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DOI: 10.1086/511173
¤ OpenAccess: Bronze
This work has “Bronze” OA status. This means it is free to read on the publisher landing page, but without any identifiable license.
First Bounds on the Very High Energy γ‐Ray Emission from Arp 220
J. Albert,E. Aliu,H. Anderhub,P. Antoranz,A. Armada,C. Baixeras,J. A. Barrio,H. Bartko,D. Bastieri,J. Becker,W. Bednarek,K. Berger,C. Bigongiari,A. Biland,R. Böck,P. Bordas,V. Bosch‐Ramon,T. Bretz,I. Britvitch,Miguel Cámara,E. Carmona,A. Chilingarian,S. Ciprini,J. A. Coarasa,S. Commichau,J. L. Contreras,J. Cortina,V. Curtef,V. Danielyan,F. Dazzi,A. De Angelis,R. de los Reyes,B. De Lotto,E. Domingo-Santamaría,D. Dorner,M. Doro,M. Errando,M. Fagiolini,D. Ferenc,E. Fernández,R. Firpo,J. Flix,M. V. Fonseca,L. Font,M. Fuchs,N. Galante,M. Garczarczyk,M. Gaug,M. Giller,F. Göebel,D. Hakobyan,M. Hayashida,T. Hengstebeck,D. Höhne,J. Hose,C. C. Hsu,P. Jacoń,T. Jogler,O. Kalekin,R. Kosyra,D. Kranich,R. Kritzer,A. Laille,P. Liebing,E. Lindfors,S. Lombardi,F. Longo,J. López,M. López,E. Lorenz,P. Majumdar,G. Maneva,Karl Mannheim,O. Mansutti,M. Mariotti,M. Martı́nez,D. Mazin,C. Merck,M. Meucci,M. Meyer,J. M. Miranda,R. Mirzoyan,S. Mizobuchi,A. Moralejo,K. Nilsson,J. Ninković,E. de Ona Wilhelmi,A. N. Otte,I. Oya,D. Paneque,R. Paoletti,J. M. Paredes,M. Pasanen,D. Pascoli,Felicitas Pauss,R. Pegna,M. Peršić,L. Peruzzo,A. Piccioli,M. Pöller,N. Puchades,E. Prandini,A. Raymers,W. Rhode,M. Ribó,J. Rico,M. Rissi,A. Robert,S. Rügamer,A. Saggion,Alejandro Sánchez,P. Sartori,V. Scalzotto,V. Scapin,R. Schmitt,T. Schweizer,M. Shayduk,K. Shinozaki,Steven N. Shore,N. Sidro,A. Sillanpaa,D. Sobczyńska,A. Stamerra,L. S. Stark,L. O. Takalo,P. Temnikov,D. Tescaro,M. Teshima,N. Tonello,D. F. Torres,N. Turini,H. Vankov,V. Vitale,R. M. Wagner,T. Wibig,W. Wittek,R. Zanin,J. Zapatero
MAGIC (telescope)
Physics
Galaxy
2007
Using the Major Atmospheric Gamma Imaging Cerenkov Telescope (MAGIC), we have observed the nearest ultraluminous infrared galaxy, Arp 220, for about 15 hr. No significant signal was detected within the dedicated amount of observation time. The first upper limits to the very high energy γ-ray flux of Arp 220 are herein reported and compared with theoretical expectations.
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“First Bounds on the Very High Energy γ‐Ray Emission from Arp 220” is a paper by J. Albert E. Aliu H. Anderhub P. Antoranz A. Armada C. Baixeras J. A. Barrio H. Bartko D. Bastieri J. Becker W. Bednarek K. Berger C. Bigongiari A. Biland R. Böck P. Bordas V. Bosch‐Ramon T. Bretz I. Britvitch Miguel Cámara E. Carmona A. Chilingarian S. Ciprini J. A. Coarasa S. Commichau J. L. Contreras J. Cortina V. Curtef V. Danielyan F. Dazzi A. De Angelis R. de los Reyes B. De Lotto E. Domingo-Santamaría D. Dorner M. Doro M. Errando M. Fagiolini D. Ferenc E. Fernández R. Firpo J. Flix M. V. Fonseca L. Font M. Fuchs N. Galante M. Garczarczyk M. Gaug M. Giller F. Göebel D. Hakobyan M. Hayashida T. Hengstebeck D. Höhne J. Hose C. C. Hsu P. Jacoń T. Jogler O. Kalekin R. Kosyra D. Kranich R. Kritzer A. Laille P. Liebing E. Lindfors S. Lombardi F. Longo J. López M. López E. Lorenz P. Majumdar G. Maneva Karl Mannheim O. Mansutti M. Mariotti M. Martı́nez D. Mazin C. Merck M. Meucci M. Meyer J. M. Miranda R. Mirzoyan S. Mizobuchi A. Moralejo K. Nilsson J. Ninković E. de Ona Wilhelmi A. N. Otte I. Oya D. Paneque R. Paoletti J. M. Paredes M. Pasanen D. Pascoli Felicitas Pauss R. Pegna M. Peršić L. Peruzzo A. Piccioli M. Pöller N. Puchades E. Prandini A. Raymers W. Rhode M. Ribó J. Rico M. Rissi A. Robert S. Rügamer A. Saggion Alejandro Sánchez P. Sartori V. Scalzotto V. Scapin R. Schmitt T. Schweizer M. Shayduk K. Shinozaki Steven N. Shore N. Sidro A. Sillanpaa D. Sobczyńska A. Stamerra L. S. Stark L. O. Takalo P. Temnikov D. Tescaro M. Teshima N. Tonello D. F. Torres N. Turini H. Vankov V. Vitale R. M. Wagner T. Wibig W. Wittek R. Zanin J. Zapatero published in 2007. It has an Open Access status of “bronze”. You can read and download a PDF Full Text of this paper here.