alphaFeedback
astro-ph.HEhep-exhep-phastro-ph.IMastro-phastro-ph.EPastro-ph.SRphysics.ins-detastro-ph.COastro-ph.GA

On Valency

published · living versions
W_p3bttx2a·v1 · currentpublished
Very high energy gamma-ray emission beyond 10 TeV from GRB 221009A
with Zhen Cao, F. Aharonian, Q. An, A. Axikegu +275
1 version

Preprints & journals

37 papers in the corpus · 2004–2025
A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane2510.06786v2 · Zhen Cao, Felix Aharonian, Yunxiang Bai et al.2025 · 0 citationsarXiv
Precise measurements of the cosmic ray proton energy spectrum in the "knee'' region2505.14447v2 · Zhen Cao, F. Aharonian, Y.X. Bai et al.2025 · 17 citationsScience Bulletin 70(2025)4173-4180
Unveiling the Mechanisms of Electron Energy Spectrum Evolution2412.09016v3 · Xu-Lin Dong, Shu-Wei Ma, Yi-Qing Guo et al.2024 · 0 citationsarXiv
An Enigmatic PeVatron in an Area around HII Region G35.6$-$0.52412.00379v2 · Zhen Cao, F. Aharonian, Axikegu et al.2024 · 0 citationsarXiv
Detection of two TeV gamma-ray outbursts from NGC 1275 by LHAASO2411.01215v3 · Zhen Cao, F. Aharonian, Axikegu et al.2024 · 9 citationsarXiv
Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASO2410.13173v3 · Zhen Cao, F. Aharonian, Y.X. Bai et al.2024 · 2 citationsPhys. Rev. D 110, 103017 (2024)
Evidence for particle acceleration approaching PeV energies in the W51 complex2407.00624v3 · Zhen Cao, F. Aharonian, Axikegu et al.2024 · 9 citationsScience Bulletin,2024
Data quality control system and long-term performance monitor of the LHAASO-KM2A2405.11826v3 · Zhen Cao, F. Aharonian, Axikegu et al.2024 · 0 citationsarXiv
Does or did the supernova remnant Cassiopeia A operate as a PeVatron?2310.17082v1 · Zhen Cao, F. Aharonian, Q. An et al.2023 · 10 citationsarXiv
The First LHAASO Catalog of Gamma-Ray Sources2305.17030v2 · Zhen Cao, F. Aharonian, Q. An et al.2023 · 283 citationsThe Astrophysical Journal Supplement Series, 271 (2024) 25
Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations.36608208 · Cao, Zhen, Aharonian, F, An, Q et al.2023 · 41 citationsPhysical review letters. 2022;129(26):261103
Flux Variations of Cosmic Ray Air Showers Detected by LHAASO-KM2A During a Thunderstorm on 10 June 20212207.12601v2 · F. Aharonian, Q. An, Axikegu et al.2022 · 14 citationsChinese Phys. C 47 015001 (2023)
Gamma-Ray Observation of the Cygnus Region in the 100-TeV Energy Region.34328784 · Amenomori, M, Bao, Y W, Bi, X J et al.2021 · 26 citationsPhysical review letters. 2021;127(3):031102
Peta-electron volt gamma-ray emission from the Crab Nebula.34261813 · LHAASO Collaboration, Cao, Zhen, Aharonian, F et al.2021 · 186 citationsScience (New York, N.Y.). 2021;373(6553):425-430
Discovery of a new γ\gamma-ray source LHAASO J0341+5258 with emission up to 200TeV2107.02020v4 · Zhen Cao, F. Aharonian, Q. An et al.2021 · 34 citationsarXiv
Discovery of the Ultra-high energy gamma-ray source LHAASO J2108+51572106.09865v3 · Zhen Cao, F. Aharonian, Q. An et al.2021 · 50 citationsarXiv
Extended Very-High-Energy Gamma-Ray Emission Surrounding PSR J0622+3749 Observed by LHAASO-KM2A.34213924 · Aharonian, F, An, Q, Axikegu et al.2021 · 136 citationsPhysical review letters. 2021;126(24):241103
First Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies.33891464 · Amenomori, M, Bao, Y W, Bi, X J et al.2021 · 224 citationsPhysical review letters. 2021;126(14):141101
Construction and On-site Performance of the LHAASO WFCTA Camera2012.14622v2 · F. Aharonian, Q. An, Axikegu et al.2020 · 29 citationsEur. Phys. J. C 81, 657 (2021)
First Detection of Photons with Energy beyond 100 TeV from an Astrophysical Source.31491288 · Amenomori, M, Bao, Y W, Bi, X J et al.2019 · 202 citationsPhysical review letters. 2019;123(5):051101
Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun.29400499 · Amenomori, M, Bi, X J, Chen, D et al.2018 · 13 citationsPhysical review letters. 2018;120(3):031101
Observation of the thunderstorm-related ground cosmic ray flux variations by ARGO-YBJ1712.01461v3 · B. Bartoli, P. Bernardini, X. J. Bi et al.2017 · 27 citationsPhys. Rev. D 97, 042001 (2018)
Search for Gamma Ray Bursts with the ARGO-YBJ Detector in Shower Mode1703.09284v1 · B. Bartoli, P. Bernardini, X. J. Bi et al.2017 · 15 citationsThe Astrophysical Journal, 2017, 842(31)
Search for GeV Gamma Ray Bursts with the ARGO-YBJ Detector: Summary of Eight Years of Observations1502.05622v1 · B. Bartoli, P. Bernardini, X.J. Bi et al.2015 · 12 citationsAPJ, 794:82 (12pp), 2014 October 10
Probe of the solar magnetic field using the "cosmic-ray shadow" of the sun.24027782 · Amenomori, M, Bi, X J, Chen, D et al.2013 · 50 citationsPhysical review letters. 2013;111(1):011101
A Monte Carlo study to measure the energy spectra of the primary cosmic-ray components at the knee using a new Tibet AS core detector array1303.2919v1 · The Tibet As\gamma Collaboration: M. Amenomori, X. J. Bi, D. Chen et al.2013 · 0 citationsarXiv
Observation of TeV gamma rays from the Cygnus region with the ARGO-YBJ experiment1201.1973v1 · B. Bartoli, P. Bernardini, X. J. Bi et al.2012 · 57 citationsThe Astrophysical Journal Letters, 745:L22 (5pp), 2012
Large-scale sidereal anisotropy of multi-TeV galactic cosmic rays and the heliosphere0909.1026v1 · M. Amenomori, X. J. Bi, D. Chen et al.2009 · 4 citationsarXiv
Anisotropy and corotation of galactic cosmic rays.17053141 · Amenomori, M, Ayabe, S, Bi, X J et al.2006 · 247 citationsScience (New York, N.Y.). 2006;314(5798):439-43
Observation by an air-shower array in Tibet of the multi-TeV cosmic-ray anisotropy due to terrestrial orbital motion around the Sun.15323615 · Amenomori, M, Ayabe, S, Cui, S W et al.2004 · 34 citationsPhysical review letters. 2004;93(6):061101
Career total: 182 works. 37 are in this corpus.

Profile built from the corpus for this byline.

Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.