WFRF:(Bosch J)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 07555naa a2202125 4500 | |
| 001 | oai:DiVA.org:su-51479 | |
| 003 | SwePub | |
| 008 | 110110s2010 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-514792 URI |
| 024 | 7 | a https://doi.org/10.1088/2041-8205/723/2/L2072 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Aleksic, J.4 aut |
| 245 | 1 0 | a DETECTION OF VERY HIGH ENERGY gamma-RAY EMISSION FROM THE PERSEUS CLUSTER HEAD-TAIL GALAXY IC 310 BY THE MAGIC TELESCOPES |
| 264 | 1 | c 2010 |
| 338 | a print2 rdacarrier | |
| 500 | a authorCount :153 | |
| 520 | a We report on the detection with the MAGIC telescopes of very high energy (VHE) gamma-rays from IC 310, a head-tail radio galaxy in the Perseus galaxy cluster, observed during the interval 2008 November to 2010 February. The Fermi satellite has also detected this galaxy. The source is detected by MAGIC at a high statistical significance of 7.6 sigma in 20.6 hr of stereo data. The observed spectral energy distribution is flat with a differential spectral index of -2.00 +/- 0.14. The mean flux above 300 GeV, between 2009 October and 2010 February, (3.1 +/- 0.5) x 10(-12) cm(-2) s(-1), corresponds to (2.5 +/- 0.4)% of Crab Nebula units. Only an upper limit, of 1.9% of Crab Nebula units above 300 GeV, was obtained with the 2008 data. This, together with strong hints (>3 sigma) of flares in the middle of 2009 October and November, implies that the emission is variable. The MAGIC results favor a scenario with the VHE emission originating from the inner jet close to the central engine. More complicated models than a simple one-zone synchrotron self-Compton (SSC) scenario, e. g., multi-zone SSC, external Compton, or hadronic, may be required to explain the very flat spectrum and its extension over more than three orders of magnitude in energy. | |
| 653 | a galaxies: active | |
| 653 | a galaxies: individual (IC 310) | |
| 653 | a gamma rays: galaxies | |
| 700 | 1 | a Antonelli, L. A.4 aut |
| 700 | 1 | a Antoranz, P.4 aut |
| 700 | 1 | a Backes, M.4 aut |
| 700 | 1 | a Barrio, J. A.4 aut |
| 700 | 1 | a Bastieri, D.4 aut |
| 700 | 1 | a Becerra Gonzalez, J.4 aut |
| 700 | 1 | a Bednarek, W.4 aut |
| 700 | 1 | a Berdyugin, A.4 aut |
| 700 | 1 | a Berger, K.4 aut |
| 700 | 1 | a Bernardini, E.4 aut |
| 700 | 1 | a Biland, A.4 aut |
| 700 | 1 | a Blanch, O.4 aut |
| 700 | 1 | a Bock, R. K.4 aut |
| 700 | 1 | a Boller, A.4 aut |
| 700 | 1 | a Bonnoli, G.4 aut |
| 700 | 1 | a Bordas, P.4 aut |
| 700 | 1 | a Tridon, D. Borla4 aut |
| 700 | 1 | a Bosch-Ramon, V.4 aut |
| 700 | 1 | a Bose, D.4 aut |
| 700 | 1 | a Braun, I.4 aut |
| 700 | 1 | a Bretz, T.4 aut |
| 700 | 1 | a Camara, M.4 aut |
| 700 | 1 | a Canellas, A.4 aut |
| 700 | 1 | a Carmona, E.4 aut |
| 700 | 1 | a Carosi, A.4 aut |
| 700 | 1 | a Colin, P.4 aut |
| 700 | 1 | a Colombo, E.4 aut |
| 700 | 1 | a Contreras, J. L.4 aut |
| 700 | 1 | a Cortina, J.4 aut |
| 700 | 1 | a Cossio, L.4 aut |
| 700 | 1 | a Covino, S.4 aut |
| 700 | 1 | a Dazzi, F.4 aut |
| 700 | 1 | a De Angelis, A.4 aut |
| 700 | 1 | a De Cea del Pozo, E.4 aut |
| 700 | 1 | a De Lotto, B.4 aut |
| 700 | 1 | a De Maria, M.4 aut |
| 700 | 1 | a De Sabata, F.4 aut |
| 700 | 1 | a Delgado Mendez, C.4 aut |
| 700 | 1 | a Diago Ortega, A.4 aut |
| 700 | 1 | a Doert, M.4 aut |
| 700 | 1 | a Dominguez, A.4 aut |
| 700 | 1 | a Prester, D. Dominis4 aut |
| 700 | 1 | a Dorner, D.4 aut |
| 700 | 1 | a Doro, M.4 aut |
| 700 | 1 | a Elsaesser, D.4 aut |
| 700 | 1 | a Errando, M.4 aut |
| 700 | 1 | a Ferenc, D.4 aut |
| 700 | 1 | a Fonseca, M. V.4 aut |
| 700 | 1 | a Font, L.4 aut |
| 700 | 1 | a Garcia Lopez, R. J.4 aut |
| 700 | 1 | a Garczarczyk, M.4 aut |
| 700 | 1 | a Giavitto, G.4 aut |
| 700 | 1 | a Godinovic, N.4 aut |
| 700 | 1 | a Hadasch, D.4 aut |
| 700 | 1 | a Herrero, A.4 aut |
| 700 | 1 | a Hildebrand, D.4 aut |
| 700 | 1 | a Hoehne-Moench, D.4 aut |
| 700 | 1 | a Hose, J.4 aut |
| 700 | 1 | a Hrupec, D.4 aut |
| 700 | 1 | a Jogler, T.4 aut |
| 700 | 1 | a Klepser, S.4 aut |
| 700 | 1 | a Kraehenbuehl, T.4 aut |
| 700 | 1 | a Kranich, D.4 aut |
| 700 | 1 | a Krause, J.4 aut |
| 700 | 1 | a La Barbera, A.4 aut |
| 700 | 1 | a Leonardo, E.4 aut |
| 700 | 1 | a Lindfors, E.4 aut |
| 700 | 1 | a Lombardi, S.4 aut |
| 700 | 1 | a Longo, F.4 aut |
| 700 | 1 | a Lopez, M.4 aut |
| 700 | 1 | a Lorenz, E.4 aut |
| 700 | 1 | a Majumdar, P.4 aut |
| 700 | 1 | a Makariev, M.4 aut |
| 700 | 1 | a Maneva, G.4 aut |
| 700 | 1 | a Mankuzhiyil, N.4 aut |
| 700 | 1 | a Mannheim, K.4 aut |
| 700 | 1 | a Maraschi, L.4 aut |
| 700 | 1 | a Mariotti, M.4 aut |
| 700 | 1 | a Martinez, M.4 aut |
| 700 | 1 | a Mazin, D.4 aut |
| 700 | 1 | a Meucci, M.4 aut |
| 700 | 1 | a Miranda, J. M.4 aut |
| 700 | 1 | a Mirzoyan, R.4 aut |
| 700 | 1 | a Miyamoto, H.4 aut |
| 700 | 1 | a Moldon, J.4 aut |
| 700 | 1 | a Moralejo, A.4 aut |
| 700 | 1 | a Nieto, D.4 aut |
| 700 | 1 | a Nilsson, K.4 aut |
| 700 | 1 | a Orito, R.4 aut |
| 700 | 1 | a Oya, I.4 aut |
| 700 | 1 | a Paoletti, R.4 aut |
| 700 | 1 | a Paredes, J. M.4 aut |
| 700 | 1 | a Partini, S.4 aut |
| 700 | 1 | a Pasanen, M.4 aut |
| 700 | 1 | a Pauss, F.4 aut |
| 700 | 1 | a Pegna, R. G.4 aut |
| 700 | 1 | a Perez-Torres, M. A.4 aut |
| 700 | 1 | a Persic, M.4 aut |
| 700 | 1 | a Peruzzo, L.4 aut |
| 700 | 1 | a Pochon, J.4 aut |
| 700 | 1 | a Prada, F.4 aut |
| 700 | 1 | a Moroni, P. G. Prada4 aut |
| 700 | 1 | a Prandini, E.4 aut |
| 700 | 1 | a Puchades, N.4 aut |
| 700 | 1 | a Puljak, I.4 aut |
| 700 | 1 | a Reichardt, I.4 aut |
| 700 | 1 | a Reinthal, R.4 aut |
| 700 | 1 | a Rhode, W.4 aut |
| 700 | 1 | a Ribo, M.4 aut |
| 700 | 1 | a Rico, J.4 aut |
| 700 | 1 | a Ruegamer, S.4 aut |
| 700 | 1 | a Saggion, A.4 aut |
| 700 | 1 | a Saito, K.4 aut |
| 700 | 1 | a Saito, T. Y.4 aut |
| 700 | 1 | a Salvati, M.4 aut |
| 700 | 1 | a Sanchez-Conde, M.4 aut |
| 700 | 1 | a Satalecka, K.4 aut |
| 700 | 1 | a Scalzotto, V.4 aut |
| 700 | 1 | a Scapin, V.4 aut |
| 700 | 1 | a Schultz, C.4 aut |
| 700 | 1 | a Schweizer, T.4 aut |
| 700 | 1 | a Shayduk, M.4 aut |
| 700 | 1 | a Shore, S. N.4 aut |
| 700 | 1 | a Sierpowska-Bartosik, A.4 aut |
| 700 | 1 | a Sillanpaa, A.4 aut |
| 700 | 1 | a Sitarek, J.4 aut |
| 700 | 1 | a Sobczynska, D.4 aut |
| 700 | 1 | a Spanier, F.4 aut |
| 700 | 1 | a Spiro, S.4 aut |
| 700 | 1 | a Stamerra, A.4 aut |
| 700 | 1 | a Steinke, B.4 aut |
| 700 | 1 | a Storz, J.4 aut |
| 700 | 1 | a Strah, N.4 aut |
| 700 | 1 | a Struebig, J. C.4 aut |
| 700 | 1 | a Suric, T.4 aut |
| 700 | 1 | a Takalo, L.4 aut |
| 700 | 1 | a Tavecchio, F.4 aut |
| 700 | 1 | a Temnikov, P.4 aut |
| 700 | 1 | a Terzic, T.4 aut |
| 700 | 1 | a Tescaro, D.4 aut |
| 700 | 1 | a Teshima, M.4 aut |
| 700 | 1 | a Torres, D. F.4 aut |
| 700 | 1 | a Vankov, H.4 aut |
| 700 | 1 | a Wagner, R. M.4 aut |
| 700 | 1 | a Weitzel, Q.4 aut |
| 700 | 1 | a Zabalza, V.4 aut |
| 700 | 1 | a Zandanel, F.4 aut |
| 700 | 1 | a Zanin, R.4 aut |
| 700 | 1 | a Neronov, A.4 aut |
| 700 | 1 | a Pfrommer, C.4 aut |
| 700 | 1 | a Pinzke, Andersu Stockholms universitet,Fysikum4 aut0 (Swepub:su)apinzke |
| 700 | 1 | a Semikoz, D. V.4 aut |
| 710 | 2 | a Stockholms universitetb Fysikum4 org |
| 773 | 0 | t The Astrophysical Journal Lettersg 723:2, s. l207-L212q 723:2<l207-L212x 2041-8205 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-51479 |
| 856 | 4 8 | u https://doi.org/10.1088/2041-8205/723/2/L207 |
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- Miyamoto, H.
- Moldon, J.
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- Nieto, D.
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- Orito, R.
- Oya, I.
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