| Design concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomy CTA Consortium J. Knapp@ leeds. ac. uk http://www. cta-observatory. org, ... Experimental Astronomy 32, 193-316, 2011 | 988 | 2011 |
| Introducing the CTA concept BS Acharya, M Actis, T Aghajani, G Agnetta, J Aguilar, F Aharonian, ... Astroparticle physics 43, 3-18, 2013 | 799 | 2013 |
| Science with the cherenkov telescope array BS Acharya, I Agudo, I Al Samarai, R Alfaro, J Alfaro, C Alispach, ... | 582* | 2019 |
| Hyper-Kamiokande design report K Abe, K Abe, H Aihara, A Aimi, R Akutsu, C Andreopoulos, I Anghel, ... arXiv preprint arXiv:1805.04163, 2018 | 486 | 2018 |
| Testing the hadronuclear origin of PeV neutrinos observed with IceCube K Murase, M Ahlers, BC Lacki Physical Review D—Particles, Fields, Gravitation, and Cosmology 88 (12), 121301, 2013 | 437 | 2013 |
| Hidden cosmic-ray accelerators as an origin of TeV-PeV cosmic neutrinos K Murase, D Guetta, M Ahlers Physical Review Letters 116 (7), 071101, 2016 | 345 | 2016 |
| Diffuse neutrino intensity from the inner jets of active galactic nuclei: Impacts of external photon fields and the blazar sequence K Murase, Y Inoue, CD Dermer Physical Review D 90 (2), 023007, 2014 | 337 | 2014 |
| TeV–PeV neutrinos from low-power gamma-ray burst jets inside stars K Murase, K Ioka Physical Review Letters 111 (12), 121102, 2013 | 328 | 2013 |
| A multimessenger picture of the flaring blazar TXS 0506+ 056: Implications for high-energy neutrino emission and cosmic-ray acceleration A Keivani, K Murase, M Petropoulou, DB Fox, SB Cenko, S Chaty, ... The Astrophysical Journal 864 (1), 84, 2018 | 294 | 2018 |
| High-energy neutrinos and cosmic rays from low-luminosity gamma-ray bursts? K Murase, K Ioka, S Nagataki, T Nakamura The Astrophysical Journal 651 (1), L5, 2006 | 276 | 2006 |
| A panchromatic view of the restless SN 2009ip reveals the explosive ejection of a massive star envelope R Margutti, D Milisavljevic, AM Soderberg, R Chornock, BA Zauderer, ... The Astrophysical Journal 780 (1), 21, 2013 | 266 | 2013 |
| Open questions in cosmic-ray research at ultrahigh energies R Alves Batista, J Biteau, M Bustamante, K Dolag, R Engel, K Fang, ... Frontiers in Astronomy and Space Sciences 6, 23, 2019 | 258 | 2019 |
| Probing the Galactic origin of the IceCube excess with gamma rays M Ahlers, K Murase Physical Review D 90 (2), 023010, 2014 | 252 | 2014 |
| Constraining high-energy cosmic neutrino sources: Implications and prospects K Murase, E Waxman Physical Review D 94 (10), 103006, 2016 | 250 | 2016 |
| A burst in a wind bubble and the impact on baryonic ejecta: high-energy gamma-ray flashes and afterglows from fast radio bursts and pulsar-driven supernova remnants K Murase, K Kashiyama, P Mészáros Monthly Notices of the Royal Astronomical Society 461 (2), 1498-1511, 2016 | 249 | 2016 |
| Star-forming galaxies as the origin of diffuse high-energy backgrounds: Gamma-ray and neutrino connections, and implications for starburst history I Tamborra, S Ando, K Murase Journal of Cosmology and Astroparticle Physics 2014 (09), 043, 2014 | 246 | 2014 |
| Blazars as ultra-high-energy cosmic-ray sources: implications for TeV gamma-ray observations K Murase, CD Dermer, H Takami, G Migliori The Astrophysical Journal 749 (1), 63, 2012 | 243 | 2012 |
| The giant radio array for neutrino detection (GRAND): science and design J Alvarez-Muniz, R Alves Batista, A Balagopal V, J Bolmont, ... Science China Physics, Mechanics & Astronomy 63 (1), 219501, 2020 | 242 | 2020 |
| High-energy cosmic-ray nuclei from high- and low-luminosity gamma-ray bursts and implications for multimessenger astronomy K Murase, K Ioka, S Nagataki, T Nakamura Physical Review D 78 (2), 023005, 2008 | 241 | 2008 |
| High energy neutrino emission and neutrino background<? format?> from gamma-ray bursts in the internal shock model K Murase, S Nagataki Physical Review D—Particles, Fields, Gravitation, and Cosmology 73 (6), 063002, 2006 | 235 | 2006 |
Peter MészárosPennsylvania State University在 psu.edu 的电子邮件经过验证
