Multi-wavelength analysis of the galactic PeVatron candidate LHAASO J2108+5157

G. Pirola; J. Juryšek; M. Balbo; D. Eckert; A. Tramacere; R. Walter; K. Abe; S. Abe; A. Aguasca-Cabot; I. Agudo; N. Alvarez Crespo; L.A. Antonelli; C. Aramo; A. Arbet-Engels; C. Arcaro; M. Artero; K. Asano; P. Aubert; A. Baktash; A. Bamba; A. Baquero Larriva; L. Baroncelli; U. Barres de Almeida; J.A. Barrio; I. Batkovic; J. Baxter; J. Becerra González; E. Bernardini; M.I. Bernardos; J. Bernete Medrano; A. Berti; P. Bhattacharjee; N. Biederbeck; C. Bigongiari; E. Bissaldi; O. Blanch; G. Bonnoli; P. Bordas; A. Bulgarelli; I. Burelli; L. Burmistrov; M. Buscemi; M. Cardillo; S. Caroff; A. Carosi; M.S. Carrasco; F. Cassol; D. Cauz; D. Cerasole; G. Ceribella; Y. Chai; K. Cheng; A. Chiavassa; M. Chikawa; L. Chytka; A. Cifuentes; J.L. Contreras; J. Cortina; H. Costantini; M. Dalchenko; F. Dazzi; A. De Angelis; M. de Bony de Lavergne; B. De Lotto; M. De Lucia; R. de Menezes; L. Del Peral; G. Deleglise; C. Delgado; J. Delgado Mengual; D. della Volpe; M. Dellaiera; A. Di Piano; F. Di Pierro; A. Di Pilato; R. Di Tria; L. Di Venere; C. Díaz; R.M. Dominik; D. Dominis Prester; A. Donini; D. Dorner; M. Doro; L. Eisenberger; D. Elsässer; G. Emery; J. Escudero; V. Fallah Ramazani; G. Ferrara; F. Ferrarotto; A. Fiasson; L. Foffano; L. Freixas Coromina; S. Fröse; S. Fukami; Y. Fukazawa; E. Garcia; R. Garcia López; C. Gasbarra; D. Gasparrini; D. Geyer; J. Giesbrecht Paiva; N. Giglietto; F. Giordano; P. Gliwny; N. Godinovic; R. Grau; J. Green; D. Green; S. Gunji; P. Günther; J. Hackfeld; D. Hadasch; A. Hahn; K. Hashiyama; T. Hassan; K. Hayashi; L. Heckmann; M. Heller; J. Herrera Llorente; K. Hirotani; D. Hoffmann; D. Horns; J. Houles; M. Hrabovsky; D. Hrupec; D. Hui; M. Hütten; M. Iarlori; R. Imazawa; T. Inada; Y. Inome; K. Ioka; M. Iori; K. Ishio; I. Jimenez Martinez; M. Kagaya; V. Karas; H. Katagiri; J. Kataoka; D. Kerszberg; Y. Kobayashi; K. Kohri; A. Kong; H. Kubo; J. Kushida; M. Lainez; G. Lamanna; A. Lamastra; T. Le Flour; M. Linhoff; F. Longo; R. López-Coto; A. López-Oramas; S. Loporchio; A. Lorini; J. Lozano Bahilo; P.L. Luque-Escamilla; P. Majumdar; M. Makariev; D. Mandat; M. Manganaro; G. Manicò; K. Mannheim; M. Mariotti; P. Marquez; G. Marsella; J. Martí; O. Martinez; G. Martínez; M. Martínez; A. Mas-Aguilar; G. Maurin; D. Mazin; E. Mestre Guillen; S. Micanovic; D. Miceli; T. Miener; J.M. Miranda; R. Mirzoyan; T. Mizuno; M. Molero Gonzalez; E. Molina; T. Montaruli; I. Monteiro; A. Moralejo; D. Morcuende; A. Morselli; V. Moya; H. Muraishi; K. Murase; S. Nagataki; T. Nakamori; A. Neronov; L. Nickel; M. Nievas Rosillo; K. Nishijima; K. Noda; D. Nosek; S. Nozaki; M. Ohishi; Y. Ohtani; T. Oka; A. Okumura; R. Orito; J. Otero-Santos; M. Palatiello; D. Paneque; F.R. Pantaleo; R. Paoletti; J.M. Paredes; M. Pech; M. Pecimotika; M. Peresano; F. Pfeiffle; E. Pietropaolo; C. Plard; F. Podobnik; V. Poireau; M. Polo; E. Pons; E. Prandini; J. Prast; G. Principe; C. Priyadarshi; M. Prouza; R. Rando; W. Rhode; M. Ribó; C. Righi; V. Rizi; G. Rodriguez Fernandez; M.D. Rodríguez Frías; T. Saito; S. Sakurai; D.A. Sanchez; T. Šarić; Y. Sato; F.G. Saturni; V. Savchenko; B. Schleicher; F. Schmuckermaier; J.L. Schubert; F. Schussler; T. Schweizer; M. Seglar Arroyo; T. Siegert; R. Silvia; J. Sitarek; V. Sliusar; A. Spolon; J. Strišković; M. Strzys; Y. Suda; H. Tajima; M. Takahashi; H. Takahashi; J. Takata; R. Takeishi; P.H.T. Tam; S.J. Tanaka; D. Tateishi; P. Temnikov; Y. Terada; K. Terauchi; T. Terzic; M. Teshima; M. Tluczykont; F. Tokanai; D.F. Torres; P. Travnicek; S. Truzzi; A. Tutone; M. Vacula; P. Vallania; J. van Scherpenberg; M. Vázquez Acosta; I. Viale; A. Vigliano; C.F. Vigorito; V. Vitale; G. Voutsinas; I. Vovk; T. Vuillaume; Z. Wei; M. Will; T. Yamamoto; R. Yamazaki; T. Yoshida; T. Yoshikoshi; N. Zywucka

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Conference paper

Multi-wavelength analysis of the galactic PeVatron candidate LHAASO J2108+5157

G. Pirola, J. Juryšek, M. Balbo, D. Eckert, A. Tramacere, R. Walter, K. Abe, S. Abe, A. Aguasca-Cabot, I. Agudo, …

Proceedings of Science, Vol.444, 727

09/2024

Abstract

Multidisciplinary

LHAASO J2108+5157 is a recently discovered source, detected in the Ultra-High-Energy band by the LHAASO collaboration. Two molecular clouds were identified in the direction coincident with LHAASO J2108+5157 and, from the spectra reported by LHAASO, there is no sign of an energy cutoff up to 200 TeV. This source makes a promising galactic PeVatron candidate. In 2021, the Large-Sized Telescope prototype (LST-1) of the Cherenkov Telescope Array (CTA) Observatory, collected about 50 hours of quality-selected data on LHAASO J2108+5157. Through these observations, we managed to compute stringent upper limits on the source emission in the multi-TeV band. Together with the analysis of XMM-Newton data and 12 years of Fermi-LAT data, we performed a multi-wavelength study of the source, investigating different possible scenarios of particle acceleration. In this contribution, we will present the results of the analysis, as well as the multi-wavelength modeling, and consequent interpretation of different possible scenarios of emission.

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Title: Multi-wavelength analysis of the galactic PeVatron candidate LHAASO J2108+5157
Translated title: Multi-wavelength analysis of the galactic PeVatron candidate LHAASO J2108+5157
Creators - without role: G. Pirola - Max-Planck-Institut für Physik
J. Juryšek - FZU - Institute of Physics , The Czech Academy of Sciences
M. Balbo - University of Geneva
D. Eckert - University of Geneva
A. Tramacere - University of Geneva
R. Walter - University of Geneva
K. Abe - Tokai University
S. Abe - Institute for Cosmic Ray Research , University of Tokyo
A. Aguasca-Cabot - Institut de Ciències del Cosmos
I. Agudo - Instituto de Astrofísica de Andalucía
N. Alvarez Crespo - Universidad Complutense de Madrid
L.A. Antonelli - INAF - Osservatorio Astronomico di Roma
C. Aramo - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
A. Arbet-Engels - Max-Planck-Institut für Physik
C. Arcaro - INFN Sezione di Padova , Università degli Studi di Padova
M. Artero - Barcelona Institute of Science and Technology
K. Asano - Institute for Cosmic Ray Research , University of Tokyo
P. Aubert - Institut National de Physique Nucléaire et de Physique des Particules
A. Baktash - Universität Hamburg
A. Bamba - Institute for Cosmic Ray Research , University of Tokyo
A. Baquero Larriva - Universidad Complutense de Madrid
L. Baroncelli - Osservatorio di Astrofisica e Scienza dello Spazio
U. Barres de Almeida - Centro Brasileiro de Pesquisas Físicas
J.A. Barrio - Universidad Complutense de Madrid
I. Batkovic - INFN Sezione di Padova , Università degli Studi di Padova
J. Baxter - Institute for Cosmic Ray Research , University of Tokyo
J. Becerra González - Instituto de Astrofísica de Canarias
E. Bernardini - INFN Sezione di Padova , Università degli Studi di Padova
M.I. Bernardos - Instituto de Astrofísica de Andalucía
J. Bernete Medrano - CIEMAT
A. Berti - Max-Planck-Institut für Physik
P. Bhattacharjee - Institut National de Physique Nucléaire et de Physique des Particules
N. Biederbeck - TU Dortmund University
C. Bigongiari - INAF - Osservatorio Astronomico di Roma
E. Bissaldi - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
O. Blanch - Barcelona Institute of Science and Technology
G. Bonnoli - Brera Astronomical Observatory
P. Bordas - Institut de Ciències del Cosmos
A. Bulgarelli - Osservatorio di Astrofisica e Scienza dello Spazio
I. Burelli - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
L. Burmistrov - University of Geneva
M. Buscemi - Istituto Nazionale di Fisica Nucleare, Sezione di Catania
M. Cardillo - INAF - Istituto di Astrofisica e Planetologia Spaziali (IAPS)
S. Caroff - Institut National de Physique Nucléaire et de Physique des Particules
A. Carosi - INAF - Osservatorio Astronomico di Roma
M.S. Carrasco - Institut National de Physique Nucléaire et de Physique des Particules
F. Cassol - Institut National de Physique Nucléaire et de Physique des Particules
D. Cauz - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
D. Cerasole - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
G. Ceribella - Max-Planck-Institut für Physik
Y. Chai - Max-Planck-Institut für Physik
K. Cheng - Institute for Cosmic Ray Research , University of Tokyo
A. Chiavassa - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
M. Chikawa - Institute for Cosmic Ray Research , University of Tokyo
L. Chytka - Palacký University Olomouc
A. Cifuentes - CIEMAT
J.L. Contreras - Universidad Complutense de Madrid
J. Cortina - CIEMAT
H. Costantini - Institut National de Physique Nucléaire et de Physique des Particules
M. Dalchenko - University of Geneva
F. Dazzi - INAF - Osservatorio Astronomico di Roma
A. De Angelis - Istituto Nazionale di Fisica Nucleare, Sezione di Padova
M. de Bony de Lavergne - Institut National de Physique Nucléaire et de Physique des Particules
B. De Lotto - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
M. De Lucia - Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
R. de Menezes - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
L. Del Peral - University of Alcalá UAH
G. Deleglise - Institut National de Physique Nucléaire et de Physique des Particules
C. Delgado - CIEMAT
J. Delgado Mengual - Port d'Informació Científica
D. della Volpe - University of Geneva
M. Dellaiera - Institut National de Physique Nucléaire et de Physique des Particules
A. Di Piano - Osservatorio di Astrofisica e Scienza dello Spazio
F. Di Pierro - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
A. Di Pilato - University of Geneva
R. Di Tria - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
L. Di Venere - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
C. Díaz - CIEMAT
R.M. Dominik - TU Dortmund University
D. Dominis Prester - University of Rijeka
A. Donini - INAF - Osservatorio Astronomico di Roma
D. Dorner - Institute for Theoretical Physics and Astrophysics , Universität Würzburg
M. Doro - INFN Sezione di Padova , Università degli Studi di Padova
L. Eisenberger - Institute for Theoretical Physics and Astrophysics , Universität Würzburg
D. Elsässer - TU Dortmund University
G. Emery - Institut National de Physique Nucléaire et de Physique des Particules
J. Escudero - Instituto de Astrofísica de Andalucía
V. Fallah Ramazani - Institut für Theoretische Physik , Lehrstuhl IV: Plasma-Astroteilchenphysik , Ruhr-Universität Bochum
G. Ferrara - Istituto Nazionale di Fisica Nucleare, Sezione di Catania
F. Ferrarotto - INFN Sezione di Roma La Sapienza
A. Fiasson - Institut National de Physique Nucléaire et de Physique des Particules
L. Foffano - INAF - Istituto di Astrofisica e Planetologia Spaziali (IAPS)
L. Freixas Coromina - CIEMAT
S. Fröse - TU Dortmund University
S. Fukami - Institute for Cosmic Ray Research , University of Tokyo
Y. Fukazawa - Hiroshima University
E. Garcia - Institut National de Physique Nucléaire et de Physique des Particules
R. Garcia López - Instituto de Astrofísica de Canarias
C. Gasbarra - INFN Sezione di Roma Tor Vergata
D. Gasparrini - INFN Sezione di Roma Tor Vergata
D. Geyer - TU Dortmund University
J. Giesbrecht Paiva - Centro Brasileiro de Pesquisas Físicas
N. Giglietto - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
F. Giordano - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
P. Gliwny - Faculty of Physics and Applied Informatics , University of Lodz
N. Godinovic - University of Split
R. Grau - Barcelona Institute of Science and Technology
J. Green - Max-Planck-Institut für Physik
D. Green - Max-Planck-Institut für Physik
S. Gunji - Yamagata University
P. Günther - Institute for Theoretical Physics and Astrophysics , Universität Würzburg
J. Hackfeld - Institut für Theoretische Physik , Lehrstuhl IV: Plasma-Astroteilchenphysik , Ruhr-Universität Bochum
D. Hadasch - Institute for Cosmic Ray Research , University of Tokyo
A. Hahn - Max-Planck-Institut für Physik
K. Hashiyama - Institute for Cosmic Ray Research , University of Tokyo
T. Hassan - CIEMAT
K. Hayashi - Institute for Cosmic Ray Research , University of Tokyo
L. Heckmann - Max-Planck-Institut für Physik
M. Heller - University of Geneva
J. Herrera Llorente - Instituto de Astrofísica de Canarias
K. Hirotani - Institute for Cosmic Ray Research , University of Tokyo
D. Hoffmann - Institut National de Physique Nucléaire et de Physique des Particules
D. Horns - Universität Hamburg
J. Houles - Institut National de Physique Nucléaire et de Physique des Particules
M. Hrabovsky - Palacký University Olomouc
D. Hrupec - University of Osijek
D. Hui - Institute for Cosmic Ray Research , University of Tokyo
M. Hütten - Institute for Cosmic Ray Research , University of Tokyo
M. Iarlori - Gran Sasso Science Institute
R. Imazawa - Hiroshima University
T. Inada - Institute for Cosmic Ray Research , University of Tokyo
Y. Inome - Institute for Cosmic Ray Research , University of Tokyo
K. Ioka - Kyoto University
M. Iori - INFN Sezione di Roma La Sapienza
K. Ishio - Faculty of Physics and Applied Informatics , University of Lodz
I. Jimenez Martinez - CIEMAT
M. Kagaya - Institute for Cosmic Ray Research , University of Tokyo
V. Karas - Czech Academy of Sciences, Astronomical Institute
H. Katagiri - Ibaraki University
J. Kataoka - Waseda University
D. Kerszberg - Barcelona Institute of Science and Technology
Y. Kobayashi - Institute for Cosmic Ray Research , University of Tokyo
K. Kohri - Institute of Particle and Nuclear Studies
A. Kong - Institute for Cosmic Ray Research , University of Tokyo
H. Kubo - Institute for Cosmic Ray Research , University of Tokyo
J. Kushida - Tokai University
M. Lainez - Universidad Complutense de Madrid
G. Lamanna - Institut National de Physique Nucléaire et de Physique des Particules
A. Lamastra - INAF - Osservatorio Astronomico di Roma
T. Le Flour - Institut National de Physique Nucléaire et de Physique des Particules
M. Linhoff - TU Dortmund University
F. Longo - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
R. López-Coto - Instituto de Astrofísica de Andalucía
A. López-Oramas - Instituto de Astrofísica de Canarias
S. Loporchio - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
A. Lorini - Terra
J. Lozano Bahilo - University of Alcalá UAH
P.L. Luque-Escamilla - Universidad de Jaén
P. Majumdar - Institute for Cosmic Ray Research , University of Tokyo
M. Makariev - Bulgarian Academy of Sciences
D. Mandat - FZU - Institute of Physics , The Czech Academy of Sciences
M. Manganaro - University of Rijeka
G. Manicò - Istituto Nazionale di Fisica Nucleare, Sezione di Catania
K. Mannheim - Institute for Theoretical Physics and Astrophysics , Universität Würzburg
M. Mariotti - INFN Sezione di Padova , Università degli Studi di Padova
P. Marquez - Barcelona Institute of Science and Technology
G. Marsella - Istituto Nazionale di Fisica Nucleare, Sezione di Catania
J. Martí - Universidad de Jaén
O. Martinez - Universidad Complutense de Madrid
G. Martínez - CIEMAT
M. Martínez - Barcelona Institute of Science and Technology
A. Mas-Aguilar - Universidad Complutense de Madrid
G. Maurin - Institut National de Physique Nucléaire et de Physique des Particules
D. Mazin - Institute for Cosmic Ray Research , University of Tokyo
E. Mestre Guillen - Universidad de Jaén
S. Micanovic - University of Rijeka
D. Miceli - INFN Sezione di Padova , Università degli Studi di Padova
T. Miener - Universidad Complutense de Madrid
J.M. Miranda - Universidad Complutense de Madrid
R. Mirzoyan - Max-Planck-Institut für Physik
T. Mizuno - Hiroshima University
M. Molero Gonzalez - Instituto de Astrofísica de Canarias
E. Molina - Institut de Ciències del Cosmos
T. Montaruli - University of Geneva
I. Monteiro - Institut National de Physique Nucléaire et de Physique des Particules
A. Moralejo - Barcelona Institute of Science and Technology
D. Morcuende - Instituto de Astrofísica de Andalucía
A. Morselli - INFN Sezione di Roma Tor Vergata
V. Moya - Universidad Complutense de Madrid
H. Muraishi - Kitasato University
K. Murase - Institute for Cosmic Ray Research , University of Tokyo
S. Nagataki - Search
T. Nakamori - Yamagata University
A. Neronov - École Polytechnique
L. Nickel - TU Dortmund University
M. Nievas Rosillo - Instituto de Astrofísica de Canarias
K. Nishijima - Tokai University
K. Noda - Institute for Cosmic Ray Research , University of Tokyo
D. Nosek - Charles University
S. Nozaki - Max-Planck-Institut für Physik
M. Ohishi - Institute for Cosmic Ray Research , University of Tokyo
Y. Ohtani - Institute for Cosmic Ray Research , University of Tokyo
T. Oka - Kyoto University
A. Okumura - Nagoya University
R. Orito - Tokushima University
J. Otero-Santos - Instituto de Astrofísica de Canarias
M. Palatiello - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
D. Paneque - Max-Planck-Institut für Physik
F.R. Pantaleo - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
R. Paoletti - Terra
J.M. Paredes - Institut de Ciències del Cosmos
M. Pech - Palacký University Olomouc
M. Pecimotika - University of Rijeka
M. Peresano - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
F. Pfeiffle - Institute for Theoretical Physics and Astrophysics , Universität Würzburg
E. Pietropaolo - Gran Sasso Science Institute
C. Plard - Institut National de Physique Nucléaire et de Physique des Particules
F. Podobnik - Terra
V. Poireau - Institut National de Physique Nucléaire et de Physique des Particules
M. Polo - CIEMAT
E. Pons - Institut National de Physique Nucléaire et de Physique des Particules
E. Prandini - INFN Sezione di Padova , Università degli Studi di Padova
J. Prast - Institut National de Physique Nucléaire et de Physique des Particules
G. Principe - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
C. Priyadarshi - Barcelona Institute of Science and Technology
M. Prouza - FZU - Institute of Physics , The Czech Academy of Sciences
R. Rando - INFN Sezione di Padova , Università degli Studi di Padova
W. Rhode - TU Dortmund University
M. Ribó - Institut de Ciències del Cosmos
C. Righi - Brera Astronomical Observatory
V. Rizi - Gran Sasso Science Institute
G. Rodriguez Fernandez - INFN Sezione di Roma Tor Vergata
M.D. Rodríguez Frías - University of Alcalá UAH
T. Saito - Institute for Cosmic Ray Research , University of Tokyo
S. Sakurai - Institute for Cosmic Ray Research , University of Tokyo
D.A. Sanchez - Institut National de Physique Nucléaire et de Physique des Particules
T. Šarić - University of Split
Y. Sato - Aoyama Gakuin University
F.G. Saturni - INAF - Osservatorio Astronomico di Roma
V. Savchenko - École Polytechnique
B. Schleicher - Institute for Theoretical Physics and Astrophysics , Universität Würzburg
F. Schmuckermaier - Max-Planck-Institut für Physik
J.L. Schubert - TU Dortmund University
F. Schussler - Université Paris-Saclay
T. Schweizer - Max-Planck-Institut für Physik
M. Seglar Arroyo - Institut National de Physique Nucléaire et de Physique des Particules
T. Siegert - Institute for Theoretical Physics and Astrophysics , Universität Würzburg
R. Silvia - Istituto Nazionale di Fisica Nucleare, Sezione di Bari
J. Sitarek - Faculty of Physics and Applied Informatics , University of Lodz
V. Sliusar - University of Geneva
A. Spolon - INFN Sezione di Padova , Università degli Studi di Padova
J. Strišković - University of Osijek
M. Strzys - Institute for Cosmic Ray Research , University of Tokyo
Y. Suda - Hiroshima University
H. Tajima - Nagoya University
M. Takahashi - Nagoya University
H. Takahashi - Hiroshima University
J. Takata - Institute for Cosmic Ray Research , University of Tokyo
R. Takeishi - Institute for Cosmic Ray Research , University of Tokyo
P.H.T. Tam - Institute for Cosmic Ray Research , University of Tokyo
S.J. Tanaka - Aoyama Gakuin University
D. Tateishi - Saitama University
P. Temnikov - Bulgarian Academy of Sciences
Y. Terada - Saitama University
K. Terauchi - Kyoto University
T. Terzic - University of Rijeka
M. Teshima - Institute for Cosmic Ray Research , University of Tokyo
M. Tluczykont - Universität Hamburg
F. Tokanai - Yamagata University
D.F. Torres - Institució Catalana de Recerca i Estudis Avançats
P. Travnicek - FZU - Institute of Physics , The Czech Academy of Sciences
S. Truzzi - Terra
A. Tutone - INAF - Osservatorio Astronomico di Roma
M. Vacula - Palacký University Olomouc
P. Vallania - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
J. van Scherpenberg - Max-Planck-Institut für Physik
M. Vázquez Acosta - Instituto de Astrofísica de Canarias
I. Viale - INFN Sezione di Padova , Università degli Studi di Padova
A. Vigliano - Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
C.F. Vigorito - Istituto Nazionale di Fisica Nucleare, Sezione di Torino
V. Vitale - INFN Sezione di Roma Tor Vergata
G. Voutsinas - University of Geneva
I. Vovk - Institute for Cosmic Ray Research , University of Tokyo
T. Vuillaume - Institut National de Physique Nucléaire et de Physique des Particules
Z. Wei - Institució Catalana de Recerca i Estudis Avançats
M. Will - Max-Planck-Institut für Physik
T. Yamamoto - Konan University
R. Yamazaki - Aoyama Gakuin University
T. Yoshida - Ibaraki University
T. Yoshikoshi - Institute for Cosmic Ray Research , University of Tokyo
N. Zywucka - Faculty of Physics and Applied Informatics , University of Lodz
Identifiers: 9957788252906774
Academic Unit: Institute of Astronomy, College of Science, National Tsing Hua University
Language: English
Resource Type: Conference paper
Publication Details: Proceedings of Science, Vol.444, 727

Multi-wavelength analysis of the galactic PeVatron candidate LHAASO J2108+5157

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