited retinal diseases. METHODS DNA sequences from retina-specific EST clusters were obtained from the TIGR Human Gene Index Database. Further processing of the EST sequence data was necessary to ensure that each EST cluster represented a novel, non-redundant mapping candidate. Processing involved screening for homologies to known genes and proteins using BLAST, excluding known human gene sequences and repeat sequences, and developing primers for PCR amplification of the gene encoding each cDNA cluster from genomic DNA. The EST clusters were mapped using the GeneBridge 4.0 Radiation Hybrid Mapping Panel with standard PCR conditions. RESULTS A total of 83 retinal-expressed EST clusters were examined as potential novel, non-redundant mapping candidates. Fifty-five clusters were mapped successfully and their locations compared to the locations of known retinal disease genes. Fourteen EST clusters localize to candidate regions for inherited retinal diseases. CONCLUSIONS This pilot study developed methodology for mapping uniquely expressed retinal ESTs and for identifying potential candidate genes for inherited retinal disorders. Despite the overall success, several complicating factors contributed to the high failure rate (33%) for mapping EST-clustered sequences. These include redundancy in the sequence data, widely dispersed sequences, ambiguous nucleotides within the sequences, the possibility of amplifying through introns and the presence of repetitive elements within the sequence. However, the combination of database analysis and laboratory mapping is a powerful method for identification of candidate genes for inherited diseases.
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Affiliation(s)
- K Malone
- Human Genetics Center, School of Public Health, The University of Texas Health Science Center, Houston, TX, USA.
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Abstract
OBJECTIVE To examine demographic and behavioral factors related to perineal application of powders. METHODS Controls from three case-control studies (N = 1206) were asked identical questions about the use of genital powders by direct perineal application. The relationship of perineal powder application with demographic factors, reproductive factors, body mass index (BMI), douching, and alcohol and tobacco use was assessed. Data were analyzed by multiple logistic regression. RESULTS Women who douched (prevalence odds ratio [prevalence OR] 2.0, 95% confidence interval [CI] 1.0, 3.9), drank alcohol (prevalence OR 1.8, 95% CI 1.2, 2.8), smoked cigarettes (prevalence OR 1.3, 95% CI 1.0, 1.8), or were in the highest BMI quartile were more likely to engage in perineal use of powder (prevalence OR 1.6, 95% CI 1.1, 2.6). There appeared to be a close response relationship between the number of perineal applications of powder and BMI (P < .002). CONCLUSION Body mass index might confound the relationship between perineal powder application and the development of ovarian cancer. Other factors, such as alcohol and tobacco use and douching, are related to perineal use of powder and may represent similar behavioral characteristics.
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Affiliation(s)
- K A Rosenblatt
- Department of Community Health, University of Illinois at Urbana-Champaign, Champaign 61820, USA.
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Affiliation(s)
- M FitzGerald
- Department of Psychiatry, New York State Psychiatric Institute, College of Physicians and Surgeons of Columbia University, New York, New York 10032, USA
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Abstract
The structure and organization of health care delivery are in the midst of rapid change. Health care providers from a variety of disciplines are being challenged to define their practice and the expected patient outcomes resulting from their processes of care delivery. Standards and clinical practice guidelines are important tools for enhancing the quality of health care delivery and for documenting care. The article describes a process for developing standards and clinical practice guidelines and presents an organizational scheme for them. Based on recommendations from diverse national groups, a format for practice guidelines is presented, and a system for implementation and ongoing evaluation is recommended.
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Affiliation(s)
- H L Yoos
- Department of Pediatric Nursing, University of Rochester School of Nursing, University of Rochester Medical Center, New York, USA
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Calle EE, Heath CW, Miracle-McMahill HL, Coates RJ, Liff JM, Franceschi S, Talamini R, Chantarakul N, Koetsawang S, Rachawat D, Morabia A, Schuman L, Stewart W, Szklo M, Bain C, Schofield F, Siskind V, Band P, Coldman AJ, Gallagher RP, Hislop TG, Yang P, Duffy SW, Kolonel LM, Nomura AMY, Oberle MW, Ory HW, Peterson HB, Wilson HG, Wingo PA, Ebeling K, Kunde D, Nishan P, Colditz G, Martin N, Pardthaisong T, Silpisornkosol S, Theetranont C, Boosiri B, Chutivongse S, Jimakorn P, Virutamasen P, Wongsrichanalai C, McMichael AJ, Rohan T, Ewertz M, Paul C, Skegg DCG, Spears GFS, Boyle P, Evstifeeva T, Daling JR, Malone K, Noonan EA, Stanford JL, Thomas DB, Weiss NS, White E, Andrieu N, Brêmond A, Clavel F, Gairard B, Lansac J, Piana L, Renaud R, Fine SRP, Cuevas HR, Ontiveros P, Palet A, Salazar SB, Aristizabel N, Cuadros A, Bachelot A, Leê MG, Deacon J, Peto J, Taylor CN, Alfandary E, Modan B, Ron E, Friedman GD, Hiatt RA, Bishop T, Kosmelj K, Primic-Zakelj M, Ravnihar B, Stare J, Beeson WL, Fraser G, Allen DS, Bulbrook RD, Cuzick J, Fentiman IS, Hayward JL, Wang DY, Hanson RL, Leske MC, Mahoney MC, Nasca PC, Varma AO, Weinstein AL, Moller TR, Olsson H, Ranstam J, Goldbohm RA, van den Brandt PA, Apelo RA, Baens J, de la Cruz JR, Javier B, Lacaya LB, Ngelangel CA, La Vecchia C, Negri E, Marbuni E, Ferraroni M, Gerber M, Richardson S, Segala C, Gatei D, Kenya P, Kungu A, Mati JG, Brinton LA, Hoover R, Schairer C, Spirtas R, Lee HP, Rookus MA, van Leeuwen FE, Schoenberg JA, Gammon MD, Clarke EA, Jones L, McPherson K, Neil A, Vessey M, Yeates D, Beral V, Bull D, Crossley B, Hermon C, Jones S, Key T, Reeves CG, Smith P, Collins R, Doll R, Peto R, Hannaford P, Kay C, Rosero-Bixby L, Yuan JM, Wei HY, Yun T, Zhiheng C, Berry G, Booth JC, Jelihovsky T, Maclennan R, Shearman R, Wang QS, Baines CJ, Miller AB, Wall C, Lund E, Stalsberg H, Dabancens A, Martinez L, Molina R, Salas O, Alexander FE, Hulka BS, Chilvers CED, Bernstein L, Haile RW, Paganini-Hill A, Pike MC, Ross RK, Ursin G, Yu MC, Adami HO, Bergstrom R, Longnecker MP, Farley TMN, Holck S, Meirik O. Breast cancer and hormonal contraceptives: further results. Collaborative Group on Hormonal Factors in Breast Cancer. Contraception 1996; 54:1S-106S. [PMID: 8899264 DOI: 10.1016/s0010-7824(15)30002-0] [Citation(s) in RCA: 77] [Impact Index Per Article: 2.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/02/2023]
Abstract
The Collaborative Group on Hormonal Factors in Breast Cancer has brought together and reanalysed the worldwide epidemiological evidence on breast cancer risk and use of hormonal contraceptives. Original data from 54 studies, representing about 90% of the information available on the topic, were collected, checked and analysed centrally. The 54 studies were performed in 26 countries and include a total of 53,297 women with breast cancer and 100,239 women without breast cancer. The studies were varied in their design, setting and timing. Most information came from case-control studies with controls chosen from the general population; most women resided in Europe or North America and most cancers were diagnosed during the 1980s. Overall 41% of the women with breast cancer and 40% of the women without breast cancer had used oral contraceptives at some time; the median age at first use was 26 years, the median duration of use was 3 years, the median year of first use was 1968, the median time since first use was 16 years, and the median time since last use was 9 years. The main findings, summarised elsewhere, are that there is a small increase in the risk of having breast cancer diagnosed in current users of combined oral contraceptives and in women who had stopped use in the past 10 years but that there is no evidence of an increase in the risk more than 10 years after stopping use. In addition, the cancers diagnosed in women who had used oral contraceptives tended to be less advanced clinically than the cancers diagnosed in women who had not used them. Despite the large number of possibilities investigated, few factors appeared to modify the main findings either in recent or in past users. For recent users who began use before age 20 the relative risks are higher than for recent users who began at older ages. For women whose use of oral contraceptives ceased more than 10 years before there was some suggestion of a reduction in breast cancer risk in certain subgroups, with a deficit of tumors that had spread beyond the breast, especially among women who had used preparations containing the highest doses of oestrogen and progestogen. These findings are unexpected and need to be confirmed. Although these data represent most of the epidemiological evidence on the topic to date, there is still insufficient information to comment reliably about the effects of specific types of oestrogen or of progestogen. What evidence there is suggests, however, no major differences in the effects for specific types of oestrogen or of progestogen and that the pattern of risk associated with use of hormonal contraceptives containing progestogens alone may be similar to that observed for preparations containing both oestrogens and progestogens. On the basis of these results, there is little difference between women who have and have not used combined oral contraceptives in terms of the estimated cumulative number of breast cancers diagnosed during the period from starting use up to 20 years after stopping. The cancers diagnosed in women who have used oral contraceptives are, however, less advanced clinically than the cancers diagnosed in never users. Further research is needed to establish whether the associations described here are due to earlier diagnosis of breast cancer in women who have used oral contraceptives, to the biological effects of the hormonal contraceptives or to a combination of both. Little information is as yet available about the effects on breast cancer risk of oral contraceptive use that ceased more than 20 years before and as such data accumulate it will be necessary to re-examine the worldwide evidence.
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Decarlo M, Malone K. Response to "an alternative material for silicone casting" by james m. Sabo. J Athl Train 1996; 31:101. [PMID: 16558381 PMCID: PMC1318437] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/08/2023]
Affiliation(s)
- M Decarlo
- Methodist Sports Medicine Center, Thomas A. Brady Clinic, Indianapolis, IN 46202
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Decarlo M, Malone K, Darmelio J, Rettig A. Casting in sport. J Athl Train 1994; 29:37-43. [PMID: 16558257 PMCID: PMC1317757] [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: 05/08/2023]
Abstract
Attempts by sports medicine professionals to return high school athletes with hand and wrist injuries to competition quickly and safely have been the source of confusion and debate on many playing fields around the country. In addition to the differing views regarding the appropriateness of playing cast usage in high school football, a debate exists among sports medicine professionals as to which material is best suited for playing cast construction. Materials used in playing cast construction should be hard enough to provide sufficient stabilization to the injured area and include adequate padding to absorb blunt impact forces. The purpose of the biomechanical portion of this investigation was to attempt to determine the most appropriate materials for use in constructing playing casts for the hand and wrist by assessing different materials for: 1) hardness using a Shore durometer, and 2) ability to absorb impact using a force platform. Results revealed that RTV11 and Scotchcast were the "least hard" of the underlying casting materials and that Temper Stick foam greatly increased the ability of RTV11 to absorb impact. Assessment of the mechanical properties of playing cast materials and review of current developments in high school football rules are used to aid practitioners in choosing the most appropriate materials for playing cast construction.
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Affiliation(s)
- M Decarlo
- Mark DeCarlo is Director of Physical Therapy at Methodist Sports Medicine Center/Thomas A. Brady Clinic, 1815 N Capitol Ave, Ste 401, Indianapolis, IN 46202
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Wei WZ, Malone K, Mahoney K, Heppner G. Characterization of lymphocytic infiltrates in normal, preneoplastic, and neoplastic mouse mammary tissues. Cancer Res 1986; 46:2680-5. [PMID: 3084071] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Grants] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/04/2023]
Abstract
Lymphocytic infiltrates were isolated from normal, preneoplastic, and neoplastic mouse mammary tissues. The surface markers on the infiltrating lymphocytes were characterized by immunofluorescent staining and flow cytometry. Preneoplastic and neoplastic tissues contained 10- to 20-fold more in situ lymphocytes than did the normal pregnant gland. Most of these lympocytes were T-cells. Relative to the T-cells in normal gland, the T-cells in C4 preneoplastic hyperplastic alveolar nodules and their spontaneous tumors have shifted in favor of the killer-suppressor subpopulation. This shift of T-cell subpopulations was a localized phenomenon and was not seen in the lymph nodes of hyperplastic alveolar nodules and tumor bearing mice. C4 lesion infiltrating cells also contained a subpopulation of lymphocytes that expressed 5- to 6-fold more LFA-1 antigen (lymphocyte function associated antigen-1) than did normal lymph node cells. The infiltrating lymphocytes of mammary tumors from cloned cell lines, on the contrary, had the same staining profile as did the lymphocytes from normal gland. Since most studies with human breast cancer infiltrates have demonstrated increased killer/suppressor T-cells and the presence of activated lymphocytes (J. Hurlimann and P. Saraga, Int. J. Cancer, 35: 753-762, 1985; H.L. Whitwell, H.P.A. Hughes, M. Moore, and A. Ahmed, Br. J. Cancer, 49: 161-172, 1984; and J.A. Ledbetter, R.V. Rouse, H. Spedding Micklem, and L. Herzenberg, J. Exp. Med., 152: 280-295, 1980) the C4 hyperplastic alveolar nodules and spontaneous tumor system may be a more relevant model for studying breast cancer infiltrates.
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