Detection of RS Oph with LST-1 and modelling of its HE/VHE gamma-ray emission

Context. The recurrent nova RS Ophiuchi (RS Oph) underwent a thermonuclear eruption in August 2021. In this event, RS Oph was detected by the High Energy Stereoscopic System (H.E.S.S.), the Major Atmospheric Gamma Imaging Cherenkov (MAGIC), and the first Large-Sized Telescope (LST-1) of the future Cherenkov Telescope Array Observatory (CTAO) at very-high gamma-ray energies above 100 GeV. This means that novae are a new class of very-high-energy (VHE) gamma-ray emitters. Aims. We report the analysis of the RS Oph observations with LST-1. We constrain the particle population that causes the observed emission in hadronic and leptonic scenarios. Additionally, we study the prospects of detecting further novae using LST-1 and the upcoming LST array of CTAO-North. Methods. We conducted target-of-opportunity observations with LST-1 from the first day of this nova event. The data were analysed in the framework of cta-lstchain and Gammapy , the official CTAO-LST reconstruction and analysis packages. One-zone hadronic and leptonic models were considered to model the gamma-ray emission of RS Oph using the spectral information from Fermi -LAT and LST-1, together with public data from the MAGIC and H.E.S.S. telescopes. Results. RS Oph was detected at 6.6 σ with LST-1 in the first 6.35 hours of observations following the eruption. The hadronic scenario is preferred over the leptonic scenario considering a proton energy spectrum with a power-law model with an exponential cutoff whose position increases from (0.26 ± 0.08) TeV on day 1 up to (1.6 ± 0.6) TeV on day 4 after the eruption. The deep sensitivity and low energy threshold of the LST-1/LST array will allow us to detect faint novae and increase their discovery rate.

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Journal
Astronomy and Astrophysics
Published
2025-02-18
DOI
https://doi.org/10.1051/0004-6361/202452447
Citations
8
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
14.96

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Detection of RS Oph with LST-1 and modelling of its HE/VHE gamma-ray emission

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article

Detection of RS Oph with LST-1 and modelling of its HE/VHE gamma-ray emission

A. Hahn, P. Romano, M. Linhoff, Patrick Günther, M. Martínez, Alan Sunny, M. Seglar-Arroyo, P. Majumdar, D. Hoffmann, I. Vovk, M. Pech, A. K. H. Kong, J. Sitarek, Matteo Balbo, Pedro L. Luque‐Escamilla, O. Blanch, K. Hirotani, O. Kalashev, R. Walter, Natalia Żywucka, F. Schüßler, Irene Burelli, M. Heller, V. Vitale, Georgios Gerasimos Voutsinas, P. Bordas, Marine Pihet, E. Molina, H. Muraishi, Francesco Gabriele Saturni, Michael Dellaiera, Alvaro Mas-Aguilar, K. Mannheim, Juliane van Scherpenberg, Dalibor Nosek, Mathieu de Bony de Lavergne, S. Abe, D. Horns, P. Temnikov, Y. Fukazawa, R. Yamazaki, Gonzalo Rodriguez Fernandez, T. Šarić, Hidetoshi Sano, Kazunori Kohri, M. Mariotti, Ivana Batković, C. Delgado Mendez, Jarred Gershon Green, A. Iuliano, Thomas Vuillaume, Daniel Morcuende, M. Strzys, R. Rando, Y. Terada, R. Paoletti, Gabriel Emery, Stefano Marchesi, V. Sliusar, Laura Eisenberger, S. Sakurai, Sreedevi K. Menon, Fuyuki Tokanai, Aya Bamba, Thomas Siegert, T. Miener, J. Baxter, U. Barres de Almeida, V. Savchenko, Y. Kobayashi, G. Lamanna, C. Bigongiari, E. Bernardini, F. Dazzi, C. Gasbarra, A. López-Oramas, A. Neronov, F. Podobnik, Cyril Martin Alispach, R. Grau, J. A. Barrio, S. Rainò, Stefan Fröse, E. Ruiz-Velasco, A. Moralejo, Kunihito Ioka, Jan Lukas Schubert, Giulio Manicò, Mirko Bunse, V. Fallah Ramazani, L. del Peral, Estelle Pons, Andrés Baquero, Patricia Márquez, Jorge Otero-Santos, R. Takeishi, Jelena Strišković, E. Prandini, A. Donini, M. Ribó, C. Vigorito, E. Bissaldi, P. Trávnı́ček, V. Rizi, Mario Pecimotika, Ambra Di Piano, B. De Lotto, Sofia Ventura, T. Yamamoto, M. Prouza, J. M. Paredes, I. Agudo, T. Terzić, Antonio Tutone, D. Doré, Nuria Álvarez Crespo, G. Verna, K. Terauchi, S. Caroff, J. Delgado, Davide Miceli, T. Nakamori, M. Nievas Rosillo, Martin Vacula, Diego F. Torres, Wei Zhang, Vladimír Novotný, A. De Angelis, V. Karas, J. Takata, Tomohiko Oka, V. Voitsekhovskyi, Pooja Bhattacharjee, G. Marsella, C. Arcaro, C. Aramo, Lluís Freixas Coromina, Lea Heckmann, A. Arbet Engels, P. H. T. Tam, David Geyer, Lihong Wan, Christoph Toennis, Katsuaki Asano, G. Ceribella, G. Bonnoli, L. Foffano, F. Schiavone, A. Stamerra, L. Burmistrov, Alessandro Costa, M. Teshima, M. Doro, D. Mazin, Bernd Schleicher, A. Lamastra, N. Giglietto, D. Dominis Prester, Miguel J. A. Láinez, H. Katagiri, M. D. Rodríguez-Friás, D. Nieto Castaño, Raniere de Menezes, Kentaro Noda, S. Vercellone, R. Imazawa, J. Houles, M. Mallamaci, Elisa Visentin, J. Cortina, T. Hassan, G. Maurin, Felix Schmuckermaier, T. Yoshikoshi, W. Rhode, D. della Volpe, Arshia Ruina, Arnau Aguasca-Cabot, S. Mičanović, F. Longo, M. Will, D. Elsäesser, D. Ambrosino, Ilaria Viale, J. Martı́, G. Pirola, T. Montaruli, M. Manganaro, Jakub Jurýšek, Davide Cerasole, A. Okumura, A. Cifuentes, Yusuke Inome, M. Ohishi, Hiroyuki Kubo, David A. Green, Irene Jiménez Martínez, A. Berti, J. M. Miranda, Tomohiro Inada, R. López-Coto, T. Schweizer, P. Ottanelli, Alessandro Vigliano, Dai Tateishi, A. Carosi, Chiara Righi, Shuta Tanaka, Oibar Martínez, Lukas Nickel, P. Gliwny, J. Kushida, M. Cardillo, M. Makariev, H. Takahashi, Takayuki Saito, M. Peresano, Yuhua Yao, Giorgio Brunelli, A. Morselli, L. A. Antonelli, Y. Ohtani, Y. Chai, M. Palatiello, L. Di Venere, A. Bulgarelli, C. Plard, J. Bernete, Felix Pfeifle, N. Castrejón, Gloria Maria Cicciari, L. Lemoigne, D. A. Sanchez⋆, Y. Suda, Carlos Barrera-Díaz, J. J. Lozano Bahilo, Yusuke Sato, Marcos López, Rune Michael Dominik, Víctor Moya, S. Nozaki, J. Jiménez Quiles, Juan Escudero, A. Chiavassa, Marie-Sophie Carrasco, F.R. Pantaleo, R. Mirzoyan, A. Abhishek, H. Tajima, A. Lorini, M. Buscemi, J. Giesbrecht Paiva, R. Di Tria, J. Herrera Llorente, N. Godinović, E. Pietropaolo, K. Hayashi, A. Fiasson, S. Loporchio, P. Da Vela, M. Kagaya, F. Ferrarotto, A. Simongini, J. Kataoka, F. Acero, M. Iori, Jonas Hackfeld, E. Mestre Guillen, R. Orito, S. Gunji, L. Chytka, D. Dorner, D. Mandat, F. Cassol, M. Tluczykont, D. Hrupec, D. Paneque, S. Nagataki, M. Takahashi, F. Di Pierro, J. Becerra González, G. Chon, M. Molero Gonzalez, R. Del Burgo, A. Baktash, K. Nishijima, F. Giordano, D Gasparrini, M. Dalchenko, D. Hadasch, H. Costantini, Shosuke Inoue, M. Iarlori, Miroslav Hrabovský, L. Barrios Jiménez, J Wójtowicz, Katherine C. Cheng, Rafaela García López, K. Abe, D. Hui, P. Aubert, T. Tavernier, T Mizuno, E. Owen, M. Chikawa, Ia. Bezshyiko, P.K.H. Yeung, J.L. Contreras, D. Kerszberg, G. Martı́nez, Bastien Lacave, H. Luciani, J. Méndez-Gallego, G. Borkowski, Tomohiro C. Yoshida, L. Nikolić, J. Jahanvi
article en
8 citations

Abstract

Context. The recurrent nova RS Ophiuchi (RS Oph) underwent a thermonuclear eruption in August 2021. In this event, RS Oph was detected by the High Energy Stereoscopic System (H.E.S.S.), the Major Atmospheric Gamma Imaging Cherenkov (MAGIC), and the first Large-Sized Telescope (LST-1) of the future Cherenkov Telescope Array Observatory (CTAO) at very-high gamma-ray energies above 100 GeV. This means that novae are a new class of very-high-energy (VHE) gamma-ray emitters. Aims. We report the analysis of the RS Oph observations with LST-1. We constrain the particle population that causes the observed emission in hadronic and leptonic scenarios. Additionally, we study the prospects of detecting further novae using LST-1 and the upcoming LST array of CTAO-North. Methods. We conducted target-of-opportunity observations with LST-1 from the first day of this nova event. The data were analysed in the framework of cta-lstchain and Gammapy , the official CTAO-LST reconstruction and analysis packages. One-zone hadronic and leptonic models were considered to model the gamma-ray emission of RS Oph using the spectral information from Fermi -LAT and LST-1, together with public data from the MAGIC and H.E.S.S. telescopes. Results. RS Oph was detected at 6.6 σ with LST-1 in the first 6.35 hours of observations following the eruption. The hadronic scenario is preferred over the leptonic scenario considering a proton energy spectrum with a power-law model with an exponential cutoff whose position increases from (0.26 ± 0.08) TeV on day 1 up to (1.6 ± 0.6) TeV on day 4 after the eruption. The deep sensitivity and low energy threshold of the LST-1/LST array will allow us to detect faint novae and increase their discovery rate.

Astronomy and AstrophysicsVol. 695
Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Laboratoire d’Annecy de Physique des Particules (FR), Astrophysique, Instrumentation et Modélisation (FR), Centre de physique des particules de Marseille (FR), Laboratoire de Physique Nucléaire et de Hautes Énergies (FR), CEA Paris-Saclay (FR), Institut de Recherche sur les Lois Fondamentales de l'Univers (FR)
National Science Foundation, Sveučilište u Zagrebu, European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Fundação de Amparo à Pesquisa do Estado de São Paulo, Ministerstvo Školství, Mládeže a Tělovýchovy, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Hrvatska Zaklada za Znanost, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Fundação Araucária, Sveučilište Josipa Jurja Strossmayera u Osijeku, Ministério da Ciência, Tecnologia, Inovações e Comunicações, Staatssekretariat für Bildung, Forschung und Innovation
Openalex Percentile: Top 1%
Astrophysics and Cosmic Phenomena
14.96
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