A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä

Detection of bridge emission above 50 GeV from the Crab pulsar with the MAGIC telescopes




TekijätAleksic J, Ansoldi S, Antonelli LA, Antoranz P, Babic A, Bangale P, de Almeida UB, Barrio JA, Gonzalez JB, Bednarek W, Bernardini E, Biasuzzi B, Biland A, Blanch O, Bonnefoy S, Bonnoli G, Borracci F, Bretz T, Carmona E, Carosi A, Colin P, Colombos E, Contreras JL, Cortina J, Covino S, Da Vela P, Dazzi E, De Angelis A, De Caneva G, De Lotto B, Mendez CCD, Doert M, Prester DD, Dorner D, Doro M, Einecke S, Eisenacher D, Elsaesser D, Farina E, Ferenc D, Fidalgo D, Fonseca MV, Font L, Frantzen K, Fruck C, Lopez RJG, Garczarczyk M, Terrats DG, Gaug M, Godinovic N, Munoz AG, Gozzini SR, Hadasch D, Hayashida M, Herrera J, Herrero A, Hildebrand D, Hirotani K, Hose J, Hrupec D, Idec W, Kadenius V, Kellermann H, Kodani K, Konno Y, Krause J, Kubo H, Kushida J, La Barbera A, Lelas D, Lewandowska N, Lindfors E, Lombardi S, Lopez M, Lopez-Coto R, Lopez-Oramas A, Lorenz E, Lozano I, Makariev M, Mallot K, Maneva G, Mankuzhiyil N, Mannheim K, Maraschi L, Marcote B, Mariotti M, Martinez M, Mazin D, Menzel U, Miranda JM, Mirzoyan R, Moralejo A, Munar-Adrover P, Nakajima D, Niedzwiecki A, Nilsson K, Nishijima K, Noda K, Nowak N, Orito R, Overkemping A, Paiano S, Palatiello M, Paneque D, Paoletti R, Paredes JM, Paredes-Fortuny X, Partini S, Persic M, Moroni PGP, Prandini E, Preziuso S, Puljak I, Reinthal R, Rhode W, Ribo M, Rico J, Garcia JR, Rugamer S, Saggion A, Saito TY, Saito K, Satalecka K, Scalzotto V, Scapin V, Schultz C, Schweizer T, Shore SN, Sillanpaa A, Sitarek J, Snidaric I, Sobczynska D, Spanier E, Stamatescu V, Stamerra A, Steinbring T, Storz M, Strzys M, Sun S, Suric T, Takalo L, Takami H, Tavecchio F, Temnikov P, Terzic T, Tescaro D, Teshima M, Thaele J, Tibolla O, Forres DE, Toyama T, Treves A, Uellenbeck M, Vogler P, Wagner RM, Zanin R

KustantajaEDP Sciences S A

Julkaisuvuosi2014

JournalAstronomy and Astrophysics

Tietokannassa oleva lehden nimiASTRONOMY & ASTROPHYSICS

Lehden akronyymiAstron astrophys

Artikkelin numeroL12

Vuosikerta565

Sivujen määrä5

ISSN0004-6361

DOIhttps://doi.org/10.1051/0004-6361/201423664


Tiivistelmä

Conclusions. We discovered the bridge emission above 50 GeV between the two main pulses. This emission can not be explained with the existing theories. These data can be used for testing new theoretical models.




Last updated on 2024-26-11 at 11:40