Very high-energy $\gamma $-ray observations of novae and dwarf novae with the MAGIC telescopes
- Ahnen, M. L.
- Ansoldi, S.
- Bednarek, W.
- Noda, K.
- Orito, R.
- Overkemping, A.
- Paiano, S.
- Palacio, J.
- Palatiello, M.
- Paneque, D.
- Paoletti, R.
- Paredes, J. M.
- Paredes-Fortuny, X.
- Bernardini, E.
- Persic, M.
- Poutanen, J.
- Prada Moroni, P. G.
- Prandini, E.
- Puljak, I.
- Reinthal, R.
- Rhode, W.
- Ribó, M.
- Rico, J.
- Rodriguez Garcia, J.
- Biasuzzi, B.
- Saito, T.
- Saito, K.
- Satalecka, K.
- Scapin, V.
- Schultz, C.
- Schweizer, T.
- Sillanpää, A.
- Sitarek, J.
- Snidaric, I.
- Sobczynska, D.
- Biland, A.
- Stamerra, A.
- Steinbring, T.
- Strzys, M.
- Takalo, L.
- Takami, H.
- Tavecchio, F.
- Temnikov, P.
- Terzić, T.
- Tescaro, D.
- Teshima, M.
- Blanch, O.
- Thaele, J.
- Torres, D. F.
- Toyama, T.
- Treves, A.
- Verguilov, V.
- Vovk, I.
- Will, M.
- Zanin, R.
- Desiante, R.
- Hays, E.
- Bonnefoy, S.
- Bonnoli, G.
- Borracci, F.
- Bretz, T.
- Carmona, E.
- Antonelli, L. A.
- Carosi, A.
- Chatterjee, A.
- Clavero, R.
- Colin, P.
- Colombo, E.
- Contreras, J. L.
- Cortina, J.
- Covino, S.
- Da Vela, P.
- Dazzi, F.
- Antoranz, P.
- De Angelis, A.
- De Caneva, G.
- De Lotto, B.
- de Oña Wilhelmi, E.
- Delgado Mendez, C.
- Di Pierro, F.
- Dominis Prester, D.
- Dorner, D.
- Doro, M.
- Einecke, S.
- Babic, A.
- Eisenacher Glawion, D.
- Elsaesser, D.
- Fernández-Barral, A.
- Fidalgo, D.
- Fonseca, M. V.
- Font, L.
- Frantzen, K.
- Fruck, C.
- Galindo, D.
- García López, R. J.
- Banerjee, B.
- Garczarczyk, M.
- Garrido Terrats, D.
- Gaug, M.
- Giammaria, P.
- Godinović, N.
- González Muñoz, A.
- Guberman, D.
- Hanabata, Y.
- Hayashida, M.
- Herrera, J.
- Bangale, P.
- Hose, J.
- Hrupec, D.
- Hughes, G.
- Idec, W.
- Kellermann, H.
- Kodani, K.
- Konno, Y.
- Kubo, H.
- Kushida, J.
- La Barbera, A.
- Barres de Almeida, U.
- Lelas, D.
- Lewandowska, N.
- Lindfors, E.
- Lombardi, S.
- Longo, F.
- López, M.
- López-Coto, R.
- López-Oramas, A.
- Lorenz, E.
- Majumdar, P.
- Barrio, J. A.
- Makariev, M.
- Mallot, K.
- Maneva, G.
- Manganaro, M.
- Mannheim, K.
- Maraschi, L.
- Marcote, B.
- Mariotti, M.
- Martínez, M.
- Mazin, D.
- Becerra González, J.
- Menzel, U.
- Miranda, J. M.
- Mirzoyan, R.
- Moralejo, A.
- Nakajima, D.
- Neustroev, V.
- Niedzwiecki, A.
- Nievas Rosillo, M.
- Nilsson, K.
- Nishijima, K.
DOIAbstract
In the last five years the Fermi Large Area Telescope (LAT) instrument detected GeV γ-ray emission from five novae. The GeV emission can be interpreted in terms of an inverse Compton process of electrons accelerated in a shock. In this case it is expected that protons in the same conditions can be accelerated to much higher energies. Consequently they may produce a second component in the γ-ray spectrum at TeV energies.Aims. We aim to explore the very high-energy domain to search for γ-ray emission above 50 GeV and to shed light on the acceleration process of leptons and hadrons in nova explosions.Methods. We have performed observations, with the MAGIC telescopes of the classical nova V339 Del shortly after the 2013 outburst; optical and su...
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