Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classe...
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Autor*in:	Acero, F. [verfasserIn] Acharyya, A. [verfasserIn] Adam, R. [verfasserIn] Aguasca-Cabot, A. [verfasserIn] Agudo, I. [verfasserIn] Aguirre-Santaella, A. [verfasserIn] Alfaro, J. [verfasserIn] Aloisio, R. [verfasserIn] Crespo, N. Álvarez [verfasserIn] Batista, R. Alves [verfasserIn] Amati, L. [verfasserIn] Amato, E. [verfasserIn] Ambrosi, G. [verfasserIn] Angüner, E.O. [verfasserIn] Aramo, C. [verfasserIn] Arcaro, C. [verfasserIn] Armstrong, T. [verfasserIn] Asano, K. [verfasserIn] Ascasibar, Y. [verfasserIn] Aschersleben, J. [verfasserIn] Backes, M. [verfasserIn] Baktash, A. [verfasserIn] Balazs, C. [verfasserIn] Balbo, M. [verfasserIn] Ballet, J. [verfasserIn] Larriva, A. Baquero [verfasserIn] Martins, V. Barbosa [verfasserIn] de Almeida, U. Barres [verfasserIn] Barrio, J.A. [verfasserIn] Bastieri, D. [verfasserIn] Baxter, J.R. [verfasserIn] Tjus, J. Becker [verfasserIn] Benbow, W. [verfasserIn] Bernardos-Martín, M.I. [verfasserIn] Bernete, J. [verfasserIn] Berti, A. [verfasserIn] Bertucci, B. [verfasserIn] Beshley, V. [verfasserIn] Bhattacharjee, P. [verfasserIn] Bhattacharyya, S. [verfasserIn] Biland, A. [verfasserIn] Bissaldi, E. [verfasserIn] Biteau, J. [verfasserIn] Blanch, O. [verfasserIn] Bordas, P. [verfasserIn] Bottacini, E. [verfasserIn] Bregeon, J. [verfasserIn] Brose, R. [verfasserIn] Bucciantini, N. [verfasserIn] Bulgarelli, A. [verfasserIn] Capasso, M. [verfasserIn] Dolcetta, R.A. Capuzzo [verfasserIn] Caraveo, P. [verfasserIn] Cardillo, M. [verfasserIn] Carosi, R. [verfasserIn] Casanova, S. [verfasserIn] Cascone, E. [verfasserIn] Cassol, F. [verfasserIn] Catalani, F. [verfasserIn] Cerruti, M. [verfasserIn] Chadwick, P. [verfasserIn] Chaty, S. [verfasserIn] Chen, A. [verfasserIn] Chernyakova, M. [verfasserIn] Chiavassa, A. [verfasserIn] Chudoba, J. [verfasserIn] Coimbra-Araujo, C. [verfasserIn] Conforti, V. [verfasserIn] Contreras, J.L. [verfasserIn] Costa, A. [verfasserIn] Costantini, H. [verfasserIn] Cristofari, P. [verfasserIn] Crocker, R. [verfasserIn] D’Amico, G. [verfasserIn] D’Ammando, F. [verfasserIn] De Angelis, A. [verfasserIn] De Caprio, V. [verfasserIn] de Gouveia Dal Pino, E.M. [verfasserIn] de Ona Wilhelmi, E. [verfasserIn] de Souza, V. [verfasserIn] Delgado, C. [verfasserIn] della Volpe, D. [verfasserIn] Depaoli, D. [verfasserIn] Di Girolamo, T. [verfasserIn] Di Pierro, F. [verfasserIn] Di Tria, R. [verfasserIn] Di Venere, L. [verfasserIn] Diebold, S. [verfasserIn] Djuvsland, J.I. [verfasserIn] Donini, A. [verfasserIn] Doro, M. [verfasserIn] Dos Anjos, R.d.C. [verfasserIn] Dwarkadas, V.V. [verfasserIn] Einecke, S. [verfasserIn] Elsässer, D. [verfasserIn] Emery, G. [verfasserIn] Evoli, C. [verfasserIn] Falceta-Goncalves, D. [verfasserIn] Fedorova, E. [verfasserIn] Fegan, S. [verfasserIn] Ferrand, G. [verfasserIn] Fiandrini, E. [verfasserIn] Filipovic, M. [verfasserIn] Fioretti, V. [verfasserIn] Fiori, M. [verfasserIn] Foffano, L. [verfasserIn] Fontaine, G. [verfasserIn] Fukami, S. [verfasserIn] Galanti, G. [verfasserIn] Galaz, G. [verfasserIn] Gammaldi, V. [verfasserIn] Gasbarra, C. [verfasserIn] Ghalumyan, A. [verfasserIn] Ghirlanda, G. [verfasserIn] Giarrusso, M. [verfasserIn] Giavitto, G. [verfasserIn] Giglietto, N. [verfasserIn] Giordano, F. [verfasserIn] Giroletti, M. [verfasserIn] Giuliani, A. [verfasserIn] Giunti, L. [verfasserIn] Godinovic, N. [verfasserIn] Coelho, J. Goulart [verfasserIn] Gréaux, L. [verfasserIn] Green, D. [verfasserIn] Grondin, M.-H. [verfasserIn] Gueta, O. [verfasserIn] Gunji, S. [verfasserIn] Hassan, T. [verfasserIn] Heller, M. [verfasserIn] Hernández-Cadena, S. [verfasserIn] Hinton, J. [verfasserIn] Hnatyk, B. [verfasserIn] Hnatyk, R. [verfasserIn] Hoffmann, D. [verfasserIn] Hofmann, W. [verfasserIn] Holder, J. [verfasserIn] Horan, D. [verfasserIn] Horvath, P. [verfasserIn] Hrabovsky, M. [verfasserIn] Hrupec, D. [verfasserIn] Inada, T. [verfasserIn] Incardona, F. [verfasserIn] Inoue, S. [verfasserIn] Ishio, K. [verfasserIn] Jamrozy, M. [verfasserIn] Janecek, P. [verfasserIn] Martínez, I. Jiménez [verfasserIn] Jin, W. [verfasserIn] Jung-Richardt, I. [verfasserIn] Jurysek, J. [verfasserIn] Kaaret, P. [verfasserIn] Karas, V. [verfasserIn] Katz, U. [verfasserIn] Kerszberg, D. [verfasserIn] Khélifi, B. [verfasserIn] Kieda, D.B. [verfasserIn] Kissmann, R. [verfasserIn] Kleiner, T. [verfasserIn] Kluge, G. [verfasserIn] Kluzniak, W. [verfasserIn] Knödlseder, J. [verfasserIn] Kobayashi, Y. [verfasserIn] Kohri, K. [verfasserIn] Komin, N. [verfasserIn] Kornecki, P. [verfasserIn] Kubo, H. [verfasserIn] La Palombara, N. [verfasserIn] Láinez, M. [verfasserIn] Lamastra, A. [verfasserIn] Lapington, J. [verfasserIn] Lemoine-Goumard, M. [verfasserIn] Lenain, J.-P. [verfasserIn] Leone, F. [verfasserIn] Leto, G. [verfasserIn] Leuschner, F. [verfasserIn] Lindfors, E. [verfasserIn] Liodakis, I. [verfasserIn] Lohse, T. [verfasserIn] Lombardi, S. [verfasserIn] Longo, F. [verfasserIn] López-Coto, R. [verfasserIn] López-Moya, M. [verfasserIn] López-Oramas, A. [verfasserIn] Loporchio, S. [verfasserIn] Luque-Escamilla, P.L. [verfasserIn] Macias, O. [verfasserIn] Mackey, J. [verfasserIn] Majumdar, P. [verfasserIn] Mandat, D. [verfasserIn] Manganaro, M. [verfasserIn] Manicò, G. [verfasserIn] Marconi, M. [verfasserIn] Martí, J. [verfasserIn] Martínez, G. [verfasserIn] Martinez, M. [verfasserIn] Martinez, O. [verfasserIn] Mello, A.J.T.S. [verfasserIn] Menchiari, S. [verfasserIn] Meyer, D.M.-A. [verfasserIn] Micanovic, S. [verfasserIn] Miceli, D. [verfasserIn] Miceli, M. [verfasserIn] Michalowski, J. [verfasserIn] Miener, T. [verfasserIn] Miranda, J.M. [verfasserIn] Mitchell, A. [verfasserIn] Mode, B. [verfasserIn] Moderski, R. [verfasserIn] Mohrmann, L. [verfasserIn] Molina, E. [verfasserIn] Montaruli, T. [verfasserIn] Morcuende, D. [verfasserIn] Morlino, G. [verfasserIn] Morselli, A. [verfasserIn] Mosè, M. [verfasserIn] Moulin, E. [verfasserIn] Mukherjee, R. [verfasserIn] Munari, K. [verfasserIn] Murach, T. [verfasserIn] Nagai, A. [verfasserIn] Nagataki, S. [verfasserIn] Nemmen, R. [verfasserIn] Niemiec, J. [verfasserIn] Nieto, D. [verfasserIn] Rosillo, M. Nievas [verfasserIn] Nikolajuk, M. [verfasserIn] Nishijima, K. [verfasserIn] Noda, K. [verfasserIn] Novosyadlyj, B. [verfasserIn] Nozaki, S. [verfasserIn] Ohishi, M. [verfasserIn] Ohm, S. [verfasserIn] Ohtani, Y. [verfasserIn] Okumura, A. [verfasserIn] Olmi, B. [verfasserIn] Ong, R.A. [verfasserIn] Orienti, M. [verfasserIn] Orito, R. [verfasserIn] Orlandini, M. [verfasserIn] Orlando, E. [verfasserIn] Orlando, S. [verfasserIn] Ostrowski, M. [verfasserIn] Oya, I. [verfasserIn] Pantaleo, F.R. [verfasserIn] Paredes, J.M. [verfasserIn] Patricelli, B. [verfasserIn] Pecimotika, M. [verfasserIn] Peresano, M. [verfasserIn] Pérez-Romero, J. [verfasserIn] Persic, M. [verfasserIn] Petruk, O. [verfasserIn] Piano, G. [verfasserIn] Pietropaolo, E. [verfasserIn] Pirola, G. [verfasserIn] Pittori, C. [verfasserIn] Pohl, M. [verfasserIn] Ponti, G. [verfasserIn] Prandini, E. [verfasserIn] Principe, G. [verfasserIn] Priyadarshi, C. [verfasserIn] Pueschel, E. [verfasserIn] Pühlhofer, G. [verfasserIn] Pumo, M.L. [verfasserIn] Quirrenbach, A. [verfasserIn] Rando, R. [verfasserIn] Razzaque, S. [verfasserIn] Reichherzer, P. [verfasserIn] Reimer, A. [verfasserIn] Reimer, O. [verfasserIn] Renaud, M. [verfasserIn] Reposeur, T. [verfasserIn] Ribó, M. [verfasserIn] Richtler, T. [verfasserIn] Rico, J. [verfasserIn] Rieger, F. [verfasserIn] Rigoselli, M. [verfasserIn] Riitano, L. [verfasserIn] Rizi, V. [verfasserIn] Roache, E. [verfasserIn] Romano, P. [verfasserIn] Romeo, G. [verfasserIn] Rosado, J. [verfasserIn] Rowell, G. [verfasserIn] Rudak, B. [verfasserIn] Sadeh, I. [verfasserIn] Safi-Harb, S. [verfasserIn] Saha, L. [verfasserIn] Sailer, S. [verfasserIn] Sánchez-Conde, M. [verfasserIn] Sarkar, S. [verfasserIn] Satalecka, K. [verfasserIn] Saturni, F.G. [verfasserIn] Scherer, A. [verfasserIn] Schovánek, P. [verfasserIn] Schussler, F. [verfasserIn] Schwanke, U. [verfasserIn] Scuderi, S. [verfasserIn] Seglar-Arroyo, M. [verfasserIn] Sergijenko, O. [verfasserIn] Servillat, M. [verfasserIn] Shang, R.-Y. [verfasserIn] Sharma, P. [verfasserIn] Siejkowski, H. [verfasserIn] Sliusar, V. [verfasserIn] Słowikowska, A. [verfasserIn] Sol, H. [verfasserIn] Specovius, A. [verfasserIn] Spencer, S.T. [verfasserIn] Spengler, G. [verfasserIn] Stamerra, A. [verfasserIn] Stanič, S. [verfasserIn] Starecki, T. [verfasserIn] Starling, R. [verfasserIn] Stolarczyk, T. [verfasserIn] Pereira, L.A. Stuani [verfasserIn] Suda, Y. [verfasserIn] Suomijarvi, T. [verfasserIn] Sushch, I. [verfasserIn] Tajima, H. [verfasserIn] Tam, P.-H.T. [verfasserIn] Tanaka, S.J. [verfasserIn] Tavecchio, F. [verfasserIn] Testa, V. [verfasserIn] Tian, W. [verfasserIn] Tibaldo, L. [verfasserIn] Torres, D.F. [verfasserIn] Tothill, N. [verfasserIn] Vallage, B. [verfasserIn] Vallania, P. [verfasserIn] van Eldik, C. [verfasserIn] van Scherpenberg, J. [verfasserIn] Vandenbroucke, J. [verfasserIn] Acosta, M. Vazquez [verfasserIn] Vecchi, M. [verfasserIn] Vercellone, S. [verfasserIn] Verna, G. [verfasserIn] Viana, A. [verfasserIn] Vignatti, J. [verfasserIn] Vitale, V. [verfasserIn] Vodeb, V. [verfasserIn] Vorobiov, S. [verfasserIn] Vuillaume, T. [verfasserIn] Wagner, S.J. [verfasserIn] Walter, R. [verfasserIn] White, M. [verfasserIn] Wierzcholska, A. [verfasserIn] Will, M. [verfasserIn] Williams, D. [verfasserIn] Yang, L. [verfasserIn] Yoshida, T. [verfasserIn] Yoshikoshi, T. [verfasserIn] Zaharijas, G. [verfasserIn] Zampieri, L. [verfasserIn] Zavrtanik, D. [verfasserIn] Zavrtanik, M. [verfasserIn] Zhdanov, V.I. [verfasserIn] Z̆ivec, M. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	Gamma rays: general Cosmic rays Galactic PeVatrons (Stars:) supernovae: general Methods: data analysis Methods: statistical

Übergeordnetes Werk:	Enthalten in: Astroparticle physics - Amsterdam [u.a.] : Elsevier Science, 1992, 150
Übergeordnetes Werk:	volume:150

DOI / URN:	10.1016/j.astropartphys.2023.102850

Katalog-ID:	ELV009642641

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024	7		\|a 10.1016/j.astropartphys.2023.102850 \|2 doi
035			\|a (DE-627)ELV009642641
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100	1		\|a Acero, F. \|e verfasserin \|4 aut
245	1	0	\|a Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
264		1	\|c 2023
336			\|a nicht spezifiziert \|b zzz \|2 rdacontent
337			\|a Computermedien \|b c \|2 rdamedia
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520			\|a The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source.
650		4	\|a Gamma rays: general
650		4	\|a Cosmic rays
650		4	\|a Galactic PeVatrons
650		4	\|a (Stars:) supernovae: general
650		4	\|a Methods: data analysis
650		4	\|a Methods: statistical
700	1		\|a Acharyya, A. \|e verfasserin \|4 aut
700	1		\|a Adam, R. \|e verfasserin \|4 aut
700	1		\|a Aguasca-Cabot, A. \|e verfasserin \|4 aut
700	1		\|a Agudo, I. \|e verfasserin \|4 aut
700	1		\|a Aguirre-Santaella, A. \|e verfasserin \|4 aut
700	1		\|a Alfaro, J. \|e verfasserin \|4 aut
700	1		\|a Aloisio, R. \|e verfasserin \|4 aut
700	1		\|a Crespo, N. Álvarez \|e verfasserin \|4 aut
700	1		\|a Batista, R. Alves \|e verfasserin \|4 aut
700	1		\|a Amati, L. \|e verfasserin \|4 aut
700	1		\|a Amato, E. \|e verfasserin \|4 aut
700	1		\|a Ambrosi, G. \|e verfasserin \|4 aut
700	1		\|a Angüner, E.O. \|e verfasserin \|4 aut
700	1		\|a Aramo, C. \|e verfasserin \|4 aut
700	1		\|a Arcaro, C. \|e verfasserin \|4 aut
700	1		\|a Armstrong, T. \|e verfasserin \|4 aut
700	1		\|a Asano, K. \|e verfasserin \|4 aut
700	1		\|a Ascasibar, Y. \|e verfasserin \|4 aut
700	1		\|a Aschersleben, J. \|e verfasserin \|4 aut
700	1		\|a Backes, M. \|e verfasserin \|4 aut
700	1		\|a Baktash, A. \|e verfasserin \|4 aut
700	1		\|a Balazs, C. \|e verfasserin \|4 aut
700	1		\|a Balbo, M. \|e verfasserin \|4 aut
700	1		\|a Ballet, J. \|e verfasserin \|4 aut
700	1		\|a Larriva, A. Baquero \|e verfasserin \|4 aut
700	1		\|a Martins, V. Barbosa \|e verfasserin \|4 aut
700	1		\|a de Almeida, U. Barres \|e verfasserin \|4 aut
700	1		\|a Barrio, J.A. \|e verfasserin \|4 aut
700	1		\|a Bastieri, D. \|e verfasserin \|4 aut
700	1		\|a Baxter, J.R. \|e verfasserin \|4 aut
700	1		\|a Tjus, J. Becker \|e verfasserin \|4 aut
700	1		\|a Benbow, W. \|e verfasserin \|4 aut
700	1		\|a Bernardos-Martín, M.I. \|e verfasserin \|4 aut
700	1		\|a Bernete, J. \|e verfasserin \|4 aut
700	1		\|a Berti, A. \|e verfasserin \|4 aut
700	1		\|a Bertucci, B. \|e verfasserin \|4 aut
700	1		\|a Beshley, V. \|e verfasserin \|4 aut
700	1		\|a Bhattacharjee, P. \|e verfasserin \|4 aut
700	1		\|a Bhattacharyya, S. \|e verfasserin \|4 aut
700	1		\|a Biland, A. \|e verfasserin \|4 aut
700	1		\|a Bissaldi, E. \|e verfasserin \|4 aut
700	1		\|a Biteau, J. \|e verfasserin \|4 aut
700	1		\|a Blanch, O. \|e verfasserin \|4 aut
700	1		\|a Bordas, P. \|e verfasserin \|4 aut
700	1		\|a Bottacini, E. \|e verfasserin \|4 aut
700	1		\|a Bregeon, J. \|e verfasserin \|4 aut
700	1		\|a Brose, R. \|e verfasserin \|4 aut
700	1		\|a Bucciantini, N. \|e verfasserin \|4 aut
700	1		\|a Bulgarelli, A. \|e verfasserin \|4 aut
700	1		\|a Capasso, M. \|e verfasserin \|4 aut
700	1		\|a Dolcetta, R.A. Capuzzo \|e verfasserin \|4 aut
700	1		\|a Caraveo, P. \|e verfasserin \|4 aut
700	1		\|a Cardillo, M. \|e verfasserin \|4 aut
700	1		\|a Carosi, R. \|e verfasserin \|4 aut
700	1		\|a Casanova, S. \|e verfasserin \|4 aut
700	1		\|a Cascone, E. \|e verfasserin \|4 aut
700	1		\|a Cassol, F. \|e verfasserin \|4 aut
700	1		\|a Catalani, F. \|e verfasserin \|4 aut
700	1		\|a Cerruti, M. \|e verfasserin \|4 aut
700	1		\|a Chadwick, P. \|e verfasserin \|4 aut
700	1		\|a Chaty, S. \|e verfasserin \|4 aut
700	1		\|a Chen, A. \|e verfasserin \|4 aut
700	1		\|a Chernyakova, M. \|e verfasserin \|4 aut
700	1		\|a Chiavassa, A. \|e verfasserin \|4 aut
700	1		\|a Chudoba, J. \|e verfasserin \|4 aut
700	1		\|a Coimbra-Araujo, C. \|e verfasserin \|4 aut
700	1		\|a Conforti, V. \|e verfasserin \|4 aut
700	1		\|a Contreras, J.L. \|e verfasserin \|4 aut
700	1		\|a Costa, A. \|e verfasserin \|4 aut
700	1		\|a Costantini, H. \|e verfasserin \|4 aut
700	1		\|a Cristofari, P. \|e verfasserin \|4 aut
700	1		\|a Crocker, R. \|e verfasserin \|4 aut
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700	1		\|a De Angelis, A. \|e verfasserin \|4 aut
700	1		\|a De Caprio, V. \|e verfasserin \|4 aut
700	1		\|a de Gouveia Dal Pino, E.M. \|e verfasserin \|4 aut
700	1		\|a de Ona Wilhelmi, E. \|e verfasserin \|4 aut
700	1		\|a de Souza, V. \|e verfasserin \|4 aut
700	1		\|a Delgado, C. \|e verfasserin \|4 aut
700	1		\|a della Volpe, D. \|e verfasserin \|4 aut
700	1		\|a Depaoli, D. \|e verfasserin \|4 aut
700	1		\|a Di Girolamo, T. \|e verfasserin \|4 aut
700	1		\|a Di Pierro, F. \|e verfasserin \|4 aut
700	1		\|a Di Tria, R. \|e verfasserin \|4 aut
700	1		\|a Di Venere, L. \|e verfasserin \|4 aut
700	1		\|a Diebold, S. \|e verfasserin \|4 aut
700	1		\|a Djuvsland, J.I. \|e verfasserin \|4 aut
700	1		\|a Donini, A. \|e verfasserin \|4 aut
700	1		\|a Doro, M. \|e verfasserin \|4 aut
700	1		\|a Dos Anjos, R.d.C. \|e verfasserin \|4 aut
700	1		\|a Dwarkadas, V.V. \|e verfasserin \|4 aut
700	1		\|a Einecke, S. \|e verfasserin \|4 aut
700	1		\|a Elsässer, D. \|e verfasserin \|4 aut
700	1		\|a Emery, G. \|e verfasserin \|4 aut
700	1		\|a Evoli, C. \|e verfasserin \|4 aut
700	1		\|a Falceta-Goncalves, D. \|e verfasserin \|4 aut
700	1		\|a Fedorova, E. \|e verfasserin \|4 aut
700	1		\|a Fegan, S. \|e verfasserin \|4 aut
700	1		\|a Ferrand, G. \|e verfasserin \|4 aut
700	1		\|a Fiandrini, E. \|e verfasserin \|4 aut
700	1		\|a Filipovic, M. \|e verfasserin \|4 aut
700	1		\|a Fioretti, V. \|e verfasserin \|4 aut
700	1		\|a Fiori, M. \|e verfasserin \|4 aut
700	1		\|a Foffano, L. \|e verfasserin \|4 aut
700	1		\|a Fontaine, G. \|e verfasserin \|4 aut
700	1		\|a Fukami, S. \|e verfasserin \|4 aut
700	1		\|a Galanti, G. \|e verfasserin \|4 aut
700	1		\|a Galaz, G. \|e verfasserin \|4 aut
700	1		\|a Gammaldi, V. \|e verfasserin \|4 aut
700	1		\|a Gasbarra, C. \|e verfasserin \|4 aut
700	1		\|a Ghalumyan, A. \|e verfasserin \|4 aut
700	1		\|a Ghirlanda, G. \|e verfasserin \|4 aut
700	1		\|a Giarrusso, M. \|e verfasserin \|4 aut
700	1		\|a Giavitto, G. \|e verfasserin \|4 aut
700	1		\|a Giglietto, N. \|e verfasserin \|4 aut
700	1		\|a Giordano, F. \|e verfasserin \|4 aut
700	1		\|a Giroletti, M. \|e verfasserin \|4 aut
700	1		\|a Giuliani, A. \|e verfasserin \|4 aut
700	1		\|a Giunti, L. \|e verfasserin \|4 aut
700	1		\|a Godinovic, N. \|e verfasserin \|4 aut
700	1		\|a Coelho, J. Goulart \|e verfasserin \|4 aut
700	1		\|a Gréaux, L. \|e verfasserin \|4 aut
700	1		\|a Green, D. \|e verfasserin \|4 aut
700	1		\|a Grondin, M.-H. \|e verfasserin \|4 aut
700	1		\|a Gueta, O. \|e verfasserin \|4 aut
700	1		\|a Gunji, S. \|e verfasserin \|4 aut
700	1		\|a Hassan, T. \|e verfasserin \|4 aut
700	1		\|a Heller, M. \|e verfasserin \|4 aut
700	1		\|a Hernández-Cadena, S. \|e verfasserin \|4 aut
700	1		\|a Hinton, J. \|e verfasserin \|4 aut
700	1		\|a Hnatyk, B. \|e verfasserin \|4 aut
700	1		\|a Hnatyk, R. \|e verfasserin \|4 aut
700	1		\|a Hoffmann, D. \|e verfasserin \|4 aut
700	1		\|a Hofmann, W. \|e verfasserin \|4 aut
700	1		\|a Holder, J. \|e verfasserin \|4 aut
700	1		\|a Horan, D. \|e verfasserin \|4 aut
700	1		\|a Horvath, P. \|e verfasserin \|4 aut
700	1		\|a Hrabovsky, M. \|e verfasserin \|4 aut
700	1		\|a Hrupec, D. \|e verfasserin \|4 aut
700	1		\|a Inada, T. \|e verfasserin \|4 aut
700	1		\|a Incardona, F. \|e verfasserin \|4 aut
700	1		\|a Inoue, S. \|e verfasserin \|4 aut
700	1		\|a Ishio, K. \|e verfasserin \|4 aut
700	1		\|a Jamrozy, M. \|e verfasserin \|4 aut
700	1		\|a Janecek, P. \|e verfasserin \|4 aut
700	1		\|a Martínez, I. Jiménez \|e verfasserin \|4 aut
700	1		\|a Jin, W. \|e verfasserin \|4 aut
700	1		\|a Jung-Richardt, I. \|e verfasserin \|4 aut
700	1		\|a Jurysek, J. \|e verfasserin \|4 aut
700	1		\|a Kaaret, P. \|e verfasserin \|4 aut
700	1		\|a Karas, V. \|e verfasserin \|4 aut
700	1		\|a Katz, U. \|e verfasserin \|4 aut
700	1		\|a Kerszberg, D. \|e verfasserin \|4 aut
700	1		\|a Khélifi, B. \|e verfasserin \|4 aut
700	1		\|a Kieda, D.B. \|e verfasserin \|4 aut
700	1		\|a Kissmann, R. \|e verfasserin \|4 aut
700	1		\|a Kleiner, T. \|e verfasserin \|4 aut
700	1		\|a Kluge, G. \|e verfasserin \|4 aut
700	1		\|a Kluzniak, W. \|e verfasserin \|4 aut
700	1		\|a Knödlseder, J. \|e verfasserin \|4 aut
700	1		\|a Kobayashi, Y. \|e verfasserin \|4 aut
700	1		\|a Kohri, K. \|e verfasserin \|4 aut
700	1		\|a Komin, N. \|e verfasserin \|4 aut
700	1		\|a Kornecki, P. \|e verfasserin \|4 aut
700	1		\|a Kubo, H. \|e verfasserin \|4 aut
700	1		\|a La Palombara, N. \|e verfasserin \|4 aut
700	1		\|a Láinez, M. \|e verfasserin \|4 aut
700	1		\|a Lamastra, A. \|e verfasserin \|4 aut
700	1		\|a Lapington, J. \|e verfasserin \|4 aut
700	1		\|a Lemoine-Goumard, M. \|e verfasserin \|4 aut
700	1		\|a Lenain, J.-P. \|e verfasserin \|4 aut
700	1		\|a Leone, F. \|e verfasserin \|4 aut
700	1		\|a Leto, G. \|e verfasserin \|4 aut
700	1		\|a Leuschner, F. \|e verfasserin \|4 aut
700	1		\|a Lindfors, E. \|e verfasserin \|4 aut
700	1		\|a Liodakis, I. \|e verfasserin \|4 aut
700	1		\|a Lohse, T. \|e verfasserin \|4 aut
700	1		\|a Lombardi, S. \|e verfasserin \|4 aut
700	1		\|a Longo, F. \|e verfasserin \|4 aut
700	1		\|a López-Coto, R. \|e verfasserin \|4 aut
700	1		\|a López-Moya, M. \|e verfasserin \|4 aut
700	1		\|a López-Oramas, A. \|e verfasserin \|4 aut
700	1		\|a Loporchio, S. \|e verfasserin \|4 aut
700	1		\|a Luque-Escamilla, P.L. \|e verfasserin \|4 aut
700	1		\|a Macias, O. \|e verfasserin \|4 aut
700	1		\|a Mackey, J. \|e verfasserin \|4 aut
700	1		\|a Majumdar, P. \|e verfasserin \|4 aut
700	1		\|a Mandat, D. \|e verfasserin \|4 aut
700	1		\|a Manganaro, M. \|e verfasserin \|4 aut
700	1		\|a Manicò, G. \|e verfasserin \|4 aut
700	1		\|a Marconi, M. \|e verfasserin \|4 aut
700	1		\|a Martí, J. \|e verfasserin \|4 aut
700	1		\|a Martínez, G. \|e verfasserin \|4 aut
700	1		\|a Martinez, M. \|e verfasserin \|4 aut
700	1		\|a Martinez, O. \|e verfasserin \|4 aut
700	1		\|a Mello, A.J.T.S. \|e verfasserin \|4 aut
700	1		\|a Menchiari, S. \|e verfasserin \|4 aut
700	1		\|a Meyer, D.M.-A. \|e verfasserin \|4 aut
700	1		\|a Micanovic, S. \|e verfasserin \|4 aut
700	1		\|a Miceli, D. \|e verfasserin \|4 aut
700	1		\|a Miceli, M. \|e verfasserin \|4 aut
700	1		\|a Michalowski, J. \|e verfasserin \|4 aut
700	1		\|a Miener, T. \|e verfasserin \|4 aut
700	1		\|a Miranda, J.M. \|e verfasserin \|4 aut
700	1		\|a Mitchell, A. \|e verfasserin \|4 aut
700	1		\|a Mode, B. \|e verfasserin \|4 aut
700	1		\|a Moderski, R. \|e verfasserin \|4 aut
700	1		\|a Mohrmann, L. \|e verfasserin \|4 aut
700	1		\|a Molina, E. \|e verfasserin \|4 aut
700	1		\|a Montaruli, T. \|e verfasserin \|4 aut
700	1		\|a Morcuende, D. \|e verfasserin \|4 aut
700	1		\|a Morlino, G. \|e verfasserin \|4 aut
700	1		\|a Morselli, A. \|e verfasserin \|4 aut
700	1		\|a Mosè, M. \|e verfasserin \|4 aut
700	1		\|a Moulin, E. \|e verfasserin \|4 aut
700	1		\|a Mukherjee, R. \|e verfasserin \|4 aut
700	1		\|a Munari, K. \|e verfasserin \|4 aut
700	1		\|a Murach, T. \|e verfasserin \|4 aut
700	1		\|a Nagai, A. \|e verfasserin \|4 aut
700	1		\|a Nagataki, S. \|e verfasserin \|4 aut
700	1		\|a Nemmen, R. \|e verfasserin \|4 aut
700	1		\|a Niemiec, J. \|e verfasserin \|4 aut
700	1		\|a Nieto, D. \|e verfasserin \|4 aut
700	1		\|a Rosillo, M. Nievas \|e verfasserin \|4 aut
700	1		\|a Nikolajuk, M. \|e verfasserin \|4 aut
700	1		\|a Nishijima, K. \|e verfasserin \|4 aut
700	1		\|a Noda, K. \|e verfasserin \|4 aut
700	1		\|a Novosyadlyj, B. \|e verfasserin \|4 aut
700	1		\|a Nozaki, S. \|e verfasserin \|4 aut
700	1		\|a Ohishi, M. \|e verfasserin \|4 aut
700	1		\|a Ohm, S. \|e verfasserin \|4 aut
700	1		\|a Ohtani, Y. \|e verfasserin \|4 aut
700	1		\|a Okumura, A. \|e verfasserin \|4 aut
700	1		\|a Olmi, B. \|e verfasserin \|4 aut
700	1		\|a Ong, R.A. \|e verfasserin \|4 aut
700	1		\|a Orienti, M. \|e verfasserin \|4 aut
700	1		\|a Orito, R. \|e verfasserin \|4 aut
700	1		\|a Orlandini, M. \|e verfasserin \|4 aut
700	1		\|a Orlando, E. \|e verfasserin \|4 aut
700	1		\|a Orlando, S. \|e verfasserin \|4 aut
700	1		\|a Ostrowski, M. \|e verfasserin \|4 aut
700	1		\|a Oya, I. \|e verfasserin \|4 aut
700	1		\|a Pantaleo, F.R. \|e verfasserin \|4 aut
700	1		\|a Paredes, J.M. \|e verfasserin \|4 aut
700	1		\|a Patricelli, B. \|e verfasserin \|4 aut
700	1		\|a Pecimotika, M. \|e verfasserin \|4 aut
700	1		\|a Peresano, M. \|e verfasserin \|4 aut
700	1		\|a Pérez-Romero, J. \|e verfasserin \|4 aut
700	1		\|a Persic, M. \|e verfasserin \|4 aut
700	1		\|a Petruk, O. \|e verfasserin \|4 aut
700	1		\|a Piano, G. \|e verfasserin \|4 aut
700	1		\|a Pietropaolo, E. \|e verfasserin \|4 aut
700	1		\|a Pirola, G. \|e verfasserin \|4 aut
700	1		\|a Pittori, C. \|e verfasserin \|4 aut
700	1		\|a Pohl, M. \|e verfasserin \|4 aut
700	1		\|a Ponti, G. \|e verfasserin \|4 aut
700	1		\|a Prandini, E. \|e verfasserin \|4 aut
700	1		\|a Principe, G. \|e verfasserin \|4 aut
700	1		\|a Priyadarshi, C. \|e verfasserin \|4 aut
700	1		\|a Pueschel, E. \|e verfasserin \|4 aut
700	1		\|a Pühlhofer, G. \|e verfasserin \|4 aut
700	1		\|a Pumo, M.L. \|e verfasserin \|4 aut
700	1		\|a Quirrenbach, A. \|e verfasserin \|4 aut
700	1		\|a Rando, R. \|e verfasserin \|4 aut
700	1		\|a Razzaque, S. \|e verfasserin \|4 aut
700	1		\|a Reichherzer, P. \|e verfasserin \|4 aut
700	1		\|a Reimer, A. \|e verfasserin \|4 aut
700	1		\|a Reimer, O. \|e verfasserin \|4 aut
700	1		\|a Renaud, M. \|e verfasserin \|4 aut
700	1		\|a Reposeur, T. \|e verfasserin \|4 aut
700	1		\|a Ribó, M. \|e verfasserin \|4 aut
700	1		\|a Richtler, T. \|e verfasserin \|4 aut
700	1		\|a Rico, J. \|e verfasserin \|4 aut
700	1		\|a Rieger, F. \|e verfasserin \|4 aut
700	1		\|a Rigoselli, M. \|e verfasserin \|4 aut
700	1		\|a Riitano, L. \|e verfasserin \|4 aut
700	1		\|a Rizi, V. \|e verfasserin \|4 aut
700	1		\|a Roache, E. \|e verfasserin \|4 aut
700	1		\|a Romano, P. \|e verfasserin \|4 aut
700	1		\|a Romeo, G. \|e verfasserin \|4 aut
700	1		\|a Rosado, J. \|e verfasserin \|4 aut
700	1		\|a Rowell, G. \|e verfasserin \|4 aut
700	1		\|a Rudak, B. \|e verfasserin \|4 aut
700	1		\|a Sadeh, I. \|e verfasserin \|4 aut
700	1		\|a Safi-Harb, S. \|e verfasserin \|4 aut
700	1		\|a Saha, L. \|e verfasserin \|4 aut
700	1		\|a Sailer, S. \|e verfasserin \|4 aut
700	1		\|a Sánchez-Conde, M. \|e verfasserin \|4 aut
700	1		\|a Sarkar, S. \|e verfasserin \|4 aut
700	1		\|a Satalecka, K. \|e verfasserin \|4 aut
700	1		\|a Saturni, F.G. \|e verfasserin \|4 aut
700	1		\|a Scherer, A. \|e verfasserin \|4 aut
700	1		\|a Schovánek, P. \|e verfasserin \|4 aut
700	1		\|a Schussler, F. \|e verfasserin \|4 aut
700	1		\|a Schwanke, U. \|e verfasserin \|4 aut
700	1		\|a Scuderi, S. \|e verfasserin \|4 aut
700	1		\|a Seglar-Arroyo, M. \|e verfasserin \|4 aut
700	1		\|a Sergijenko, O. \|e verfasserin \|4 aut
700	1		\|a Servillat, M. \|e verfasserin \|4 aut
700	1		\|a Shang, R.-Y. \|e verfasserin \|4 aut
700	1		\|a Sharma, P. \|e verfasserin \|4 aut
700	1		\|a Siejkowski, H. \|e verfasserin \|4 aut
700	1		\|a Sliusar, V. \|e verfasserin \|4 aut
700	1		\|a Słowikowska, A. \|e verfasserin \|4 aut
700	1		\|a Sol, H. \|e verfasserin \|4 aut
700	1		\|a Specovius, A. \|e verfasserin \|4 aut
700	1		\|a Spencer, S.T. \|e verfasserin \|4 aut
700	1		\|a Spengler, G. \|e verfasserin \|4 aut
700	1		\|a Stamerra, A. \|e verfasserin \|4 aut
700	1		\|a Stanič, S. \|e verfasserin \|4 aut
700	1		\|a Starecki, T. \|e verfasserin \|4 aut
700	1		\|a Starling, R. \|e verfasserin \|4 aut
700	1		\|a Stolarczyk, T. \|e verfasserin \|4 aut
700	1		\|a Pereira, L.A. Stuani \|e verfasserin \|4 aut
700	1		\|a Suda, Y. \|e verfasserin \|4 aut
700	1		\|a Suomijarvi, T. \|e verfasserin \|4 aut
700	1		\|a Sushch, I. \|e verfasserin \|4 aut
700	1		\|a Tajima, H. \|e verfasserin \|4 aut
700	1		\|a Tam, P.-H.T. \|e verfasserin \|4 aut
700	1		\|a Tanaka, S.J. \|e verfasserin \|4 aut
700	1		\|a Tavecchio, F. \|e verfasserin \|4 aut
700	1		\|a Testa, V. \|e verfasserin \|4 aut
700	1		\|a Tian, W. \|e verfasserin \|4 aut
700	1		\|a Tibaldo, L. \|e verfasserin \|4 aut
700	1		\|a Torres, D.F. \|e verfasserin \|4 aut
700	1		\|a Tothill, N. \|e verfasserin \|4 aut
700	1		\|a Vallage, B. \|e verfasserin \|4 aut
700	1		\|a Vallania, P. \|e verfasserin \|4 aut
700	1		\|a van Eldik, C. \|e verfasserin \|4 aut
700	1		\|a van Scherpenberg, J. \|e verfasserin \|4 aut
700	1		\|a Vandenbroucke, J. \|e verfasserin \|4 aut
700	1		\|a Acosta, M. Vazquez \|e verfasserin \|4 aut
700	1		\|a Vecchi, M. \|e verfasserin \|4 aut
700	1		\|a Vercellone, S. \|e verfasserin \|4 aut
700	1		\|a Verna, G. \|e verfasserin \|4 aut
700	1		\|a Viana, A. \|e verfasserin \|4 aut
700	1		\|a Vignatti, J. \|e verfasserin \|4 aut
700	1		\|a Vitale, V. \|e verfasserin \|4 aut
700	1		\|a Vodeb, V. \|e verfasserin \|4 aut
700	1		\|a Vorobiov, S. \|e verfasserin \|4 aut
700	1		\|a Vuillaume, T. \|e verfasserin \|4 aut
700	1		\|a Wagner, S.J. \|e verfasserin \|4 aut
700	1		\|a Walter, R. \|e verfasserin \|4 aut
700	1		\|a White, M. \|e verfasserin \|4 aut
700	1		\|a Wierzcholska, A. \|e verfasserin \|4 aut
700	1		\|a Will, M. \|e verfasserin \|4 aut
700	1		\|a Williams, D. \|e verfasserin \|4 aut
700	1		\|a Yang, L. \|e verfasserin \|4 aut
700	1		\|a Yoshida, T. \|e verfasserin \|4 aut
700	1		\|a Yoshikoshi, T. \|e verfasserin \|4 aut
700	1		\|a Zaharijas, G. \|e verfasserin \|4 aut
700	1		\|a Zampieri, L. \|e verfasserin \|4 aut
700	1		\|a Zavrtanik, D. \|e verfasserin \|4 aut
700	1		\|a Zavrtanik, M. \|e verfasserin \|4 aut
700	1		\|a Zhdanov, V.I. \|e verfasserin \|4 aut
700	1		\|a Z̆ivec, M. \|e verfasserin \|4 aut
773	0	8	\|i Enthalten in \|t Astroparticle physics \|d Amsterdam [u.a.] : Elsevier Science, 1992 \|g 150 \|h Online-Ressource \|w (DE-627)306654059 \|w (DE-600)1499883-X \|w (DE-576)116226218 \|x 0927-6505 \|7 nnns
773	1	8	\|g volume:150
912			\|a GBV_USEFLAG_U
912			\|a SYSFLAG_U
912			\|a GBV_ELV
912			\|a SSG-OLC-PHA
912			\|a SSG-OPC-AST
912			\|a GBV_ILN_20
912			\|a GBV_ILN_22
912			\|a GBV_ILN_23
912			\|a GBV_ILN_24
912			\|a GBV_ILN_31
912			\|a GBV_ILN_32
912			\|a GBV_ILN_40
912			\|a GBV_ILN_60
912			\|a GBV_ILN_62
912			\|a GBV_ILN_65
912			\|a GBV_ILN_69
912			\|a GBV_ILN_70
912			\|a GBV_ILN_73
912			\|a GBV_ILN_74
912			\|a GBV_ILN_90
912			\|a GBV_ILN_95
912			\|a GBV_ILN_100
912			\|a GBV_ILN_101
912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_150
912			\|a GBV_ILN_151
912			\|a GBV_ILN_187
912			\|a GBV_ILN_213
912			\|a GBV_ILN_224
912			\|a GBV_ILN_230
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_702
912			\|a GBV_ILN_2001
912			\|a GBV_ILN_2003
912			\|a GBV_ILN_2004
912			\|a GBV_ILN_2005
912			\|a GBV_ILN_2007
912			\|a GBV_ILN_2008
912			\|a GBV_ILN_2009
912			\|a GBV_ILN_2010
912			\|a GBV_ILN_2011
912			\|a GBV_ILN_2014
912			\|a GBV_ILN_2015
912			\|a GBV_ILN_2020
912			\|a GBV_ILN_2021
912			\|a GBV_ILN_2025
912			\|a GBV_ILN_2026
912			\|a GBV_ILN_2027
912			\|a GBV_ILN_2034
912			\|a GBV_ILN_2044
912			\|a GBV_ILN_2048
912			\|a GBV_ILN_2049
912			\|a GBV_ILN_2050
912			\|a GBV_ILN_2055
912			\|a GBV_ILN_2056
912			\|a GBV_ILN_2059
912			\|a GBV_ILN_2061
912			\|a GBV_ILN_2064
912			\|a GBV_ILN_2088
912			\|a GBV_ILN_2106
912			\|a GBV_ILN_2110
912			\|a GBV_ILN_2111
912			\|a GBV_ILN_2112
912			\|a GBV_ILN_2122
912			\|a GBV_ILN_2129
912			\|a GBV_ILN_2143
912			\|a GBV_ILN_2152
912			\|a GBV_ILN_2153
912			\|a GBV_ILN_2190
912			\|a GBV_ILN_2232
912			\|a GBV_ILN_2336
912			\|a GBV_ILN_2470
912			\|a GBV_ILN_2507
912			\|a GBV_ILN_4035
912			\|a GBV_ILN_4037
912			\|a GBV_ILN_4112
912			\|a GBV_ILN_4125
912			\|a GBV_ILN_4242
912			\|a GBV_ILN_4249
912			\|a GBV_ILN_4251
912			\|a GBV_ILN_4305
912			\|a GBV_ILN_4306
912			\|a GBV_ILN_4307
912			\|a GBV_ILN_4313
912			\|a GBV_ILN_4322
912			\|a GBV_ILN_4323
912			\|a GBV_ILN_4324
912			\|a GBV_ILN_4325
912			\|a GBV_ILN_4326
912			\|a GBV_ILN_4333
912			\|a GBV_ILN_4334
912			\|a GBV_ILN_4338
912			\|a GBV_ILN_4393
912			\|a GBV_ILN_4700
936	b	k	\|a 39.22 \|j Astrophysik
951			\|a AR
952			\|d 150

Indexfelder

author_variant	f a fa a a aa r a ra a a c aac i a ia a a s aas j a ja r a ra n á c ná nác r a b ra rab l a la e a ea g a ga e a ea c a ca c a ca t a ta k a ka y a ya j a ja m b mb a b ab c b cb m b mb j b jb a b l ab abl v b m vb vbm a u b d aub aubd j b jb d b db j b jb j b t jb jbt w b wb m b m mbm j b jb a b ab b b bb v b vb p b pb s b sb a b ab e b eb j b jb o b ob p b pb e b eb j b jb r b rb n b nb a b ab m c mc r c d rc rcd p c pc m c mc r c rc s c sc e c ec f c fc f c fc m c mc p c pc s c sc a c ac m c mc a c ac j c jc c c a cca v c vc j c jc a c ac h c hc p c pc r c rc g d gd f d fd a a d aa aad c v d cv cvd g d p e d gdpe gdped o w e d owe owed s v d sv svd c d cd v d d vd vdd d d dd g t d gt gtd p f d pf pfd t r d tr trd v l d vl vld s d sd j d jd a d ad m d md a r d ar ard v d vd s e se d e de g e ge c e ce d f g dfg e f ef s f sf g f gf e f ef m f mf v f vf m f mf l f lf g f gf s f sf g g gg g g gg v g vg c g cg a g ag g g gg m g mg g g gg n g ng f g fg m g mg a g ag l g lg n g ng j g c jg jgc l g lg d g dg m h g mhg o g og s g sg t h th m h mh s h c shc j h jh b h bh r h rh d h dh w h wh j h jh d h dh p h ph m h mh d h dh t i ti f i fi s i si k i ki m j mj p j pj i j m ij ijm w j wj i j r ijr j j jj p k pk v k vk u k uk d k dk b k bk d k dk r k rk t k tk g k gk w k wk j k jk y k yk k k kk n k nk p k pk h k hk p n l pn pnl m l ml a l al j l jl m l g mlg j p l jpl f l fl g l gl f l fl e l el i l il t l tl s l sl f l fl r l c rlc m l m mlm a l o alo s l sl p l e ple o m om j m jm p m pm d m dm m m mm g m gm m m mm j m jm g m gm m m mm o m om a m am s m sm d a m dam s m sm d m dm m m mm j m jm t m tm j m jm a m am b m bm r m rm l m lm e m em t m tm d m dm g m gm a m am m m mm e m em r m rm k m km t m tm a n an s n sn r n rn j n jn d n dn m n r mn mnr m n mn k n kn k n kn b n bn s n sn m o mo s o so y o yo a o ao b o bo r o ro m o mo r o ro m o mo e o eo s o so m o mo i o io f p fp j p jp b p bp m p mp m p mp j p r jpr m p mp o p op g p gp e p ep g p gp c p cp m p mp g p gp e p ep g p gp c p cp e p ep g p gp m p mp a q aq r r rr s r sr p r pr a r ar o r or m r mr t r tr m r mr t r tr j r jr f r fr m r mr l r lr v r vr e r er p r pr g r gr j r jr g r gr b r br i s is s s h ssh l s ls s s ss m s c msc s s ss k s ks f s fs a s as p s ps f s fs u s us s s ss m s a msa o s os m s ms r y s rys p s ps h s hs v s vs a s as h s hs a s as s s ss g s gs a s as s s ss t s ts r s rs t s ts l s p ls lsp y s ys t s ts i s is h t ht p h t pht s t st f t ft v t vt w t wt l t lt d t dt n t nt b v bv p v pv e c v ec ecv s j v sj sjv j v jv m v a mv mva m v mv s v sv g v gv a v av j v jv v v vv v v vv s v sv t v tv s w sw r w rw m w mw a w aw m w mw d w dw l y ly t y ty t y ty g z gz l z lz d z dz m z mz v z vz m z mz
matchkey_str	article:09276505:2023----::estvtotehrnotlsoeratsetasgaueohdoipvtosihplct
hierarchy_sort_str	2023
bklnumber	39.22
publishDate	2023
allfields	10.1016/j.astropartphys.2023.102850 doi (DE-627)ELV009642641 (ELSEVIER)S0927-6505(23)00036-1 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Acero, F. verfasserin aut Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source. Gamma rays: general Cosmic rays Galactic PeVatrons (Stars:) supernovae: general Methods: data analysis Methods: statistical Acharyya, A. verfasserin aut Adam, R. verfasserin aut Aguasca-Cabot, A. verfasserin aut Agudo, I. verfasserin aut Aguirre-Santaella, A. verfasserin aut Alfaro, J. verfasserin aut Aloisio, R. verfasserin aut Crespo, N. Álvarez verfasserin aut Batista, R. Alves verfasserin aut Amati, L. verfasserin aut Amato, E. verfasserin aut Ambrosi, G. verfasserin aut Angüner, E.O. verfasserin aut Aramo, C. verfasserin aut Arcaro, C. verfasserin aut Armstrong, T. verfasserin aut Asano, K. verfasserin aut Ascasibar, Y. verfasserin aut Aschersleben, J. verfasserin aut Backes, M. verfasserin aut Baktash, A. verfasserin aut Balazs, C. verfasserin aut Balbo, M. verfasserin aut Ballet, J. verfasserin aut Larriva, A. Baquero verfasserin aut Martins, V. Barbosa verfasserin aut de Almeida, U. Barres verfasserin aut Barrio, J.A. verfasserin aut Bastieri, D. verfasserin aut Baxter, J.R. verfasserin aut Tjus, J. Becker verfasserin aut Benbow, W. verfasserin aut Bernardos-Martín, M.I. verfasserin aut Bernete, J. verfasserin aut Berti, A. verfasserin aut Bertucci, B. verfasserin aut Beshley, V. verfasserin aut Bhattacharjee, P. verfasserin aut Bhattacharyya, S. verfasserin aut Biland, A. verfasserin aut Bissaldi, E. verfasserin aut Biteau, J. verfasserin aut Blanch, O. verfasserin aut Bordas, P. verfasserin aut Bottacini, E. verfasserin aut Bregeon, J. verfasserin aut Brose, R. verfasserin aut Bucciantini, N. verfasserin aut Bulgarelli, A. verfasserin aut Capasso, M. verfasserin aut Dolcetta, R.A. Capuzzo verfasserin aut Caraveo, P. verfasserin aut Cardillo, M. verfasserin aut Carosi, R. verfasserin aut Casanova, S. verfasserin aut Cascone, E. verfasserin aut Cassol, F. verfasserin aut Catalani, F. verfasserin aut Cerruti, M. verfasserin aut Chadwick, P. verfasserin aut Chaty, S. verfasserin aut Chen, A. verfasserin aut Chernyakova, M. verfasserin aut Chiavassa, A. verfasserin aut Chudoba, J. verfasserin aut Coimbra-Araujo, C. verfasserin aut Conforti, V. verfasserin aut Contreras, J.L. verfasserin aut Costa, A. verfasserin aut Costantini, H. verfasserin aut Cristofari, P. verfasserin aut Crocker, R. verfasserin aut D’Amico, G. verfasserin aut D’Ammando, F. verfasserin aut De Angelis, A. verfasserin aut De Caprio, V. verfasserin aut de Gouveia Dal Pino, E.M. verfasserin aut de Ona Wilhelmi, E. verfasserin aut de Souza, V. verfasserin aut Delgado, C. verfasserin aut della Volpe, D. verfasserin aut Depaoli, D. verfasserin aut Di Girolamo, T. verfasserin aut Di Pierro, F. verfasserin aut Di Tria, R. verfasserin aut Di Venere, L. verfasserin aut Diebold, S. verfasserin aut Djuvsland, J.I. verfasserin aut Donini, A. verfasserin aut Doro, M. verfasserin aut Dos Anjos, R.d.C. verfasserin aut Dwarkadas, V.V. verfasserin aut Einecke, S. verfasserin aut Elsässer, D. verfasserin aut Emery, G. verfasserin aut Evoli, C. verfasserin aut Falceta-Goncalves, D. verfasserin aut Fedorova, E. verfasserin aut Fegan, S. verfasserin aut Ferrand, G. verfasserin aut Fiandrini, E. verfasserin aut Filipovic, M. verfasserin aut Fioretti, V. verfasserin aut Fiori, M. verfasserin aut Foffano, L. verfasserin aut Fontaine, G. verfasserin aut Fukami, S. verfasserin aut Galanti, G. verfasserin aut Galaz, G. verfasserin aut Gammaldi, V. verfasserin aut Gasbarra, C. verfasserin aut Ghalumyan, A. verfasserin aut Ghirlanda, G. verfasserin aut Giarrusso, M. verfasserin aut Giavitto, G. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Giroletti, M. verfasserin aut Giuliani, A. verfasserin aut Giunti, L. verfasserin aut Godinovic, N. verfasserin aut Coelho, J. Goulart verfasserin aut Gréaux, L. verfasserin aut Green, D. verfasserin aut Grondin, M.-H. verfasserin aut Gueta, O. verfasserin aut Gunji, S. verfasserin aut Hassan, T. verfasserin aut Heller, M. verfasserin aut Hernández-Cadena, S. verfasserin aut Hinton, J. verfasserin aut Hnatyk, B. verfasserin aut Hnatyk, R. verfasserin aut Hoffmann, D. verfasserin aut Hofmann, W. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Horvath, P. verfasserin aut Hrabovsky, M. verfasserin aut Hrupec, D. verfasserin aut Inada, T. verfasserin aut Incardona, F. verfasserin aut Inoue, S. verfasserin aut Ishio, K. verfasserin aut Jamrozy, M. verfasserin aut Janecek, P. verfasserin aut Martínez, I. Jiménez verfasserin aut Jin, W. verfasserin aut Jung-Richardt, I. verfasserin aut Jurysek, J. verfasserin aut Kaaret, P. verfasserin aut Karas, V. verfasserin aut Katz, U. verfasserin aut Kerszberg, D. verfasserin aut Khélifi, B. verfasserin aut Kieda, D.B. verfasserin aut Kissmann, R. verfasserin aut Kleiner, T. verfasserin aut Kluge, G. verfasserin aut Kluzniak, W. verfasserin aut Knödlseder, J. verfasserin aut Kobayashi, Y. verfasserin aut Kohri, K. verfasserin aut Komin, N. verfasserin aut Kornecki, P. verfasserin aut Kubo, H. verfasserin aut La Palombara, N. verfasserin aut Láinez, M. verfasserin aut Lamastra, A. verfasserin aut Lapington, J. verfasserin aut Lemoine-Goumard, M. verfasserin aut Lenain, J.-P. verfasserin aut Leone, F. verfasserin aut Leto, G. verfasserin aut Leuschner, F. verfasserin aut Lindfors, E. verfasserin aut Liodakis, I. verfasserin aut Lohse, T. verfasserin aut Lombardi, S. verfasserin aut Longo, F. verfasserin aut López-Coto, R. verfasserin aut López-Moya, M. verfasserin aut López-Oramas, A. verfasserin aut Loporchio, S. verfasserin aut Luque-Escamilla, P.L. verfasserin aut Macias, O. verfasserin aut Mackey, J. verfasserin aut Majumdar, P. verfasserin aut Mandat, D. verfasserin aut Manganaro, M. verfasserin aut Manicò, G. verfasserin aut Marconi, M. verfasserin aut Martí, J. verfasserin aut Martínez, G. verfasserin aut Martinez, M. verfasserin aut Martinez, O. verfasserin aut Mello, A.J.T.S. verfasserin aut Menchiari, S. verfasserin aut Meyer, D.M.-A. verfasserin aut Micanovic, S. verfasserin aut Miceli, D. verfasserin aut Miceli, M. verfasserin aut Michalowski, J. verfasserin aut Miener, T. verfasserin aut Miranda, J.M. verfasserin aut Mitchell, A. verfasserin aut Mode, B. verfasserin aut Moderski, R. verfasserin aut Mohrmann, L. verfasserin aut Molina, E. verfasserin aut Montaruli, T. verfasserin aut Morcuende, D. verfasserin aut Morlino, G. verfasserin aut Morselli, A. verfasserin aut Mosè, M. verfasserin aut Moulin, E. verfasserin aut Mukherjee, R. verfasserin aut Munari, K. verfasserin aut Murach, T. verfasserin aut Nagai, A. verfasserin aut Nagataki, S. verfasserin aut Nemmen, R. verfasserin aut Niemiec, J. verfasserin aut Nieto, D. verfasserin aut Rosillo, M. Nievas verfasserin aut Nikolajuk, M. verfasserin aut Nishijima, K. verfasserin aut Noda, K. verfasserin aut Novosyadlyj, B. verfasserin aut Nozaki, S. verfasserin aut Ohishi, M. verfasserin aut Ohm, S. verfasserin aut Ohtani, Y. verfasserin aut Okumura, A. verfasserin aut Olmi, B. verfasserin aut Ong, R.A. verfasserin aut Orienti, M. verfasserin aut Orito, R. verfasserin aut Orlandini, M. verfasserin aut Orlando, E. verfasserin aut Orlando, S. verfasserin aut Ostrowski, M. verfasserin aut Oya, I. verfasserin aut Pantaleo, F.R. verfasserin aut Paredes, J.M. verfasserin aut Patricelli, B. verfasserin aut Pecimotika, M. verfasserin aut Peresano, M. verfasserin aut Pérez-Romero, J. verfasserin aut Persic, M. verfasserin aut Petruk, O. verfasserin aut Piano, G. verfasserin aut Pietropaolo, E. verfasserin aut Pirola, G. verfasserin aut Pittori, C. verfasserin aut Pohl, M. verfasserin aut Ponti, G. verfasserin aut Prandini, E. verfasserin aut Principe, G. verfasserin aut Priyadarshi, C. verfasserin aut Pueschel, E. verfasserin aut Pühlhofer, G. verfasserin aut Pumo, M.L. verfasserin aut Quirrenbach, A. verfasserin aut Rando, R. verfasserin aut Razzaque, S. verfasserin aut Reichherzer, P. verfasserin aut Reimer, A. verfasserin aut Reimer, O. verfasserin aut Renaud, M. verfasserin aut Reposeur, T. verfasserin aut Ribó, M. verfasserin aut Richtler, T. verfasserin aut Rico, J. verfasserin aut Rieger, F. verfasserin aut Rigoselli, M. verfasserin aut Riitano, L. verfasserin aut Rizi, V. verfasserin aut Roache, E. verfasserin aut Romano, P. verfasserin aut Romeo, G. verfasserin aut Rosado, J. verfasserin aut Rowell, G. verfasserin aut Rudak, B. verfasserin aut Sadeh, I. verfasserin aut Safi-Harb, S. verfasserin aut Saha, L. verfasserin aut Sailer, S. verfasserin aut Sánchez-Conde, M. verfasserin aut Sarkar, S. verfasserin aut Satalecka, K. verfasserin aut Saturni, F.G. verfasserin aut Scherer, A. verfasserin aut Schovánek, P. verfasserin aut Schussler, F. verfasserin aut Schwanke, U. verfasserin aut Scuderi, S. verfasserin aut Seglar-Arroyo, M. verfasserin aut Sergijenko, O. verfasserin aut Servillat, M. verfasserin aut Shang, R.-Y. verfasserin aut Sharma, P. verfasserin aut Siejkowski, H. verfasserin aut Sliusar, V. verfasserin aut Słowikowska, A. verfasserin aut Sol, H. verfasserin aut Specovius, A. verfasserin aut Spencer, S.T. verfasserin aut Spengler, G. verfasserin aut Stamerra, A. verfasserin aut Stanič, S. verfasserin aut Starecki, T. verfasserin aut Starling, R. verfasserin aut Stolarczyk, T. verfasserin aut Pereira, L.A. Stuani verfasserin aut Suda, Y. verfasserin aut Suomijarvi, T. verfasserin aut Sushch, I. verfasserin aut Tajima, H. verfasserin aut Tam, P.-H.T. verfasserin aut Tanaka, S.J. verfasserin aut Tavecchio, F. verfasserin aut Testa, V. verfasserin aut Tian, W. verfasserin aut Tibaldo, L. verfasserin aut Torres, D.F. verfasserin aut Tothill, N. verfasserin aut Vallage, B. verfasserin aut Vallania, P. verfasserin aut van Eldik, C. verfasserin aut van Scherpenberg, J. verfasserin aut Vandenbroucke, J. verfasserin aut Acosta, M. Vazquez verfasserin aut Vecchi, M. verfasserin aut Vercellone, S. verfasserin aut Verna, G. verfasserin aut Viana, A. verfasserin aut Vignatti, J. verfasserin aut Vitale, V. verfasserin aut Vodeb, V. verfasserin aut Vorobiov, S. verfasserin aut Vuillaume, T. verfasserin aut Wagner, S.J. verfasserin aut Walter, R. verfasserin aut White, M. verfasserin aut Wierzcholska, A. verfasserin aut Will, M. verfasserin aut Williams, D. verfasserin aut Yang, L. verfasserin aut Yoshida, T. verfasserin aut Yoshikoshi, T. verfasserin aut Zaharijas, G. verfasserin aut Zampieri, L. verfasserin aut Zavrtanik, D. verfasserin aut Zavrtanik, M. verfasserin aut Zhdanov, V.I. verfasserin aut Z̆ivec, M. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 150 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:150 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.22 Astrophysik AR 150
spelling	10.1016/j.astropartphys.2023.102850 doi (DE-627)ELV009642641 (ELSEVIER)S0927-6505(23)00036-1 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Acero, F. verfasserin aut Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source. Gamma rays: general Cosmic rays Galactic PeVatrons (Stars:) supernovae: general Methods: data analysis Methods: statistical Acharyya, A. verfasserin aut Adam, R. verfasserin aut Aguasca-Cabot, A. verfasserin aut Agudo, I. verfasserin aut Aguirre-Santaella, A. verfasserin aut Alfaro, J. verfasserin aut Aloisio, R. verfasserin aut Crespo, N. Álvarez verfasserin aut Batista, R. Alves verfasserin aut Amati, L. verfasserin aut Amato, E. verfasserin aut Ambrosi, G. verfasserin aut Angüner, E.O. verfasserin aut Aramo, C. verfasserin aut Arcaro, C. verfasserin aut Armstrong, T. verfasserin aut Asano, K. verfasserin aut Ascasibar, Y. verfasserin aut Aschersleben, J. verfasserin aut Backes, M. verfasserin aut Baktash, A. verfasserin aut Balazs, C. verfasserin aut Balbo, M. verfasserin aut Ballet, J. verfasserin aut Larriva, A. Baquero verfasserin aut Martins, V. Barbosa verfasserin aut de Almeida, U. Barres verfasserin aut Barrio, J.A. verfasserin aut Bastieri, D. verfasserin aut Baxter, J.R. verfasserin aut Tjus, J. Becker verfasserin aut Benbow, W. verfasserin aut Bernardos-Martín, M.I. verfasserin aut Bernete, J. verfasserin aut Berti, A. verfasserin aut Bertucci, B. verfasserin aut Beshley, V. verfasserin aut Bhattacharjee, P. verfasserin aut Bhattacharyya, S. verfasserin aut Biland, A. verfasserin aut Bissaldi, E. verfasserin aut Biteau, J. verfasserin aut Blanch, O. verfasserin aut Bordas, P. verfasserin aut Bottacini, E. verfasserin aut Bregeon, J. verfasserin aut Brose, R. verfasserin aut Bucciantini, N. verfasserin aut Bulgarelli, A. verfasserin aut Capasso, M. verfasserin aut Dolcetta, R.A. Capuzzo verfasserin aut Caraveo, P. verfasserin aut Cardillo, M. verfasserin aut Carosi, R. verfasserin aut Casanova, S. verfasserin aut Cascone, E. verfasserin aut Cassol, F. verfasserin aut Catalani, F. verfasserin aut Cerruti, M. verfasserin aut Chadwick, P. verfasserin aut Chaty, S. verfasserin aut Chen, A. verfasserin aut Chernyakova, M. verfasserin aut Chiavassa, A. verfasserin aut Chudoba, J. verfasserin aut Coimbra-Araujo, C. verfasserin aut Conforti, V. verfasserin aut Contreras, J.L. verfasserin aut Costa, A. verfasserin aut Costantini, H. verfasserin aut Cristofari, P. verfasserin aut Crocker, R. verfasserin aut D’Amico, G. verfasserin aut D’Ammando, F. verfasserin aut De Angelis, A. verfasserin aut De Caprio, V. verfasserin aut de Gouveia Dal Pino, E.M. verfasserin aut de Ona Wilhelmi, E. verfasserin aut de Souza, V. verfasserin aut Delgado, C. verfasserin aut della Volpe, D. verfasserin aut Depaoli, D. verfasserin aut Di Girolamo, T. verfasserin aut Di Pierro, F. verfasserin aut Di Tria, R. verfasserin aut Di Venere, L. verfasserin aut Diebold, S. verfasserin aut Djuvsland, J.I. verfasserin aut Donini, A. verfasserin aut Doro, M. verfasserin aut Dos Anjos, R.d.C. verfasserin aut Dwarkadas, V.V. verfasserin aut Einecke, S. verfasserin aut Elsässer, D. verfasserin aut Emery, G. verfasserin aut Evoli, C. verfasserin aut Falceta-Goncalves, D. verfasserin aut Fedorova, E. verfasserin aut Fegan, S. verfasserin aut Ferrand, G. verfasserin aut Fiandrini, E. verfasserin aut Filipovic, M. verfasserin aut Fioretti, V. verfasserin aut Fiori, M. verfasserin aut Foffano, L. verfasserin aut Fontaine, G. verfasserin aut Fukami, S. verfasserin aut Galanti, G. verfasserin aut Galaz, G. verfasserin aut Gammaldi, V. verfasserin aut Gasbarra, C. verfasserin aut Ghalumyan, A. verfasserin aut Ghirlanda, G. verfasserin aut Giarrusso, M. verfasserin aut Giavitto, G. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Giroletti, M. verfasserin aut Giuliani, A. verfasserin aut Giunti, L. verfasserin aut Godinovic, N. verfasserin aut Coelho, J. Goulart verfasserin aut Gréaux, L. verfasserin aut Green, D. verfasserin aut Grondin, M.-H. verfasserin aut Gueta, O. verfasserin aut Gunji, S. verfasserin aut Hassan, T. verfasserin aut Heller, M. verfasserin aut Hernández-Cadena, S. verfasserin aut Hinton, J. verfasserin aut Hnatyk, B. verfasserin aut Hnatyk, R. verfasserin aut Hoffmann, D. verfasserin aut Hofmann, W. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Horvath, P. verfasserin aut Hrabovsky, M. verfasserin aut Hrupec, D. verfasserin aut Inada, T. verfasserin aut Incardona, F. verfasserin aut Inoue, S. verfasserin aut Ishio, K. verfasserin aut Jamrozy, M. verfasserin aut Janecek, P. verfasserin aut Martínez, I. Jiménez verfasserin aut Jin, W. verfasserin aut Jung-Richardt, I. verfasserin aut Jurysek, J. verfasserin aut Kaaret, P. verfasserin aut Karas, V. verfasserin aut Katz, U. verfasserin aut Kerszberg, D. verfasserin aut Khélifi, B. verfasserin aut Kieda, D.B. verfasserin aut Kissmann, R. verfasserin aut Kleiner, T. verfasserin aut Kluge, G. verfasserin aut Kluzniak, W. verfasserin aut Knödlseder, J. verfasserin aut Kobayashi, Y. verfasserin aut Kohri, K. verfasserin aut Komin, N. verfasserin aut Kornecki, P. verfasserin aut Kubo, H. verfasserin aut La Palombara, N. verfasserin aut Láinez, M. verfasserin aut Lamastra, A. verfasserin aut Lapington, J. verfasserin aut Lemoine-Goumard, M. verfasserin aut Lenain, J.-P. verfasserin aut Leone, F. verfasserin aut Leto, G. verfasserin aut Leuschner, F. verfasserin aut Lindfors, E. verfasserin aut Liodakis, I. verfasserin aut Lohse, T. verfasserin aut Lombardi, S. verfasserin aut Longo, F. verfasserin aut López-Coto, R. verfasserin aut López-Moya, M. verfasserin aut López-Oramas, A. verfasserin aut Loporchio, S. verfasserin aut Luque-Escamilla, P.L. verfasserin aut Macias, O. verfasserin aut Mackey, J. verfasserin aut Majumdar, P. verfasserin aut Mandat, D. verfasserin aut Manganaro, M. verfasserin aut Manicò, G. verfasserin aut Marconi, M. verfasserin aut Martí, J. verfasserin aut Martínez, G. verfasserin aut Martinez, M. verfasserin aut Martinez, O. verfasserin aut Mello, A.J.T.S. verfasserin aut Menchiari, S. verfasserin aut Meyer, D.M.-A. verfasserin aut Micanovic, S. verfasserin aut Miceli, D. verfasserin aut Miceli, M. verfasserin aut Michalowski, J. verfasserin aut Miener, T. verfasserin aut Miranda, J.M. verfasserin aut Mitchell, A. verfasserin aut Mode, B. verfasserin aut Moderski, R. verfasserin aut Mohrmann, L. verfasserin aut Molina, E. verfasserin aut Montaruli, T. verfasserin aut Morcuende, D. verfasserin aut Morlino, G. verfasserin aut Morselli, A. verfasserin aut Mosè, M. verfasserin aut Moulin, E. verfasserin aut Mukherjee, R. verfasserin aut Munari, K. verfasserin aut Murach, T. verfasserin aut Nagai, A. verfasserin aut Nagataki, S. verfasserin aut Nemmen, R. verfasserin aut Niemiec, J. verfasserin aut Nieto, D. verfasserin aut Rosillo, M. Nievas verfasserin aut Nikolajuk, M. verfasserin aut Nishijima, K. verfasserin aut Noda, K. verfasserin aut Novosyadlyj, B. verfasserin aut Nozaki, S. verfasserin aut Ohishi, M. verfasserin aut Ohm, S. verfasserin aut Ohtani, Y. verfasserin aut Okumura, A. verfasserin aut Olmi, B. verfasserin aut Ong, R.A. verfasserin aut Orienti, M. verfasserin aut Orito, R. verfasserin aut Orlandini, M. verfasserin aut Orlando, E. verfasserin aut Orlando, S. verfasserin aut Ostrowski, M. verfasserin aut Oya, I. verfasserin aut Pantaleo, F.R. verfasserin aut Paredes, J.M. verfasserin aut Patricelli, B. verfasserin aut Pecimotika, M. verfasserin aut Peresano, M. verfasserin aut Pérez-Romero, J. verfasserin aut Persic, M. verfasserin aut Petruk, O. verfasserin aut Piano, G. verfasserin aut Pietropaolo, E. verfasserin aut Pirola, G. verfasserin aut Pittori, C. verfasserin aut Pohl, M. verfasserin aut Ponti, G. verfasserin aut Prandini, E. verfasserin aut Principe, G. verfasserin aut Priyadarshi, C. verfasserin aut Pueschel, E. verfasserin aut Pühlhofer, G. verfasserin aut Pumo, M.L. verfasserin aut Quirrenbach, A. verfasserin aut Rando, R. verfasserin aut Razzaque, S. verfasserin aut Reichherzer, P. verfasserin aut Reimer, A. verfasserin aut Reimer, O. verfasserin aut Renaud, M. verfasserin aut Reposeur, T. verfasserin aut Ribó, M. verfasserin aut Richtler, T. verfasserin aut Rico, J. verfasserin aut Rieger, F. verfasserin aut Rigoselli, M. verfasserin aut Riitano, L. verfasserin aut Rizi, V. verfasserin aut Roache, E. verfasserin aut Romano, P. verfasserin aut Romeo, G. verfasserin aut Rosado, J. verfasserin aut Rowell, G. verfasserin aut Rudak, B. verfasserin aut Sadeh, I. verfasserin aut Safi-Harb, S. verfasserin aut Saha, L. verfasserin aut Sailer, S. verfasserin aut Sánchez-Conde, M. verfasserin aut Sarkar, S. verfasserin aut Satalecka, K. verfasserin aut Saturni, F.G. verfasserin aut Scherer, A. verfasserin aut Schovánek, P. verfasserin aut Schussler, F. verfasserin aut Schwanke, U. verfasserin aut Scuderi, S. verfasserin aut Seglar-Arroyo, M. verfasserin aut Sergijenko, O. verfasserin aut Servillat, M. verfasserin aut Shang, R.-Y. verfasserin aut Sharma, P. verfasserin aut Siejkowski, H. verfasserin aut Sliusar, V. verfasserin aut Słowikowska, A. verfasserin aut Sol, H. verfasserin aut Specovius, A. verfasserin aut Spencer, S.T. verfasserin aut Spengler, G. verfasserin aut Stamerra, A. verfasserin aut Stanič, S. verfasserin aut Starecki, T. verfasserin aut Starling, R. verfasserin aut Stolarczyk, T. verfasserin aut Pereira, L.A. Stuani verfasserin aut Suda, Y. verfasserin aut Suomijarvi, T. verfasserin aut Sushch, I. verfasserin aut Tajima, H. verfasserin aut Tam, P.-H.T. verfasserin aut Tanaka, S.J. verfasserin aut Tavecchio, F. verfasserin aut Testa, V. verfasserin aut Tian, W. verfasserin aut Tibaldo, L. verfasserin aut Torres, D.F. verfasserin aut Tothill, N. verfasserin aut Vallage, B. verfasserin aut Vallania, P. verfasserin aut van Eldik, C. verfasserin aut van Scherpenberg, J. verfasserin aut Vandenbroucke, J. verfasserin aut Acosta, M. 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allfields_unstemmed	10.1016/j.astropartphys.2023.102850 doi (DE-627)ELV009642641 (ELSEVIER)S0927-6505(23)00036-1 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Acero, F. verfasserin aut Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source. Gamma rays: general Cosmic rays Galactic PeVatrons (Stars:) supernovae: general Methods: data analysis Methods: statistical Acharyya, A. verfasserin aut Adam, R. verfasserin aut Aguasca-Cabot, A. verfasserin aut Agudo, I. verfasserin aut Aguirre-Santaella, A. verfasserin aut Alfaro, J. verfasserin aut Aloisio, R. verfasserin aut Crespo, N. Álvarez verfasserin aut Batista, R. Alves verfasserin aut Amati, L. verfasserin aut Amato, E. verfasserin aut Ambrosi, G. verfasserin aut Angüner, E.O. verfasserin aut Aramo, C. verfasserin aut Arcaro, C. verfasserin aut Armstrong, T. verfasserin aut Asano, K. verfasserin aut Ascasibar, Y. verfasserin aut Aschersleben, J. verfasserin aut Backes, M. verfasserin aut Baktash, A. verfasserin aut Balazs, C. verfasserin aut Balbo, M. verfasserin aut Ballet, J. verfasserin aut Larriva, A. Baquero verfasserin aut Martins, V. Barbosa verfasserin aut de Almeida, U. Barres verfasserin aut Barrio, J.A. verfasserin aut Bastieri, D. verfasserin aut Baxter, J.R. verfasserin aut Tjus, J. Becker verfasserin aut Benbow, W. verfasserin aut Bernardos-Martín, M.I. verfasserin aut Bernete, J. verfasserin aut Berti, A. verfasserin aut Bertucci, B. verfasserin aut Beshley, V. verfasserin aut Bhattacharjee, P. verfasserin aut Bhattacharyya, S. verfasserin aut Biland, A. verfasserin aut Bissaldi, E. verfasserin aut Biteau, J. verfasserin aut Blanch, O. verfasserin aut Bordas, P. verfasserin aut Bottacini, E. verfasserin aut Bregeon, J. verfasserin aut Brose, R. verfasserin aut Bucciantini, N. verfasserin aut Bulgarelli, A. verfasserin aut Capasso, M. verfasserin aut Dolcetta, R.A. Capuzzo verfasserin aut Caraveo, P. verfasserin aut Cardillo, M. verfasserin aut Carosi, R. verfasserin aut Casanova, S. verfasserin aut Cascone, E. verfasserin aut Cassol, F. verfasserin aut Catalani, F. verfasserin aut Cerruti, M. verfasserin aut Chadwick, P. verfasserin aut Chaty, S. verfasserin aut Chen, A. verfasserin aut Chernyakova, M. verfasserin aut Chiavassa, A. verfasserin aut Chudoba, J. verfasserin aut Coimbra-Araujo, C. verfasserin aut Conforti, V. verfasserin aut Contreras, J.L. verfasserin aut Costa, A. verfasserin aut Costantini, H. verfasserin aut Cristofari, P. verfasserin aut Crocker, R. verfasserin aut D’Amico, G. verfasserin aut D’Ammando, F. verfasserin aut De Angelis, A. verfasserin aut De Caprio, V. verfasserin aut de Gouveia Dal Pino, E.M. verfasserin aut de Ona Wilhelmi, E. verfasserin aut de Souza, V. verfasserin aut Delgado, C. verfasserin aut della Volpe, D. verfasserin aut Depaoli, D. verfasserin aut Di Girolamo, T. verfasserin aut Di Pierro, F. verfasserin aut Di Tria, R. verfasserin aut Di Venere, L. verfasserin aut Diebold, S. verfasserin aut Djuvsland, J.I. verfasserin aut Donini, A. verfasserin aut Doro, M. verfasserin aut Dos Anjos, R.d.C. verfasserin aut Dwarkadas, V.V. verfasserin aut Einecke, S. verfasserin aut Elsässer, D. verfasserin aut Emery, G. verfasserin aut Evoli, C. verfasserin aut Falceta-Goncalves, D. verfasserin aut Fedorova, E. verfasserin aut Fegan, S. verfasserin aut Ferrand, G. verfasserin aut Fiandrini, E. verfasserin aut Filipovic, M. verfasserin aut Fioretti, V. verfasserin aut Fiori, M. verfasserin aut Foffano, L. verfasserin aut Fontaine, G. verfasserin aut Fukami, S. verfasserin aut Galanti, G. verfasserin aut Galaz, G. verfasserin aut Gammaldi, V. verfasserin aut Gasbarra, C. verfasserin aut Ghalumyan, A. verfasserin aut Ghirlanda, G. verfasserin aut Giarrusso, M. verfasserin aut Giavitto, G. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Giroletti, M. verfasserin aut Giuliani, A. verfasserin aut Giunti, L. verfasserin aut Godinovic, N. verfasserin aut Coelho, J. Goulart verfasserin aut Gréaux, L. verfasserin aut Green, D. verfasserin aut Grondin, M.-H. verfasserin aut Gueta, O. verfasserin aut Gunji, S. verfasserin aut Hassan, T. verfasserin aut Heller, M. verfasserin aut Hernández-Cadena, S. verfasserin aut Hinton, J. verfasserin aut Hnatyk, B. verfasserin aut Hnatyk, R. verfasserin aut Hoffmann, D. verfasserin aut Hofmann, W. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Horvath, P. verfasserin aut Hrabovsky, M. verfasserin aut Hrupec, D. verfasserin aut Inada, T. verfasserin aut Incardona, F. verfasserin aut Inoue, S. verfasserin aut Ishio, K. verfasserin aut Jamrozy, M. verfasserin aut Janecek, P. verfasserin aut Martínez, I. Jiménez verfasserin aut Jin, W. verfasserin aut Jung-Richardt, I. verfasserin aut Jurysek, J. verfasserin aut Kaaret, P. verfasserin aut Karas, V. verfasserin aut Katz, U. verfasserin aut Kerszberg, D. verfasserin aut Khélifi, B. verfasserin aut Kieda, D.B. verfasserin aut Kissmann, R. verfasserin aut Kleiner, T. verfasserin aut Kluge, G. verfasserin aut Kluzniak, W. verfasserin aut Knödlseder, J. verfasserin aut Kobayashi, Y. verfasserin aut Kohri, K. verfasserin aut Komin, N. verfasserin aut Kornecki, P. verfasserin aut Kubo, H. verfasserin aut La Palombara, N. verfasserin aut Láinez, M. verfasserin aut Lamastra, A. verfasserin aut Lapington, J. verfasserin aut Lemoine-Goumard, M. verfasserin aut Lenain, J.-P. verfasserin aut Leone, F. verfasserin aut Leto, G. verfasserin aut Leuschner, F. verfasserin aut Lindfors, E. verfasserin aut Liodakis, I. verfasserin aut Lohse, T. verfasserin aut Lombardi, S. verfasserin aut Longo, F. verfasserin aut López-Coto, R. verfasserin aut López-Moya, M. verfasserin aut López-Oramas, A. verfasserin aut Loporchio, S. verfasserin aut Luque-Escamilla, P.L. verfasserin aut Macias, O. verfasserin aut Mackey, J. verfasserin aut Majumdar, P. verfasserin aut Mandat, D. verfasserin aut Manganaro, M. verfasserin aut Manicò, G. verfasserin aut Marconi, M. verfasserin aut Martí, J. verfasserin aut Martínez, G. verfasserin aut Martinez, M. verfasserin aut Martinez, O. verfasserin aut Mello, A.J.T.S. verfasserin aut Menchiari, S. verfasserin aut Meyer, D.M.-A. verfasserin aut Micanovic, S. verfasserin aut Miceli, D. verfasserin aut Miceli, M. verfasserin aut Michalowski, J. verfasserin aut Miener, T. verfasserin aut Miranda, J.M. verfasserin aut Mitchell, A. verfasserin aut Mode, B. verfasserin aut Moderski, R. verfasserin aut Mohrmann, L. verfasserin aut Molina, E. verfasserin aut Montaruli, T. verfasserin aut Morcuende, D. verfasserin aut Morlino, G. verfasserin aut Morselli, A. verfasserin aut Mosè, M. verfasserin aut Moulin, E. verfasserin aut Mukherjee, R. verfasserin aut Munari, K. verfasserin aut Murach, T. verfasserin aut Nagai, A. verfasserin aut Nagataki, S. verfasserin aut Nemmen, R. verfasserin aut Niemiec, J. verfasserin aut Nieto, D. verfasserin aut Rosillo, M. Nievas verfasserin aut Nikolajuk, M. verfasserin aut Nishijima, K. verfasserin aut Noda, K. verfasserin aut Novosyadlyj, B. verfasserin aut Nozaki, S. verfasserin aut Ohishi, M. verfasserin aut Ohm, S. verfasserin aut Ohtani, Y. verfasserin aut Okumura, A. verfasserin aut Olmi, B. verfasserin aut Ong, R.A. verfasserin aut Orienti, M. verfasserin aut Orito, R. verfasserin aut Orlandini, M. verfasserin aut Orlando, E. verfasserin aut Orlando, S. verfasserin aut Ostrowski, M. verfasserin aut Oya, I. verfasserin aut Pantaleo, F.R. verfasserin aut Paredes, J.M. verfasserin aut Patricelli, B. verfasserin aut Pecimotika, M. verfasserin aut Peresano, M. verfasserin aut Pérez-Romero, J. verfasserin aut Persic, M. verfasserin aut Petruk, O. verfasserin aut Piano, G. verfasserin aut Pietropaolo, E. verfasserin aut Pirola, G. verfasserin aut Pittori, C. verfasserin aut Pohl, M. verfasserin aut Ponti, G. verfasserin aut Prandini, E. verfasserin aut Principe, G. verfasserin aut Priyadarshi, C. verfasserin aut Pueschel, E. verfasserin aut Pühlhofer, G. verfasserin aut Pumo, M.L. verfasserin aut Quirrenbach, A. verfasserin aut Rando, R. verfasserin aut Razzaque, S. verfasserin aut Reichherzer, P. verfasserin aut Reimer, A. verfasserin aut Reimer, O. verfasserin aut Renaud, M. verfasserin aut Reposeur, T. verfasserin aut Ribó, M. verfasserin aut Richtler, T. verfasserin aut Rico, J. verfasserin aut Rieger, F. verfasserin aut Rigoselli, M. verfasserin aut Riitano, L. verfasserin aut Rizi, V. verfasserin aut Roache, E. verfasserin aut Romano, P. verfasserin aut Romeo, G. verfasserin aut Rosado, J. verfasserin aut Rowell, G. verfasserin aut Rudak, B. verfasserin aut Sadeh, I. verfasserin aut Safi-Harb, S. verfasserin aut Saha, L. verfasserin aut Sailer, S. verfasserin aut Sánchez-Conde, M. verfasserin aut Sarkar, S. verfasserin aut Satalecka, K. verfasserin aut Saturni, F.G. verfasserin aut Scherer, A. verfasserin aut Schovánek, P. verfasserin aut Schussler, F. verfasserin aut Schwanke, U. verfasserin aut Scuderi, S. verfasserin aut Seglar-Arroyo, M. verfasserin aut Sergijenko, O. verfasserin aut Servillat, M. verfasserin aut Shang, R.-Y. verfasserin aut Sharma, P. verfasserin aut Siejkowski, H. verfasserin aut Sliusar, V. verfasserin aut Słowikowska, A. verfasserin aut Sol, H. verfasserin aut Specovius, A. verfasserin aut Spencer, S.T. verfasserin aut Spengler, G. verfasserin aut Stamerra, A. verfasserin aut Stanič, S. verfasserin aut Starecki, T. verfasserin aut Starling, R. verfasserin aut Stolarczyk, T. verfasserin aut Pereira, L.A. Stuani verfasserin aut Suda, Y. verfasserin aut Suomijarvi, T. verfasserin aut Sushch, I. verfasserin aut Tajima, H. verfasserin aut Tam, P.-H.T. verfasserin aut Tanaka, S.J. verfasserin aut Tavecchio, F. verfasserin aut Testa, V. verfasserin aut Tian, W. verfasserin aut Tibaldo, L. verfasserin aut Torres, D.F. verfasserin aut Tothill, N. verfasserin aut Vallage, B. verfasserin aut Vallania, P. verfasserin aut van Eldik, C. verfasserin aut van Scherpenberg, J. verfasserin aut Vandenbroucke, J. verfasserin aut Acosta, M. Vazquez verfasserin aut Vecchi, M. verfasserin aut Vercellone, S. verfasserin aut Verna, G. verfasserin aut Viana, A. verfasserin aut Vignatti, J. verfasserin aut Vitale, V. verfasserin aut Vodeb, V. verfasserin aut Vorobiov, S. verfasserin aut Vuillaume, T. verfasserin aut Wagner, S.J. verfasserin aut Walter, R. verfasserin aut White, M. verfasserin aut Wierzcholska, A. verfasserin aut Will, M. verfasserin aut Williams, D. verfasserin aut Yang, L. verfasserin aut Yoshida, T. verfasserin aut Yoshikoshi, T. verfasserin aut Zaharijas, G. verfasserin aut Zampieri, L. verfasserin aut Zavrtanik, D. verfasserin aut Zavrtanik, M. verfasserin aut Zhdanov, V.I. verfasserin aut Z̆ivec, M. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 150 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:150 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.22 Astrophysik AR 150
allfieldsGer	10.1016/j.astropartphys.2023.102850 doi (DE-627)ELV009642641 (ELSEVIER)S0927-6505(23)00036-1 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Acero, F. verfasserin aut Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source. Gamma rays: general Cosmic rays Galactic PeVatrons (Stars:) supernovae: general Methods: data analysis Methods: statistical Acharyya, A. verfasserin aut Adam, R. verfasserin aut Aguasca-Cabot, A. verfasserin aut Agudo, I. verfasserin aut Aguirre-Santaella, A. verfasserin aut Alfaro, J. verfasserin aut Aloisio, R. verfasserin aut Crespo, N. Álvarez verfasserin aut Batista, R. Alves verfasserin aut Amati, L. verfasserin aut Amato, E. verfasserin aut Ambrosi, G. verfasserin aut Angüner, E.O. verfasserin aut Aramo, C. verfasserin aut Arcaro, C. verfasserin aut Armstrong, T. verfasserin aut Asano, K. verfasserin aut Ascasibar, Y. verfasserin aut Aschersleben, J. verfasserin aut Backes, M. verfasserin aut Baktash, A. verfasserin aut Balazs, C. verfasserin aut Balbo, M. verfasserin aut Ballet, J. verfasserin aut Larriva, A. Baquero verfasserin aut Martins, V. Barbosa verfasserin aut de Almeida, U. Barres verfasserin aut Barrio, J.A. verfasserin aut Bastieri, D. verfasserin aut Baxter, J.R. verfasserin aut Tjus, J. Becker verfasserin aut Benbow, W. verfasserin aut Bernardos-Martín, M.I. verfasserin aut Bernete, J. verfasserin aut Berti, A. verfasserin aut Bertucci, B. verfasserin aut Beshley, V. verfasserin aut Bhattacharjee, P. verfasserin aut Bhattacharyya, S. verfasserin aut Biland, A. verfasserin aut Bissaldi, E. verfasserin aut Biteau, J. verfasserin aut Blanch, O. verfasserin aut Bordas, P. verfasserin aut Bottacini, E. verfasserin aut Bregeon, J. verfasserin aut Brose, R. verfasserin aut Bucciantini, N. verfasserin aut Bulgarelli, A. verfasserin aut Capasso, M. verfasserin aut Dolcetta, R.A. Capuzzo verfasserin aut Caraveo, P. verfasserin aut Cardillo, M. verfasserin aut Carosi, R. verfasserin aut Casanova, S. verfasserin aut Cascone, E. verfasserin aut Cassol, F. verfasserin aut Catalani, F. verfasserin aut Cerruti, M. verfasserin aut Chadwick, P. verfasserin aut Chaty, S. verfasserin aut Chen, A. verfasserin aut Chernyakova, M. verfasserin aut Chiavassa, A. verfasserin aut Chudoba, J. verfasserin aut Coimbra-Araujo, C. verfasserin aut Conforti, V. verfasserin aut Contreras, J.L. verfasserin aut Costa, A. verfasserin aut Costantini, H. verfasserin aut Cristofari, P. verfasserin aut Crocker, R. verfasserin aut D’Amico, G. verfasserin aut D’Ammando, F. verfasserin aut De Angelis, A. verfasserin aut De Caprio, V. verfasserin aut de Gouveia Dal Pino, E.M. verfasserin aut de Ona Wilhelmi, E. verfasserin aut de Souza, V. verfasserin aut Delgado, C. verfasserin aut della Volpe, D. verfasserin aut Depaoli, D. verfasserin aut Di Girolamo, T. verfasserin aut Di Pierro, F. verfasserin aut Di Tria, R. verfasserin aut Di Venere, L. verfasserin aut Diebold, S. verfasserin aut Djuvsland, J.I. verfasserin aut Donini, A. verfasserin aut Doro, M. verfasserin aut Dos Anjos, R.d.C. verfasserin aut Dwarkadas, V.V. verfasserin aut Einecke, S. verfasserin aut Elsässer, D. verfasserin aut Emery, G. verfasserin aut Evoli, C. verfasserin aut Falceta-Goncalves, D. verfasserin aut Fedorova, E. verfasserin aut Fegan, S. verfasserin aut Ferrand, G. verfasserin aut Fiandrini, E. verfasserin aut Filipovic, M. verfasserin aut Fioretti, V. verfasserin aut Fiori, M. verfasserin aut Foffano, L. verfasserin aut Fontaine, G. verfasserin aut Fukami, S. verfasserin aut Galanti, G. verfasserin aut Galaz, G. verfasserin aut Gammaldi, V. verfasserin aut Gasbarra, C. verfasserin aut Ghalumyan, A. verfasserin aut Ghirlanda, G. verfasserin aut Giarrusso, M. verfasserin aut Giavitto, G. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Giroletti, M. verfasserin aut Giuliani, A. verfasserin aut Giunti, L. verfasserin aut Godinovic, N. verfasserin aut Coelho, J. Goulart verfasserin aut Gréaux, L. verfasserin aut Green, D. verfasserin aut Grondin, M.-H. verfasserin aut Gueta, O. verfasserin aut Gunji, S. verfasserin aut Hassan, T. verfasserin aut Heller, M. verfasserin aut Hernández-Cadena, S. verfasserin aut Hinton, J. verfasserin aut Hnatyk, B. verfasserin aut Hnatyk, R. verfasserin aut Hoffmann, D. verfasserin aut Hofmann, W. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Horvath, P. verfasserin aut Hrabovsky, M. verfasserin aut Hrupec, D. verfasserin aut Inada, T. verfasserin aut Incardona, F. verfasserin aut Inoue, S. verfasserin aut Ishio, K. verfasserin aut Jamrozy, M. verfasserin aut Janecek, P. verfasserin aut Martínez, I. Jiménez verfasserin aut Jin, W. verfasserin aut Jung-Richardt, I. verfasserin aut Jurysek, J. verfasserin aut Kaaret, P. verfasserin aut Karas, V. verfasserin aut Katz, U. verfasserin aut Kerszberg, D. verfasserin aut Khélifi, B. verfasserin aut Kieda, D.B. verfasserin aut Kissmann, R. verfasserin aut Kleiner, T. verfasserin aut Kluge, G. verfasserin aut Kluzniak, W. verfasserin aut Knödlseder, J. verfasserin aut Kobayashi, Y. verfasserin aut Kohri, K. verfasserin aut Komin, N. verfasserin aut Kornecki, P. verfasserin aut Kubo, H. verfasserin aut La Palombara, N. verfasserin aut Láinez, M. verfasserin aut Lamastra, A. verfasserin aut Lapington, J. verfasserin aut Lemoine-Goumard, M. verfasserin aut Lenain, J.-P. verfasserin aut Leone, F. verfasserin aut Leto, G. verfasserin aut Leuschner, F. verfasserin aut Lindfors, E. verfasserin aut Liodakis, I. verfasserin aut Lohse, T. verfasserin aut Lombardi, S. verfasserin aut Longo, F. verfasserin aut López-Coto, R. verfasserin aut López-Moya, M. verfasserin aut López-Oramas, A. verfasserin aut Loporchio, S. verfasserin aut Luque-Escamilla, P.L. verfasserin aut Macias, O. verfasserin aut Mackey, J. verfasserin aut Majumdar, P. verfasserin aut Mandat, D. verfasserin aut Manganaro, M. verfasserin aut Manicò, G. verfasserin aut Marconi, M. verfasserin aut Martí, J. verfasserin aut Martínez, G. verfasserin aut Martinez, M. verfasserin aut Martinez, O. verfasserin aut Mello, A.J.T.S. verfasserin aut Menchiari, S. verfasserin aut Meyer, D.M.-A. verfasserin aut Micanovic, S. verfasserin aut Miceli, D. verfasserin aut Miceli, M. verfasserin aut Michalowski, J. verfasserin aut Miener, T. verfasserin aut Miranda, J.M. verfasserin aut Mitchell, A. verfasserin aut Mode, B. verfasserin aut Moderski, R. verfasserin aut Mohrmann, L. verfasserin aut Molina, E. verfasserin aut Montaruli, T. verfasserin aut Morcuende, D. verfasserin aut Morlino, G. verfasserin aut Morselli, A. verfasserin aut Mosè, M. verfasserin aut Moulin, E. verfasserin aut Mukherjee, R. verfasserin aut Munari, K. verfasserin aut Murach, T. verfasserin aut Nagai, A. verfasserin aut Nagataki, S. verfasserin aut Nemmen, R. verfasserin aut Niemiec, J. verfasserin aut Nieto, D. verfasserin aut Rosillo, M. Nievas verfasserin aut Nikolajuk, M. verfasserin aut Nishijima, K. verfasserin aut Noda, K. verfasserin aut Novosyadlyj, B. verfasserin aut Nozaki, S. verfasserin aut Ohishi, M. verfasserin aut Ohm, S. verfasserin aut Ohtani, Y. verfasserin aut Okumura, A. verfasserin aut Olmi, B. verfasserin aut Ong, R.A. verfasserin aut Orienti, M. verfasserin aut Orito, R. verfasserin aut Orlandini, M. verfasserin aut Orlando, E. verfasserin aut Orlando, S. verfasserin aut Ostrowski, M. verfasserin aut Oya, I. verfasserin aut Pantaleo, F.R. verfasserin aut Paredes, J.M. verfasserin aut Patricelli, B. verfasserin aut Pecimotika, M. verfasserin aut Peresano, M. verfasserin aut Pérez-Romero, J. verfasserin aut Persic, M. verfasserin aut Petruk, O. verfasserin aut Piano, G. verfasserin aut Pietropaolo, E. verfasserin aut Pirola, G. verfasserin aut Pittori, C. verfasserin aut Pohl, M. verfasserin aut Ponti, G. verfasserin aut Prandini, E. verfasserin aut Principe, G. verfasserin aut Priyadarshi, C. verfasserin aut Pueschel, E. verfasserin aut Pühlhofer, G. verfasserin aut Pumo, M.L. verfasserin aut Quirrenbach, A. verfasserin aut Rando, R. verfasserin aut Razzaque, S. verfasserin aut Reichherzer, P. verfasserin aut Reimer, A. verfasserin aut Reimer, O. verfasserin aut Renaud, M. verfasserin aut Reposeur, T. verfasserin aut Ribó, M. verfasserin aut Richtler, T. verfasserin aut Rico, J. verfasserin aut Rieger, F. verfasserin aut Rigoselli, M. verfasserin aut Riitano, L. verfasserin aut Rizi, V. verfasserin aut Roache, E. verfasserin aut Romano, P. verfasserin aut Romeo, G. verfasserin aut Rosado, J. verfasserin aut Rowell, G. verfasserin aut Rudak, B. verfasserin aut Sadeh, I. verfasserin aut Safi-Harb, S. verfasserin aut Saha, L. verfasserin aut Sailer, S. verfasserin aut Sánchez-Conde, M. verfasserin aut Sarkar, S. verfasserin aut Satalecka, K. verfasserin aut Saturni, F.G. verfasserin aut Scherer, A. verfasserin aut Schovánek, P. verfasserin aut Schussler, F. verfasserin aut Schwanke, U. verfasserin aut Scuderi, S. verfasserin aut Seglar-Arroyo, M. verfasserin aut Sergijenko, O. verfasserin aut Servillat, M. verfasserin aut Shang, R.-Y. verfasserin aut Sharma, P. verfasserin aut Siejkowski, H. verfasserin aut Sliusar, V. verfasserin aut Słowikowska, A. verfasserin aut Sol, H. verfasserin aut Specovius, A. verfasserin aut Spencer, S.T. verfasserin aut Spengler, G. verfasserin aut Stamerra, A. verfasserin aut Stanič, S. verfasserin aut Starecki, T. verfasserin aut Starling, R. verfasserin aut Stolarczyk, T. verfasserin aut Pereira, L.A. Stuani verfasserin aut Suda, Y. verfasserin aut Suomijarvi, T. verfasserin aut Sushch, I. verfasserin aut Tajima, H. verfasserin aut Tam, P.-H.T. verfasserin aut Tanaka, S.J. verfasserin aut Tavecchio, F. verfasserin aut Testa, V. verfasserin aut Tian, W. verfasserin aut Tibaldo, L. verfasserin aut Torres, D.F. verfasserin aut Tothill, N. verfasserin aut Vallage, B. verfasserin aut Vallania, P. verfasserin aut van Eldik, C. verfasserin aut van Scherpenberg, J. verfasserin aut Vandenbroucke, J. verfasserin aut Acosta, M. Vazquez verfasserin aut Vecchi, M. verfasserin aut Vercellone, S. verfasserin aut Verna, G. verfasserin aut Viana, A. verfasserin aut Vignatti, J. verfasserin aut Vitale, V. verfasserin aut Vodeb, V. verfasserin aut Vorobiov, S. verfasserin aut Vuillaume, T. verfasserin aut Wagner, S.J. verfasserin aut Walter, R. verfasserin aut White, M. verfasserin aut Wierzcholska, A. verfasserin aut Will, M. verfasserin aut Williams, D. verfasserin aut Yang, L. verfasserin aut Yoshida, T. verfasserin aut Yoshikoshi, T. verfasserin aut Zaharijas, G. verfasserin aut Zampieri, L. verfasserin aut Zavrtanik, D. verfasserin aut Zavrtanik, M. verfasserin aut Zhdanov, V.I. verfasserin aut Z̆ivec, M. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 150 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:150 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.22 Astrophysik AR 150
allfieldsSound	10.1016/j.astropartphys.2023.102850 doi (DE-627)ELV009642641 (ELSEVIER)S0927-6505(23)00036-1 DE-627 ger DE-627 rda eng 540 DE-600 39.22 bkl Acero, F. verfasserin aut Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source. Gamma rays: general Cosmic rays Galactic PeVatrons (Stars:) supernovae: general Methods: data analysis Methods: statistical Acharyya, A. verfasserin aut Adam, R. verfasserin aut Aguasca-Cabot, A. verfasserin aut Agudo, I. verfasserin aut Aguirre-Santaella, A. verfasserin aut Alfaro, J. verfasserin aut Aloisio, R. verfasserin aut Crespo, N. Álvarez verfasserin aut Batista, R. Alves verfasserin aut Amati, L. verfasserin aut Amato, E. verfasserin aut Ambrosi, G. verfasserin aut Angüner, E.O. verfasserin aut Aramo, C. verfasserin aut Arcaro, C. verfasserin aut Armstrong, T. verfasserin aut Asano, K. verfasserin aut Ascasibar, Y. verfasserin aut Aschersleben, J. verfasserin aut Backes, M. verfasserin aut Baktash, A. verfasserin aut Balazs, C. verfasserin aut Balbo, M. verfasserin aut Ballet, J. verfasserin aut Larriva, A. Baquero verfasserin aut Martins, V. Barbosa verfasserin aut de Almeida, U. Barres verfasserin aut Barrio, J.A. verfasserin aut Bastieri, D. verfasserin aut Baxter, J.R. verfasserin aut Tjus, J. Becker verfasserin aut Benbow, W. verfasserin aut Bernardos-Martín, M.I. verfasserin aut Bernete, J. verfasserin aut Berti, A. verfasserin aut Bertucci, B. verfasserin aut Beshley, V. verfasserin aut Bhattacharjee, P. verfasserin aut Bhattacharyya, S. verfasserin aut Biland, A. verfasserin aut Bissaldi, E. verfasserin aut Biteau, J. verfasserin aut Blanch, O. verfasserin aut Bordas, P. verfasserin aut Bottacini, E. verfasserin aut Bregeon, J. verfasserin aut Brose, R. verfasserin aut Bucciantini, N. verfasserin aut Bulgarelli, A. verfasserin aut Capasso, M. verfasserin aut Dolcetta, R.A. Capuzzo verfasserin aut Caraveo, P. verfasserin aut Cardillo, M. verfasserin aut Carosi, R. verfasserin aut Casanova, S. verfasserin aut Cascone, E. verfasserin aut Cassol, F. verfasserin aut Catalani, F. verfasserin aut Cerruti, M. verfasserin aut Chadwick, P. verfasserin aut Chaty, S. verfasserin aut Chen, A. verfasserin aut Chernyakova, M. verfasserin aut Chiavassa, A. verfasserin aut Chudoba, J. verfasserin aut Coimbra-Araujo, C. verfasserin aut Conforti, V. verfasserin aut Contreras, J.L. verfasserin aut Costa, A. verfasserin aut Costantini, H. verfasserin aut Cristofari, P. verfasserin aut Crocker, R. verfasserin aut D’Amico, G. verfasserin aut D’Ammando, F. verfasserin aut De Angelis, A. verfasserin aut De Caprio, V. verfasserin aut de Gouveia Dal Pino, E.M. verfasserin aut de Ona Wilhelmi, E. verfasserin aut de Souza, V. verfasserin aut Delgado, C. verfasserin aut della Volpe, D. verfasserin aut Depaoli, D. verfasserin aut Di Girolamo, T. verfasserin aut Di Pierro, F. verfasserin aut Di Tria, R. verfasserin aut Di Venere, L. verfasserin aut Diebold, S. verfasserin aut Djuvsland, J.I. verfasserin aut Donini, A. verfasserin aut Doro, M. verfasserin aut Dos Anjos, R.d.C. verfasserin aut Dwarkadas, V.V. verfasserin aut Einecke, S. verfasserin aut Elsässer, D. verfasserin aut Emery, G. verfasserin aut Evoli, C. verfasserin aut Falceta-Goncalves, D. verfasserin aut Fedorova, E. verfasserin aut Fegan, S. verfasserin aut Ferrand, G. verfasserin aut Fiandrini, E. verfasserin aut Filipovic, M. verfasserin aut Fioretti, V. verfasserin aut Fiori, M. verfasserin aut Foffano, L. verfasserin aut Fontaine, G. verfasserin aut Fukami, S. verfasserin aut Galanti, G. verfasserin aut Galaz, G. verfasserin aut Gammaldi, V. verfasserin aut Gasbarra, C. verfasserin aut Ghalumyan, A. verfasserin aut Ghirlanda, G. verfasserin aut Giarrusso, M. verfasserin aut Giavitto, G. verfasserin aut Giglietto, N. verfasserin aut Giordano, F. verfasserin aut Giroletti, M. verfasserin aut Giuliani, A. verfasserin aut Giunti, L. verfasserin aut Godinovic, N. verfasserin aut Coelho, J. Goulart verfasserin aut Gréaux, L. verfasserin aut Green, D. verfasserin aut Grondin, M.-H. verfasserin aut Gueta, O. verfasserin aut Gunji, S. verfasserin aut Hassan, T. verfasserin aut Heller, M. verfasserin aut Hernández-Cadena, S. verfasserin aut Hinton, J. verfasserin aut Hnatyk, B. verfasserin aut Hnatyk, R. verfasserin aut Hoffmann, D. verfasserin aut Hofmann, W. verfasserin aut Holder, J. verfasserin aut Horan, D. verfasserin aut Horvath, P. verfasserin aut Hrabovsky, M. verfasserin aut Hrupec, D. verfasserin aut Inada, T. verfasserin aut Incardona, F. verfasserin aut Inoue, S. verfasserin aut Ishio, K. verfasserin aut Jamrozy, M. verfasserin aut Janecek, P. verfasserin aut Martínez, I. Jiménez verfasserin aut Jin, W. verfasserin aut Jung-Richardt, I. verfasserin aut Jurysek, J. verfasserin aut Kaaret, P. verfasserin aut Karas, V. verfasserin aut Katz, U. verfasserin aut Kerszberg, D. verfasserin aut Khélifi, B. verfasserin aut Kieda, D.B. verfasserin aut Kissmann, R. verfasserin aut Kleiner, T. verfasserin aut Kluge, G. verfasserin aut Kluzniak, W. verfasserin aut Knödlseder, J. verfasserin aut Kobayashi, Y. verfasserin aut Kohri, K. verfasserin aut Komin, N. verfasserin aut Kornecki, P. verfasserin aut Kubo, H. verfasserin aut La Palombara, N. verfasserin aut Láinez, M. verfasserin aut Lamastra, A. verfasserin aut Lapington, J. verfasserin aut Lemoine-Goumard, M. verfasserin aut Lenain, J.-P. verfasserin aut Leone, F. verfasserin aut Leto, G. verfasserin aut Leuschner, F. verfasserin aut Lindfors, E. verfasserin aut Liodakis, I. verfasserin aut Lohse, T. verfasserin aut Lombardi, S. verfasserin aut Longo, F. verfasserin aut López-Coto, R. verfasserin aut López-Moya, M. verfasserin aut López-Oramas, A. verfasserin aut Loporchio, S. verfasserin aut Luque-Escamilla, P.L. verfasserin aut Macias, O. verfasserin aut Mackey, J. verfasserin aut Majumdar, P. verfasserin aut Mandat, D. verfasserin aut Manganaro, M. verfasserin aut Manicò, G. verfasserin aut Marconi, M. verfasserin aut Martí, J. verfasserin aut Martínez, G. verfasserin aut Martinez, M. verfasserin aut Martinez, O. verfasserin aut Mello, A.J.T.S. verfasserin aut Menchiari, S. verfasserin aut Meyer, D.M.-A. verfasserin aut Micanovic, S. verfasserin aut Miceli, D. verfasserin aut Miceli, M. verfasserin aut Michalowski, J. verfasserin aut Miener, T. verfasserin aut Miranda, J.M. verfasserin aut Mitchell, A. verfasserin aut Mode, B. verfasserin aut Moderski, R. verfasserin aut Mohrmann, L. verfasserin aut Molina, E. verfasserin aut Montaruli, T. verfasserin aut Morcuende, D. verfasserin aut Morlino, G. verfasserin aut Morselli, A. verfasserin aut Mosè, M. verfasserin aut Moulin, E. verfasserin aut Mukherjee, R. verfasserin aut Munari, K. verfasserin aut Murach, T. verfasserin aut Nagai, A. verfasserin aut Nagataki, S. verfasserin aut Nemmen, R. verfasserin aut Niemiec, J. verfasserin aut Nieto, D. verfasserin aut Rosillo, M. Nievas verfasserin aut Nikolajuk, M. verfasserin aut Nishijima, K. verfasserin aut Noda, K. verfasserin aut Novosyadlyj, B. verfasserin aut Nozaki, S. verfasserin aut Ohishi, M. verfasserin aut Ohm, S. verfasserin aut Ohtani, Y. verfasserin aut Okumura, A. verfasserin aut Olmi, B. verfasserin aut Ong, R.A. verfasserin aut Orienti, M. verfasserin aut Orito, R. verfasserin aut Orlandini, M. verfasserin aut Orlando, E. verfasserin aut Orlando, S. verfasserin aut Ostrowski, M. verfasserin aut Oya, I. verfasserin aut Pantaleo, F.R. verfasserin aut Paredes, J.M. verfasserin aut Patricelli, B. verfasserin aut Pecimotika, M. verfasserin aut Peresano, M. verfasserin aut Pérez-Romero, J. verfasserin aut Persic, M. verfasserin aut Petruk, O. verfasserin aut Piano, G. verfasserin aut Pietropaolo, E. verfasserin aut Pirola, G. verfasserin aut Pittori, C. verfasserin aut Pohl, M. verfasserin aut Ponti, G. verfasserin aut Prandini, E. verfasserin aut Principe, G. verfasserin aut Priyadarshi, C. verfasserin aut Pueschel, E. verfasserin aut Pühlhofer, G. verfasserin aut Pumo, M.L. verfasserin aut Quirrenbach, A. verfasserin aut Rando, R. verfasserin aut Razzaque, S. verfasserin aut Reichherzer, P. verfasserin aut Reimer, A. verfasserin aut Reimer, O. verfasserin aut Renaud, M. verfasserin aut Reposeur, T. verfasserin aut Ribó, M. verfasserin aut Richtler, T. verfasserin aut Rico, J. verfasserin aut Rieger, F. verfasserin aut Rigoselli, M. verfasserin aut Riitano, L. verfasserin aut Rizi, V. verfasserin aut Roache, E. verfasserin aut Romano, P. verfasserin aut Romeo, G. verfasserin aut Rosado, J. verfasserin aut Rowell, G. verfasserin aut Rudak, B. verfasserin aut Sadeh, I. verfasserin aut Safi-Harb, S. verfasserin aut Saha, L. verfasserin aut Sailer, S. verfasserin aut Sánchez-Conde, M. verfasserin aut Sarkar, S. verfasserin aut Satalecka, K. verfasserin aut Saturni, F.G. verfasserin aut Scherer, A. verfasserin aut Schovánek, P. verfasserin aut Schussler, F. verfasserin aut Schwanke, U. verfasserin aut Scuderi, S. verfasserin aut Seglar-Arroyo, M. verfasserin aut Sergijenko, O. verfasserin aut Servillat, M. verfasserin aut Shang, R.-Y. verfasserin aut Sharma, P. verfasserin aut Siejkowski, H. verfasserin aut Sliusar, V. verfasserin aut Słowikowska, A. verfasserin aut Sol, H. verfasserin aut Specovius, A. verfasserin aut Spencer, S.T. verfasserin aut Spengler, G. verfasserin aut Stamerra, A. verfasserin aut Stanič, S. verfasserin aut Starecki, T. verfasserin aut Starling, R. verfasserin aut Stolarczyk, T. verfasserin aut Pereira, L.A. Stuani verfasserin aut Suda, Y. verfasserin aut Suomijarvi, T. verfasserin aut Sushch, I. verfasserin aut Tajima, H. verfasserin aut Tam, P.-H.T. verfasserin aut Tanaka, S.J. verfasserin aut Tavecchio, F. verfasserin aut Testa, V. verfasserin aut Tian, W. verfasserin aut Tibaldo, L. verfasserin aut Torres, D.F. verfasserin aut Tothill, N. verfasserin aut Vallage, B. verfasserin aut Vallania, P. verfasserin aut van Eldik, C. verfasserin aut van Scherpenberg, J. verfasserin aut Vandenbroucke, J. verfasserin aut Acosta, M. Vazquez verfasserin aut Vecchi, M. verfasserin aut Vercellone, S. verfasserin aut Verna, G. verfasserin aut Viana, A. verfasserin aut Vignatti, J. verfasserin aut Vitale, V. verfasserin aut Vodeb, V. verfasserin aut Vorobiov, S. verfasserin aut Vuillaume, T. verfasserin aut Wagner, S.J. verfasserin aut Walter, R. verfasserin aut White, M. verfasserin aut Wierzcholska, A. verfasserin aut Will, M. verfasserin aut Williams, D. verfasserin aut Yang, L. verfasserin aut Yoshida, T. verfasserin aut Yoshikoshi, T. verfasserin aut Zaharijas, G. verfasserin aut Zampieri, L. verfasserin aut Zavrtanik, D. verfasserin aut Zavrtanik, M. verfasserin aut Zhdanov, V.I. verfasserin aut Z̆ivec, M. verfasserin aut Enthalten in Astroparticle physics Amsterdam [u.a.] : Elsevier Science, 1992 150 Online-Ressource (DE-627)306654059 (DE-600)1499883-X (DE-576)116226218 0927-6505 nnns volume:150 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHA SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.22 Astrophysik AR 150
language	English
source	Enthalten in Astroparticle physics 150 volume:150
sourceStr	Enthalten in Astroparticle physics 150 volume:150
format_phy_str_mv	Article
bklname	Astrophysik
institution	findex.gbv.de
topic_facet	Gamma rays: general Cosmic rays Galactic PeVatrons (Stars:) supernovae: general Methods: data analysis Methods: statistical
dewey-raw	540
isfreeaccess_bool	false
container_title	Astroparticle physics
authorswithroles_txt_mv	Acero, F. @@aut@@ Acharyya, A. @@aut@@ Adam, R. @@aut@@ Aguasca-Cabot, A. @@aut@@ Agudo, I. @@aut@@ Aguirre-Santaella, A. @@aut@@ Alfaro, J. @@aut@@ Aloisio, R. @@aut@@ Crespo, N. Álvarez @@aut@@ Batista, R. Alves @@aut@@ Amati, L. @@aut@@ Amato, E. @@aut@@ Ambrosi, G. @@aut@@ Angüner, E.O. @@aut@@ Aramo, C. @@aut@@ Arcaro, C. @@aut@@ Armstrong, T. @@aut@@ Asano, K. @@aut@@ Ascasibar, Y. @@aut@@ Aschersleben, J. @@aut@@ Backes, M. @@aut@@ Baktash, A. @@aut@@ Balazs, C. @@aut@@ Balbo, M. @@aut@@ Ballet, J. @@aut@@ Larriva, A. Baquero @@aut@@ Martins, V. Barbosa @@aut@@ de Almeida, U. Barres @@aut@@ Barrio, J.A. @@aut@@ Bastieri, D. @@aut@@ Baxter, J.R. @@aut@@ Tjus, J. Becker @@aut@@ Benbow, W. @@aut@@ Bernardos-Martín, M.I. @@aut@@ Bernete, J. @@aut@@ Berti, A. @@aut@@ Bertucci, B. @@aut@@ Beshley, V. @@aut@@ Bhattacharjee, P. @@aut@@ Bhattacharyya, S. @@aut@@ Biland, A. @@aut@@ Bissaldi, E. @@aut@@ Biteau, J. @@aut@@ Blanch, O. @@aut@@ Bordas, P. @@aut@@ Bottacini, E. @@aut@@ Bregeon, J. @@aut@@ Brose, R. @@aut@@ Bucciantini, N. @@aut@@ Bulgarelli, A. @@aut@@ Capasso, M. @@aut@@ Dolcetta, R.A. Capuzzo @@aut@@ Caraveo, P. @@aut@@ Cardillo, M. @@aut@@ Carosi, R. @@aut@@ Casanova, S. @@aut@@ Cascone, E. @@aut@@ Cassol, F. @@aut@@ Catalani, F. @@aut@@ Cerruti, M. @@aut@@ Chadwick, P. @@aut@@ Chaty, S. @@aut@@ Chen, A. @@aut@@ Chernyakova, M. @@aut@@ Chiavassa, A. @@aut@@ Chudoba, J. @@aut@@ Coimbra-Araujo, C. @@aut@@ Conforti, V. @@aut@@ Contreras, J.L. @@aut@@ Costa, A. @@aut@@ Costantini, H. @@aut@@ Cristofari, P. @@aut@@ Crocker, R. @@aut@@ D’Amico, G. @@aut@@ D’Ammando, F. @@aut@@ De Angelis, A. @@aut@@ De Caprio, V. @@aut@@ de Gouveia Dal Pino, E.M. @@aut@@ de Ona Wilhelmi, E. @@aut@@ de Souza, V. @@aut@@ Delgado, C. @@aut@@ della Volpe, D. @@aut@@ Depaoli, D. @@aut@@ Di Girolamo, T. @@aut@@ Di Pierro, F. @@aut@@ Di Tria, R. @@aut@@ Di Venere, L. @@aut@@ Diebold, S. @@aut@@ Djuvsland, J.I. @@aut@@ Donini, A. @@aut@@ Doro, M. @@aut@@ Dos Anjos, R.d.C. @@aut@@ Dwarkadas, V.V. @@aut@@ Einecke, S. @@aut@@ Elsässer, D. @@aut@@ Emery, G. @@aut@@ Evoli, C. @@aut@@ Falceta-Goncalves, D. @@aut@@ Fedorova, E. @@aut@@ Fegan, S. @@aut@@ Ferrand, G. @@aut@@ Fiandrini, E. @@aut@@ Filipovic, M. @@aut@@ Fioretti, V. @@aut@@ Fiori, M. @@aut@@ Foffano, L. @@aut@@ Fontaine, G. @@aut@@ Fukami, S. @@aut@@ Galanti, G. @@aut@@ Galaz, G. @@aut@@ Gammaldi, V. @@aut@@ Gasbarra, C. @@aut@@ Ghalumyan, A. @@aut@@ Ghirlanda, G. @@aut@@ Giarrusso, M. @@aut@@ Giavitto, G. @@aut@@ Giglietto, N. @@aut@@ Giordano, F. @@aut@@ Giroletti, M. @@aut@@ Giuliani, A. @@aut@@ Giunti, L. @@aut@@ Godinovic, N. @@aut@@ Coelho, J. Goulart @@aut@@ Gréaux, L. @@aut@@ Green, D. @@aut@@ Grondin, M.-H. @@aut@@ Gueta, O. @@aut@@ Gunji, S. @@aut@@ Hassan, T. @@aut@@ Heller, M. @@aut@@ Hernández-Cadena, S. @@aut@@ Hinton, J. @@aut@@ Hnatyk, B. @@aut@@ Hnatyk, R. @@aut@@ Hoffmann, D. @@aut@@ Hofmann, W. @@aut@@ Holder, J. @@aut@@ Horan, D. @@aut@@ Horvath, P. @@aut@@ Hrabovsky, M. @@aut@@ Hrupec, D. @@aut@@ Inada, T. @@aut@@ Incardona, F. @@aut@@ Inoue, S. @@aut@@ Ishio, K. @@aut@@ Jamrozy, M. @@aut@@ Janecek, P. @@aut@@ Martínez, I. Jiménez @@aut@@ Jin, W. @@aut@@ Jung-Richardt, I. @@aut@@ Jurysek, J. @@aut@@ Kaaret, P. @@aut@@ Karas, V. @@aut@@ Katz, U. @@aut@@ Kerszberg, D. @@aut@@ Khélifi, B. @@aut@@ Kieda, D.B. @@aut@@ Kissmann, R. @@aut@@ Kleiner, T. @@aut@@ Kluge, G. @@aut@@ Kluzniak, W. @@aut@@ Knödlseder, J. @@aut@@ Kobayashi, Y. @@aut@@ Kohri, K. @@aut@@ Komin, N. @@aut@@ Kornecki, P. @@aut@@ Kubo, H. @@aut@@ La Palombara, N. @@aut@@ Láinez, M. @@aut@@ Lamastra, A. @@aut@@ Lapington, J. @@aut@@ Lemoine-Goumard, M. @@aut@@ Lenain, J.-P. @@aut@@ Leone, F. @@aut@@ Leto, G. @@aut@@ Leuschner, F. @@aut@@ Lindfors, E. @@aut@@ Liodakis, I. @@aut@@ Lohse, T. @@aut@@ Lombardi, S. @@aut@@ Longo, F. @@aut@@ López-Coto, R. @@aut@@ López-Moya, M. @@aut@@ López-Oramas, A. @@aut@@ Loporchio, S. @@aut@@ Luque-Escamilla, P.L. @@aut@@ Macias, O. @@aut@@ Mackey, J. @@aut@@ Majumdar, P. @@aut@@ Mandat, D. @@aut@@ Manganaro, M. @@aut@@ Manicò, G. @@aut@@ Marconi, M. @@aut@@ Martí, J. @@aut@@ Martínez, G. @@aut@@ Martinez, M. @@aut@@ Martinez, O. @@aut@@ Mello, A.J.T.S. @@aut@@ Menchiari, S. @@aut@@ Meyer, D.M.-A. @@aut@@ Micanovic, S. @@aut@@ Miceli, D. @@aut@@ Miceli, M. @@aut@@ Michalowski, J. @@aut@@ Miener, T. @@aut@@ Miranda, J.M. @@aut@@ Mitchell, A. @@aut@@ Mode, B. @@aut@@ Moderski, R. @@aut@@ Mohrmann, L. @@aut@@ Molina, E. @@aut@@ Montaruli, T. @@aut@@ Morcuende, D. @@aut@@ Morlino, G. @@aut@@ Morselli, A. @@aut@@ Mosè, M. @@aut@@ Moulin, E. @@aut@@ Mukherjee, R. @@aut@@ Munari, K. @@aut@@ Murach, T. @@aut@@ Nagai, A. @@aut@@ Nagataki, S. @@aut@@ Nemmen, R. @@aut@@ Niemiec, J. @@aut@@ Nieto, D. @@aut@@ Rosillo, M. Nievas @@aut@@ Nikolajuk, M. @@aut@@ Nishijima, K. @@aut@@ Noda, K. @@aut@@ Novosyadlyj, B. @@aut@@ Nozaki, S. @@aut@@ Ohishi, M. @@aut@@ Ohm, S. @@aut@@ Ohtani, Y. @@aut@@ Okumura, A. @@aut@@ Olmi, B. @@aut@@ Ong, R.A. @@aut@@ Orienti, M. @@aut@@ Orito, R. @@aut@@ Orlandini, M. @@aut@@ Orlando, E. @@aut@@ Orlando, S. @@aut@@ Ostrowski, M. @@aut@@ Oya, I. @@aut@@ Pantaleo, F.R. @@aut@@ Paredes, J.M. @@aut@@ Patricelli, B. @@aut@@ Pecimotika, M. @@aut@@ Peresano, M. @@aut@@ Pérez-Romero, J. @@aut@@ Persic, M. @@aut@@ Petruk, O. @@aut@@ Piano, G. @@aut@@ Pietropaolo, E. @@aut@@ Pirola, G. @@aut@@ Pittori, C. @@aut@@ Pohl, M. @@aut@@ Ponti, G. @@aut@@ Prandini, E. @@aut@@ Principe, G. @@aut@@ Priyadarshi, C. @@aut@@ Pueschel, E. @@aut@@ Pühlhofer, G. @@aut@@ Pumo, M.L. @@aut@@ Quirrenbach, A. @@aut@@ Rando, R. @@aut@@ Razzaque, S. @@aut@@ Reichherzer, P. @@aut@@ Reimer, A. @@aut@@ Reimer, O. @@aut@@ Renaud, M. @@aut@@ Reposeur, T. @@aut@@ Ribó, M. @@aut@@ Richtler, T. @@aut@@ Rico, J. @@aut@@ Rieger, F. @@aut@@ Rigoselli, M. @@aut@@ Riitano, L. @@aut@@ Rizi, V. @@aut@@ Roache, E. @@aut@@ Romano, P. @@aut@@ Romeo, G. @@aut@@ Rosado, J. @@aut@@ Rowell, G. @@aut@@ Rudak, B. @@aut@@ Sadeh, I. @@aut@@ Safi-Harb, S. @@aut@@ Saha, L. @@aut@@ Sailer, S. @@aut@@ Sánchez-Conde, M. @@aut@@ Sarkar, S. @@aut@@ Satalecka, K. @@aut@@ Saturni, F.G. @@aut@@ Scherer, A. @@aut@@ Schovánek, P. @@aut@@ Schussler, F. @@aut@@ Schwanke, U. @@aut@@ Scuderi, S. @@aut@@ Seglar-Arroyo, M. @@aut@@ Sergijenko, O. @@aut@@ Servillat, M. @@aut@@ Shang, R.-Y. @@aut@@ Sharma, P. @@aut@@ Siejkowski, H. @@aut@@ Sliusar, V. @@aut@@ Słowikowska, A. @@aut@@ Sol, H. @@aut@@ Specovius, A. @@aut@@ Spencer, S.T. @@aut@@ Spengler, G. @@aut@@ Stamerra, A. @@aut@@ Stanič, S. @@aut@@ Starecki, T. @@aut@@ Starling, R. @@aut@@ Stolarczyk, T. @@aut@@ Pereira, L.A. Stuani @@aut@@ Suda, Y. @@aut@@ Suomijarvi, T. @@aut@@ Sushch, I. @@aut@@ Tajima, H. @@aut@@ Tam, P.-H.T. @@aut@@ Tanaka, S.J. @@aut@@ Tavecchio, F. @@aut@@ Testa, V. @@aut@@ Tian, W. @@aut@@ Tibaldo, L. @@aut@@ Torres, D.F. @@aut@@ Tothill, N. @@aut@@ Vallage, B. @@aut@@ Vallania, P. @@aut@@ van Eldik, C. @@aut@@ van Scherpenberg, J. @@aut@@ Vandenbroucke, J. @@aut@@ Acosta, M. Vazquez @@aut@@ Vecchi, M. @@aut@@ Vercellone, S. @@aut@@ Verna, G. @@aut@@ Viana, A. @@aut@@ Vignatti, J. @@aut@@ Vitale, V. @@aut@@ Vodeb, V. @@aut@@ Vorobiov, S. @@aut@@ Vuillaume, T. @@aut@@ Wagner, S.J. @@aut@@ Walter, R. @@aut@@ White, M. @@aut@@ Wierzcholska, A. @@aut@@ Will, M. @@aut@@ Williams, D. @@aut@@ Yang, L. @@aut@@ Yoshida, T. @@aut@@ Yoshikoshi, T. @@aut@@ Zaharijas, G. @@aut@@ Zampieri, L. @@aut@@ Zavrtanik, D. @@aut@@ Zavrtanik, M. @@aut@@ Zhdanov, V.I. @@aut@@ Z̆ivec, M. @@aut@@
publishDateDaySort_date	2023-01-01T00:00:00Z
hierarchy_top_id	306654059
dewey-sort	3540
id	ELV009642641
language_de	englisch
fullrecord	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV009642641</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230524164524.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">230511s2023 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.astropartphys.2023.102850</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV009642641</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0927-6505(23)00036-1</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">540</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.22</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Acero, F.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2023</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Gamma rays: general</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Cosmic rays</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Galactic PeVatrons</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">(Stars:) supernovae: general</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Methods: data analysis</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Methods: statistical</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Acharyya, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Adam, R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aguasca-Cabot, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Agudo, I.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aguirre-Santaella, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Alfaro, J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aloisio, R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Crespo, N. Álvarez</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Batista, R. Alves</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Amati, L.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Amato, E.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ambrosi, G.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Angüner, E.O.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aramo, C.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Arcaro, C.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Armstrong, T.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Asano, K.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ascasibar, Y.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Aschersleben, J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Backes, M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Baktash, A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Balazs, C.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Balbo, M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ballet, J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Larriva, A. 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Barres</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Barrio, J.A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bastieri, D.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Baxter, J.R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Tjus, J. 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ind1="1" ind2=" "><subfield code="a">Rosillo, M. 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code="a">Oya, I.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pantaleo, F.R.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Paredes, J.M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Patricelli, B.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pecimotika, M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Peresano, M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" 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author	Acero, F.
spellingShingle	Acero, F. ddc 540 bkl 39.22 misc Gamma rays: general misc Cosmic rays misc Galactic PeVatrons misc (Stars:) supernovae: general misc Methods: data analysis misc Methods: statistical Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
authorStr	Acero, F.
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topic_title	540 DE-600 39.22 bkl Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants Gamma rays: general Cosmic rays Galactic PeVatrons (Stars:) supernovae: general Methods: data analysis Methods: statistical
topic	ddc 540 bkl 39.22 misc Gamma rays: general misc Cosmic rays misc Galactic PeVatrons misc (Stars:) supernovae: general misc Methods: data analysis misc Methods: statistical
topic_unstemmed	ddc 540 bkl 39.22 misc Gamma rays: general misc Cosmic rays misc Galactic PeVatrons misc (Stars:) supernovae: general misc Methods: data analysis misc Methods: statistical
topic_browse	ddc 540 bkl 39.22 misc Gamma rays: general misc Cosmic rays misc Galactic PeVatrons misc (Stars:) supernovae: general misc Methods: data analysis misc Methods: statistical
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title	Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
ctrlnum	(DE-627)ELV009642641 (ELSEVIER)S0927-6505(23)00036-1
title_full	Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
author_sort	Acero, F.
journal	Astroparticle physics
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author_browse	Acero, F. Acharyya, A. Adam, R. Aguasca-Cabot, A. Agudo, I. Aguirre-Santaella, A. Alfaro, J. Aloisio, R. Crespo, N. Álvarez Batista, R. Alves Amati, L. Amato, E. Ambrosi, G. Angüner, E.O. Aramo, C. Arcaro, C. Armstrong, T. Asano, K. Ascasibar, Y. Aschersleben, J. Backes, M. Baktash, A. Balazs, C. Balbo, M. Ballet, J. Larriva, A. Baquero Martins, V. Barbosa de Almeida, U. Barres Barrio, J.A. Bastieri, D. Baxter, J.R. Tjus, J. Becker Benbow, W. Bernardos-Martín, M.I. Bernete, J. Berti, A. Bertucci, B. Beshley, V. Bhattacharjee, P. Bhattacharyya, S. Biland, A. Bissaldi, E. Biteau, J. Blanch, O. Bordas, P. Bottacini, E. Bregeon, J. Brose, R. Bucciantini, N. Bulgarelli, A. Capasso, M. Dolcetta, R.A. Capuzzo Caraveo, P. Cardillo, M. Carosi, R. Casanova, S. Cascone, E. Cassol, F. Catalani, F. Cerruti, M. Chadwick, P. Chaty, S. Chen, A. Chernyakova, M. Chiavassa, A. Chudoba, J. Coimbra-Araujo, C. Conforti, V. Contreras, J.L. Costa, A. Costantini, H. Cristofari, P. Crocker, R. D’Amico, G. D’Ammando, F. De Angelis, A. De Caprio, V. de Gouveia Dal Pino, E.M. de Ona Wilhelmi, E. de Souza, V. Delgado, C. della Volpe, D. Depaoli, D. Di Girolamo, T. Di Pierro, F. Di Tria, R. Di Venere, L. Diebold, S. Djuvsland, J.I. Donini, A. Doro, M. Dos Anjos, R.d.C. Dwarkadas, V.V. Einecke, S. Elsässer, D. Emery, G. Evoli, C. Falceta-Goncalves, D. Fedorova, E. Fegan, S. Ferrand, G. Fiandrini, E. Filipovic, M. Fioretti, V. Fiori, M. Foffano, L. Fontaine, G. Fukami, S. Galanti, G. Galaz, G. Gammaldi, V. Gasbarra, C. Ghalumyan, A. Ghirlanda, G. Giarrusso, M. Giavitto, G. Giglietto, N. Giordano, F. Giroletti, M. Giuliani, A. Giunti, L. Godinovic, N. Coelho, J. Goulart Gréaux, L. Green, D. Grondin, M.-H. Gueta, O. Gunji, S. Hassan, T. Heller, M. Hernández-Cadena, S. Hinton, J. Hnatyk, B. Hnatyk, R. Hoffmann, D. Hofmann, W. Holder, J. Horan, D. Horvath, P. Hrabovsky, M. Hrupec, D. Inada, T. Incardona, F. Inoue, S. Ishio, K. Jamrozy, M. Janecek, P. Martínez, I. Jiménez Jin, W. Jung-Richardt, I. Jurysek, J. Kaaret, P. Karas, V. Katz, U. Kerszberg, D. Khélifi, B. Kieda, D.B. Kissmann, R. Kleiner, T. Kluge, G. Kluzniak, W. Knödlseder, J. Kobayashi, Y. Kohri, K. Komin, N. Kornecki, P. Kubo, H. La Palombara, N. Láinez, M. Lamastra, A. Lapington, J. Lemoine-Goumard, M. Lenain, J.-P. Leone, F. Leto, G. Leuschner, F. Lindfors, E. Liodakis, I. Lohse, T. Lombardi, S. Longo, F. López-Coto, R. López-Moya, M. López-Oramas, A. Loporchio, S. Luque-Escamilla, P.L. Macias, O. Mackey, J. Majumdar, P. Mandat, D. Manganaro, M. Manicò, G. Marconi, M. Martí, J. Martínez, G. Martinez, M. Martinez, O. Mello, A.J.T.S. Menchiari, S. Meyer, D.M.-A. Micanovic, S. Miceli, D. Miceli, M. Michalowski, J. Miener, T. Miranda, J.M. Mitchell, A. Mode, B. Moderski, R. Mohrmann, L. Molina, E. Montaruli, T. Morcuende, D. Morlino, G. Morselli, A. Mosè, M. Moulin, E. Mukherjee, R. Munari, K. Murach, T. Nagai, A. Nagataki, S. Nemmen, R. Niemiec, J. Nieto, D. Rosillo, M. Nievas Nikolajuk, M. Nishijima, K. Noda, K. Novosyadlyj, B. Nozaki, S. Ohishi, M. Ohm, S. Ohtani, Y. Okumura, A. Olmi, B. Ong, R.A. Orienti, M. Orito, R. Orlandini, M. Orlando, E. Orlando, S. Ostrowski, M. Oya, I. Pantaleo, F.R. Paredes, J.M. Patricelli, B. Pecimotika, M. Peresano, M. Pérez-Romero, J. Persic, M. Petruk, O. Piano, G. Pietropaolo, E. Pirola, G. Pittori, C. Pohl, M. Ponti, G. Prandini, E. Principe, G. Priyadarshi, C. Pueschel, E. Pühlhofer, G. Pumo, M.L. Quirrenbach, A. Rando, R. Razzaque, S. Reichherzer, P. Reimer, A. Reimer, O. Renaud, M. Reposeur, T. Ribó, M. Richtler, T. Rico, J. Rieger, F. Rigoselli, M. Riitano, L. Rizi, V. Roache, E. Romano, P. Romeo, G. Rosado, J. Rowell, G. Rudak, B. Sadeh, I. Safi-Harb, S. Saha, L. Sailer, S. Sánchez-Conde, M. Sarkar, S. Satalecka, K. Saturni, F.G. Scherer, A. Schovánek, P. Schussler, F. Schwanke, U. Scuderi, S. Seglar-Arroyo, M. Sergijenko, O. Servillat, M. Shang, R.-Y. Sharma, P. Siejkowski, H. Sliusar, V. Słowikowska, A. Sol, H. Specovius, A. Spencer, S.T. Spengler, G. Stamerra, A. Stanič, S. Starecki, T. Starling, R. Stolarczyk, T. Pereira, L.A. Stuani Suda, Y. Suomijarvi, T. Sushch, I. Tajima, H. Tam, P.-H.T. Tanaka, S.J. Tavecchio, F. Testa, V. Tian, W. Tibaldo, L. Torres, D.F. Tothill, N. Vallage, B. Vallania, P. van Eldik, C. van Scherpenberg, J. Vandenbroucke, J. Acosta, M. Vazquez Vecchi, M. Vercellone, S. Verna, G. Viana, A. Vignatti, J. Vitale, V. Vodeb, V. Vorobiov, S. Vuillaume, T. Wagner, S.J. Walter, R. White, M. Wierzcholska, A. Will, M. Williams, D. Yang, L. Yoshida, T. Yoshikoshi, T. Zaharijas, G. Zampieri, L. Zavrtanik, D. Zavrtanik, M. Zhdanov, V.I. Z̆ivec, M.
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class	540 DE-600 39.22 bkl
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author-letter	Acero, F.
doi_str_mv	10.1016/j.astropartphys.2023.102850
dewey-full	540
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title_sort	sensitivity of the cherenkov telescope array to spectral signatures of hadronic pevatrons with application to galactic supernova remnants
title_auth	Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
abstract	The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source.
abstractGer	The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source.
abstract_unstemmed	The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. CTA is also shown to have excellent potential to confirm these sources as PeVatrons in deep observations with O ( 100 ) hours of exposure per source.
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title_short	Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
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author2	Acharyya, A. Adam, R. Aguasca-Cabot, A. Agudo, I. Aguirre-Santaella, A. Alfaro, J. Aloisio, R. Crespo, N. Álvarez Batista, R. Alves Amati, L. Amato, E. Ambrosi, G. Angüner, E.O. Aramo, C. Arcaro, C. Armstrong, T. Asano, K. Ascasibar, Y. Aschersleben, J. Backes, M. Baktash, A. Balazs, C. Balbo, M. Ballet, J. Larriva, A. Baquero Martins, V. Barbosa de Almeida, U. Barres Barrio, J.A. Bastieri, D. Baxter, J.R. Tjus, J. Becker Benbow, W. Bernardos-Martín, M.I. Bernete, J. Berti, A. Bertucci, B. Beshley, V. Bhattacharjee, P. Bhattacharyya, S. Biland, A. Bissaldi, E. Biteau, J. Blanch, O. Bordas, P. Bottacini, E. Bregeon, J. Brose, R. Bucciantini, N. Bulgarelli, A. Capasso, M. Dolcetta, R.A. Capuzzo Caraveo, P. Cardillo, M. Carosi, R. Casanova, S. Cascone, E. Cassol, F. Catalani, F. Cerruti, M. Chadwick, P. Chaty, S. Chen, A. Chernyakova, M. Chiavassa, A. Chudoba, J. Coimbra-Araujo, C. Conforti, V. Contreras, J.L. Costa, A. Costantini, H. Cristofari, P. Crocker, R. D’Amico, G. D’Ammando, F. De Angelis, A. De Caprio, V. de Gouveia Dal Pino, E.M. de Ona Wilhelmi, E. de Souza, V. Delgado, C. della Volpe, D. Depaoli, D. Di Girolamo, T. Di Pierro, F. Di Tria, R. Di Venere, L. Diebold, S. Djuvsland, J.I. Donini, A. Doro, M. Dos Anjos, R.d.C. Dwarkadas, V.V. Einecke, S. Elsässer, D. Emery, G. Evoli, C. Falceta-Goncalves, D. Fedorova, E. Fegan, S. Ferrand, G. Fiandrini, E. Filipovic, M. Fioretti, V. Fiori, M. Foffano, L. Fontaine, G. Fukami, S. Galanti, G. Galaz, G. Gammaldi, V. Gasbarra, C. Ghalumyan, A. Ghirlanda, G. Giarrusso, M. Giavitto, G. Giglietto, N. Giordano, F. Giroletti, M. Giuliani, A. Giunti, L. Godinovic, N. Coelho, J. Goulart Gréaux, L. Green, D. Grondin, M.-H. Gueta, O. Gunji, S. Hassan, T. Heller, M. Hernández-Cadena, S. Hinton, J. Hnatyk, B. Hnatyk, R. Hoffmann, D. Hofmann, W. Holder, J. Horan, D. Horvath, P. Hrabovsky, M. Hrupec, D. Inada, T. Incardona, F. Inoue, S. Ishio, K. Jamrozy, M. Janecek, P. Martínez, I. Jiménez Jin, W. Jung-Richardt, I. Jurysek, J. Kaaret, P. Karas, V. Katz, U. Kerszberg, D. Khélifi, B. Kieda, D.B. Kissmann, R. Kleiner, T. Kluge, G. Kluzniak, W. Knödlseder, J. Kobayashi, Y. Kohri, K. Komin, N. Kornecki, P. Kubo, H. La Palombara, N. Láinez, M. Lamastra, A. Lapington, J. Lemoine-Goumard, M. Lenain, J.-P. Leone, F. Leto, G. Leuschner, F. Lindfors, E. Liodakis, I. Lohse, T. Lombardi, S. Longo, F. López-Coto, R. López-Moya, M. López-Oramas, A. Loporchio, S. Luque-Escamilla, P.L. Macias, O. Mackey, J. Majumdar, P. Mandat, D. Manganaro, M. Manicò, G. Marconi, M. Martí, J. Martínez, G. Martinez, M. Martinez, O. Mello, A.J.T.S. Menchiari, S. Meyer, D.M.-A. Micanovic, S. Miceli, D. Miceli, M. Michalowski, J. Miener, T. Miranda, J.M. Mitchell, A. Mode, B. Moderski, R. Mohrmann, L. Molina, E. Montaruli, T. Morcuende, D. Morlino, G. Morselli, A. Mosè, M. Moulin, E. Mukherjee, R. Munari, K. Murach, T. Nagai, A. Nagataki, S. Nemmen, R. Niemiec, J. Nieto, D. Rosillo, M. Nievas Nikolajuk, M. Nishijima, K. Noda, K. Novosyadlyj, B. Nozaki, S. Ohishi, M. Ohm, S. Ohtani, Y. Okumura, A. Olmi, B. Ong, R.A. Orienti, M. Orito, R. Orlandini, M. Orlando, E. Orlando, S. Ostrowski, M. Oya, I. Pantaleo, F.R. Paredes, J.M. Patricelli, B. Pecimotika, M. Peresano, M. Pérez-Romero, J. Persic, M. Petruk, O. Piano, G. Pietropaolo, E. Pirola, G. Pittori, C. Pohl, M. Ponti, G. Prandini, E. Principe, G. Priyadarshi, C. Pueschel, E. Pühlhofer, G. Pumo, M.L. Quirrenbach, A. Rando, R. Razzaque, S. Reichherzer, P. Reimer, A. Reimer, O. Renaud, M. Reposeur, T. Ribó, M. Richtler, T. Rico, J. Rieger, F. Rigoselli, M. Riitano, L. Rizi, V. Roache, E. Romano, P. Romeo, G. Rosado, J. Rowell, G. Rudak, B. Sadeh, I. Safi-Harb, S. Saha, L. Sailer, S. Sánchez-Conde, M. Sarkar, S. Satalecka, K. Saturni, F.G. Scherer, A. Schovánek, P. Schussler, F. Schwanke, U. Scuderi, S. Seglar-Arroyo, M. Sergijenko, O. Servillat, M. Shang, R.-Y. Sharma, P. Siejkowski, H. Sliusar, V. Słowikowska, A. Sol, H. Specovius, A. Spencer, S.T. Spengler, G. Stamerra, A. Stanič, S. Starecki, T. Starling, R. Stolarczyk, T. Pereira, L.A. Stuani Suda, Y. Suomijarvi, T. Sushch, I. Tajima, H. Tam, P.-H.T. Tanaka, S.J. Tavecchio, F. Testa, V. Tian, W. Tibaldo, L. Torres, D.F. Tothill, N. Vallage, B. Vallania, P. van Eldik, C. van Scherpenberg, J. Vandenbroucke, J. Acosta, M. Vazquez Vecchi, M. Vercellone, S. Verna, G. Viana, A. Vignatti, J. Vitale, V. Vodeb, V. Vorobiov, S. Vuillaume, T. Wagner, S.J. Walter, R. White, M. Wierzcholska, A. Will, M. Williams, D. Yang, L. Yoshida, T. Yoshikoshi, T. Zaharijas, G. Zampieri, L. Zavrtanik, D. Zavrtanik, M. Zhdanov, V.I. Z̆ivec, M.
author2Str	Acharyya, A. Adam, R. Aguasca-Cabot, A. Agudo, I. Aguirre-Santaella, A. Alfaro, J. Aloisio, R. Crespo, N. Álvarez Batista, R. Alves Amati, L. Amato, E. Ambrosi, G. Angüner, E.O. Aramo, C. Arcaro, C. Armstrong, T. Asano, K. Ascasibar, Y. Aschersleben, J. Backes, M. Baktash, A. Balazs, C. Balbo, M. Ballet, J. Larriva, A. Baquero Martins, V. Barbosa de Almeida, U. Barres Barrio, J.A. Bastieri, D. Baxter, J.R. Tjus, J. Becker Benbow, W. Bernardos-Martín, M.I. Bernete, J. Berti, A. Bertucci, B. Beshley, V. Bhattacharjee, P. Bhattacharyya, S. Biland, A. Bissaldi, E. Biteau, J. Blanch, O. Bordas, P. Bottacini, E. Bregeon, J. Brose, R. Bucciantini, N. Bulgarelli, A. Capasso, M. Dolcetta, R.A. Capuzzo Caraveo, P. Cardillo, M. Carosi, R. Casanova, S. Cascone, E. Cassol, F. Catalani, F. Cerruti, M. Chadwick, P. Chaty, S. Chen, A. Chernyakova, M. Chiavassa, A. Chudoba, J. Coimbra-Araujo, C. Conforti, V. Contreras, J.L. Costa, A. Costantini, H. Cristofari, P. Crocker, R. D’Amico, G. D’Ammando, F. De Angelis, A. De Caprio, V. de Gouveia Dal Pino, E.M. de Ona Wilhelmi, E. de Souza, V. Delgado, C. della Volpe, D. Depaoli, D. Di Girolamo, T. Di Pierro, F. Di Tria, R. Di Venere, L. Diebold, S. Djuvsland, J.I. Donini, A. Doro, M. Dos Anjos, R.d.C. Dwarkadas, V.V. Einecke, S. Elsässer, D. Emery, G. Evoli, C. Falceta-Goncalves, D. Fedorova, E. Fegan, S. Ferrand, G. Fiandrini, E. Filipovic, M. Fioretti, V. Fiori, M. Foffano, L. Fontaine, G. Fukami, S. Galanti, G. Galaz, G. Gammaldi, V. Gasbarra, C. Ghalumyan, A. Ghirlanda, G. Giarrusso, M. Giavitto, G. Giglietto, N. Giordano, F. Giroletti, M. Giuliani, A. Giunti, L. Godinovic, N. Coelho, J. Goulart Gréaux, L. Green, D. Grondin, M.-H. Gueta, O. Gunji, S. Hassan, T. Heller, M. Hernández-Cadena, S. Hinton, J. Hnatyk, B. Hnatyk, R. Hoffmann, D. Hofmann, W. Holder, J. Horan, D. Horvath, P. Hrabovsky, M. Hrupec, D. Inada, T. Incardona, F. Inoue, S. Ishio, K. Jamrozy, M. Janecek, P. Martínez, I. Jiménez Jin, W. Jung-Richardt, I. Jurysek, J. Kaaret, P. Karas, V. Katz, U. Kerszberg, D. Khélifi, B. Kieda, D.B. Kissmann, R. Kleiner, T. Kluge, G. Kluzniak, W. Knödlseder, J. Kobayashi, Y. Kohri, K. Komin, N. Kornecki, P. Kubo, H. La Palombara, N. Láinez, M. Lamastra, A. Lapington, J. Lemoine-Goumard, M. Lenain, J.-P. Leone, F. Leto, G. Leuschner, F. Lindfors, E. Liodakis, I. Lohse, T. Lombardi, S. Longo, F. López-Coto, R. López-Moya, M. López-Oramas, A. Loporchio, S. Luque-Escamilla, P.L. Macias, O. Mackey, J. Majumdar, P. Mandat, D. Manganaro, M. Manicò, G. Marconi, M. Martí, J. Martínez, G. Martinez, M. Martinez, O. Mello, A.J.T.S. Menchiari, S. Meyer, D.M.-A. Micanovic, S. Miceli, D. Miceli, M. Michalowski, J. Miener, T. Miranda, J.M. Mitchell, A. Mode, B. Moderski, R. Mohrmann, L. Molina, E. Montaruli, T. Morcuende, D. Morlino, G. Morselli, A. Mosè, M. Moulin, E. Mukherjee, R. Munari, K. Murach, T. Nagai, A. Nagataki, S. Nemmen, R. Niemiec, J. Nieto, D. Rosillo, M. Nievas Nikolajuk, M. Nishijima, K. Noda, K. Novosyadlyj, B. Nozaki, S. Ohishi, M. Ohm, S. Ohtani, Y. Okumura, A. Olmi, B. Ong, R.A. Orienti, M. Orito, R. Orlandini, M. Orlando, E. Orlando, S. Ostrowski, M. Oya, I. Pantaleo, F.R. Paredes, J.M. Patricelli, B. Pecimotika, M. Peresano, M. Pérez-Romero, J. Persic, M. Petruk, O. Piano, G. Pietropaolo, E. Pirola, G. Pittori, C. Pohl, M. Ponti, G. Prandini, E. Principe, G. Priyadarshi, C. Pueschel, E. Pühlhofer, G. Pumo, M.L. Quirrenbach, A. Rando, R. Razzaque, S. Reichherzer, P. Reimer, A. Reimer, O. Renaud, M. Reposeur, T. Ribó, M. Richtler, T. Rico, J. Rieger, F. Rigoselli, M. Riitano, L. Rizi, V. Roache, E. Romano, P. Romeo, G. Rosado, J. Rowell, G. Rudak, B. Sadeh, I. Safi-Harb, S. Saha, L. Sailer, S. Sánchez-Conde, M. Sarkar, S. Satalecka, K. Saturni, F.G. Scherer, A. Schovánek, P. Schussler, F. Schwanke, U. Scuderi, S. Seglar-Arroyo, M. Sergijenko, O. Servillat, M. Shang, R.-Y. Sharma, P. Siejkowski, H. Sliusar, V. Słowikowska, A. Sol, H. Specovius, A. Spencer, S.T. Spengler, G. Stamerra, A. Stanič, S. Starecki, T. Starling, R. Stolarczyk, T. Pereira, L.A. Stuani Suda, Y. Suomijarvi, T. Sushch, I. Tajima, H. Tam, P.-H.T. Tanaka, S.J. Tavecchio, F. Testa, V. Tian, W. Tibaldo, L. Torres, D.F. Tothill, N. Vallage, B. Vallania, P. van Eldik, C. van Scherpenberg, J. Vandenbroucke, J. Acosta, M. Vazquez Vecchi, M. Vercellone, S. Verna, G. Viana, A. Vignatti, J. Vitale, V. Vodeb, V. Vorobiov, S. Vuillaume, T. Wagner, S.J. Walter, R. White, M. Wierzcholska, A. Will, M. Williams, D. Yang, L. Yoshida, T. Yoshikoshi, T. Zaharijas, G. Zampieri, L. Zavrtanik, D. Zavrtanik, M. Zhdanov, V.I. Z̆ivec, M.
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doi_str	10.1016/j.astropartphys.2023.102850
up_date	2024-07-06T23:51:42.016Z
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fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV009642641</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230524164524.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">230511s2023 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.astropartphys.2023.102850</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV009642641</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0927-6505(23)00036-1</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">540</subfield><subfield code="q">DE-600</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.22</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Acero, F.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2023</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several source classes, including Galactic Supernova Remnants (SNRs), have been proposed as PeVatron candidates. The potential to search for hadronic PeVatrons with the Cherenkov Telescope Array (CTA) is assessed. The focus is on the usage of very high energy γ -ray spectral signatures for the identification of PeVatrons. Assuming that SNRs can accelerate CRs up to knee energies, the number of Galactic SNRs which can be identified as PeVatrons with CTA is estimated within a model for the evolution of SNRs. Additionally, the potential of a follow-up observation strategy under moonlight conditions for PeVatron searches is investigated. Statistical methods for the identification of PeVatrons are introduced, and realistic Monte-Carlo simulations of the response of the CTA observatory to the emission spectra from hadronic PeVatrons are performed. Based on simulations of a simplified model for the evolution for SNRs, the detection of a γ -ray signal from in average 9 Galactic PeVatron SNRs is expected to result from the scan of the Galactic plane with CTA after 10 h of exposure. 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Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

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