Accès ouvert déclaré
2023
article
Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data
Hidetarô Abe, K. Abe, S. Abe, V. A. Acciari, Arnau Aguasca-Cabot, I. Agudo, Nuria Álvarez Crespo, T. Aniello, S. Ansoldi, L. A. Antonelli, C. Aramo, A. Arbet Engels, Cornelia Arcaro, Manuel Artero, K. Asano, P. Aubert, Dominik Baack, Ana Babić, Ali Baktash, Aya Bamba, Andrés Baquero, L. Baroncelli, U. Barres de Almeida, J. A. Barrio, I. Batkovi'c, J. Baxter, Jordi Gonzàlez, W. Bednarek, E. Bernardini, M.I Bernardos, A. Berti, J. Besenrieder, Pooja Bhattacharjee, Noah Biederbeck, C. Bigongiari, A. Biland, E. Bissaldi, O. Blanch, G. Bonnoli, P. Bordas, Ž. Bošnjak, A. Bulgarelli, Irene Burelli, L. Burmistrov, Mario Buscemi, G. Busetto, A. Campoy Ordaz, M Cardillo, Sami Caroff, A. Carosi, R. Carosi, Marie-Sophie Carrasco, M. Carretero-Castrillo, A.J. Castro-Tirado, D. Cauz, Davide Cerasole, G. Ceribella, Yating Chai, Katherine C. Cheng, A. Chiavassa, M. Chikawa, L. Chytka, A. Cifuentes, S. Cikota, E. Colombo, J. L. Contreras, A. Cornelia, J. Cortina, H. Costantini, S. Covino, Giacomo D’Amico, V. D’Elia, P. Da Vela, M. Dalchenko, F. Dazzi, Mathieu de Bony de Lavergne, B. De Lotto, Mario de Lucia, Raniere de Menezes, L. del Peral, A. Del Popolo, Guillaume Deleglise, M. Delfino, C. Delgado Mendez, J. Delgado Mengual, D. della Volpe, Michael Dellaiera, Davide Depaoli, Ambra Di Piano, F. Di Pierro, Antonio Di Pilato, R. Di Tria, L. Di Venere, Rune Michael Dominik, D. Dominis Prester, Alice Donini, D. Dorner, M. Doro, Carlos Díaz, Laura Eisenberger, Dominik Elsässer, Gabriel Emery, Juan Escudero, V. Fallah Ramazani, Luis Fariña, Alicia Fattorini, G. Ferrara, F. Ferrarotto, A. Fiaßon, L. Foffano, L. Font, Lluís Freixas Coromina, Stefan Fröse, Satoshi Fukami, Y. Fukazawa, E. García, M. Garczarczyk, C. Gasbarra, D Gasparrini, Sargis Gasparyan, M. Gaug, David Geyer, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, Paweł Gliwny, N. Godinović, R. Grau, D. Green, Jarred Gershon Green, S. Gunji, Patrick Günther, Jonas Hackfeld, D. Hadasch, A. Hahn, K. Hashiyama, T. Hassan, K. Hayashi, Lea Heckmann, Matthieu Heller, J. Herrera Llorente, Kouichi Hirotani, D. Hoffmann, D. Horns, J. Houles, M Hrabovsky, Dario Hrupec, D. Hui, Moritz Hütten, M. Iarlori, Ryo Imazawa, Tomohiro Inada, Yusuke Inome, Kunihito Ioka, M. Iori, Roman Iotov, Kazuma Ishio, Mikaël Jacquemont, Irene Jiménez Martínez, Elli Jobst, Jenni Jormanainen, Jakub Jurýšek, M. Kagaya, V. Karas, H. Katagiri, J. Kataoka, D. Kerszberg, Gert Werner Kluge, Yukiho Kobayashi, Kazunori Kohri, A. K. H. Kong, Pouya M. Kouch, H. Kubo, J. Kushida, Miguel J. A. Láinez, G. Lamanna, A. Lamastra, T. Le Flour, F. Leone, E. Lindfors, Lena Linhoff, M. Linhoff, S. Lombardi, F. Longo, S. Loporchio, A. Lorini, J. J. Lozano Bahilo, Pedro L. Luque‐Escamilla, E. Lyard, M. Láinez Lezáun, R. López-Coto, A. López-Oramas, B. Machado de Oliveira Fraga, P. Majumdar, M. Makariev, Dušan Mandát, G. Maneva, M. Manganaro, S. Mangano, N. Mang, Giulio Manicò, K. Mannheim, M. Mariotti, Patricia Márquez, G. Marsella, Oibar Martínez, G. Martı́nez, M. Martínez, Alvaro Mas-Aguilar, G. Maurin, D. Mazin, Stefano Menchiari, S. Mender, E. Mestre Guillen, S. Mičanović, Davide Miceli, Tjark Miener, J. M. Miranda, R. Mirzoyan, Tsunefumi Mizuno, Miguel Molero Gonzalez, E. Molina, T. Montaruli, I. Monteiro, A. Moralejo, Daniel Morcuende, A. Morselli, V Moya, H. Muraishi, Kohta Murase, S. Nagataki, Takeshi Nakamori, C. Nanci, A. Neronov, V. Neustroev, Lukas Nickel, M. Nievas Rosillo, Cosimo Nigro, L. Nikolić, K. Nilsson, K. Nishijima, T. Njoh Ekoume, K. Noda, Dalibor Nosek, S. Nozaki, M. Ohishi, Y. Ohtani, Tomohiko Oka, A. Okumura, R. Orito, Jorge Otero-Santos, S. Paiano, M. Palatiello, D. Paneque, R. Paoletti, L. Pavletić, M. Pech, Mario Pecimotika, M. Peresano, M Persic, Felix Pfeiffle, E. Pietropaolo, Marine Pihet, G. Pirola, C. Plard, F. Podobnik, V. Poireau, Estelle Pons, E. Prandini, Julie Prast, G. Principe, C Priyadarshi, M. Prouza, R Rando, W. Rhode, M. Ribó, J. Rico, Chiara Righi, V. Rizi, N. Sahakyan, Takayuki Saito, S. Sakurai, K. Satalecka, M. Sato, Y. Sato, V. Savchenko, Bernd Schleicher, K. Schmidt, Felix Schmuckermaier, F. Schüßler, T. Schweizer, A. Sciaccaluga, Thomas Siegert, R Silvia, J. Sitarek, Vitalii Sliusar, D. Sobczyńska, Alessia Spolon, A. Stamerra, Jelena Strišković, D. Strom, M. Strzys, Y. Suda, Sofia Suutarinen, T. Šarić, H. Tajima, H. Takahashi, M Takahashi, J. Takata, Ryuji Takeishi, F. Tavecchio, P. Temnikov, Y. Terada, K. Terauchi, T. Terzić, M. Teshima, M. Tluczykont, Fuyuki Tokanai, Luca Tosti, P. Trávnı́ček, Stefano Truzzi, Antonio Tutone, Santiago Ubach, Martin Vacula, P Vallania, Juliane van Scherpenberg, M. Vázquez Acosta, Sofia Ventura, V. Verguilov, Ilaria Viale, Alessandro Vigliano, Elisa Visentin, V. Vitale, Georgios Gerasimos Voutsinas, Ievgen Vovk, R. Walter, Ze-Lin Wei, Martin Will, Takayuki Yamamoto, Ryo Yamazaki, T. Yoshida, T. Yoshikoshi, Natalia Żywucka
13Citations signalées, ce qui n’est pas une note de qualité
26Institutions déclarées
11Pays d’affiliation déclarés
Rattachement africain : it, fr, hr, jp, fi, cz, sk, no, es, ru, au.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
Aims. Large-Sized Telescope 1 (LST-1), the prototype for the Large-Sized Telescope at the upcoming Cherenkov Telescope Array Observatory, is concluding its commissioning phase at the Observatorio del Roque de los Muchachos on the island of La Palma. The proximity of LST-1 to the two MAGIC (Major Atmospheric Gamma Imaging Cherenkov) telescopes makes it possible to carry out observations of the same gamma-ray events with both systems. Methods. We describe the joint LST-1+MAGIC analysis pipeline and used simultaneous Crab Nebula observations and Monte Carlo simulations to assess the performance of the three-telescope system. The addition of the LST-1 telescope allows for the recovery of events in which one of the MAGIC images is too dim to survive analysis quality cuts. Results. Thanks to the resulting increase in the collection area and stronger background rejection, we found a significant improvement in sensitivity, allowing for the detection of 30% weaker fluxes in the energy range between 200 GeV and 3 TeV. The spectrum of the Crab Nebula, reconstructed in the energy range between ~60 GeV and ~10 TeV, is in agreement with previous measurements.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data
- Date Crossref
- 01/12/2023
- Éditeur
- EDP Sciences
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.
Les institutions déclarées
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Astrophysics and Cosmic PhenomenaRadioactivity and Radon MeasurementsRadiation Detection and Scintillator Technologies