13 citations · 16 across the 13 of their papers we have counts for
13 papers
Reconstruction of Shower-like Events in NEON Using Likelihood and Graph Neural Network Methods
Sujie Lin, Weiqin Huang, Yihan Liu +3
The Neutrino Observatory in the Nanhai (NEON) is a proposed deep-sea neutrino telescope deployed in the South China Sea. Accurate reconstruction of shower-like events is crucial fo…
Time-dependent multi-energy neutrino emission from symbiotic recurrent novae: the role of accretion disks
Rui Xu, Yudong Cui, Yihan Shi +1
Symbiotic recurrent novae provide a unique laboratory for studying thermonuclear explosions, shock evolution, and nonthermal particle acceleration in dense circumstellar environmen…
Risk assessment of muon single-event effects for low-altitude aircraft
Zijian Qiu, Sujie Lin, Yudong Cui +2
With the rapid development of low-altitude economy, the radiation environment safety of low-altitude aircraft such as drones and electric vertical take-off and landing aircraft has…
Data-driven modeling of Galactic diffuse emission with multi-wavelength observations
Xi Liu, Xiaodong Li, Sujie Lin +4
We present a data-driven investigation of Galactic diffuse emission. Using multi-frequency Planck radio/microwave maps (30-857 GHz) and Fermi-LAT gamma-ray data (50 MeV-814 GeV), w…
LHAASO J18490002: A Hybrid Lepto-Hadronic Interpretation of PeV Gamma-Ray Emission
Yihan Shi, Yudong Cui, Lili Yang
Recently, LHAASO detected gamma-ray emission from the pulsar wind nebula (PWN) J1849-0001 extending up to approximately 2 PeV, providing strong evidence for PeV particle accelerati…
Radio Study of G76.9+1.0 Pulsar Wind Nebula
Haotian Qiu, Yunlei Huang, C-Y. Ng +3
Pulsar Wind Nebulae (PWNe) are key astrophysical laboratories for high energy phenomena. Specifically, radio observations and related polarimetry are essential probes to understand…
Deciphering the IceCube Diffuse Neutrino Observations via AGN Variability
Caijin Xie, Zijian Qiu, Yudong Cui +2
The physical origin of the diffuse neutrino background and its spectral break at 30 TeV remain a major puzzle in multi-messenger astrophysics. In this work, we demonstrate t…
Radio Study of Vela X Cocoon
Yihan Liu, Yu Zhang, C. -Y. Ng +3
The evolution of pulsar Wind Nebulae (PWNe) influences how high energy particles in the vicinity are generated and transport. The Vela PWN (only \,pc away), provides a rat…
SNR G54.1+0.3, a PeVatron candidate unveiled by LHAASO
Yihan Shi, Yudong Cui, Lili Yang
Recently, the LHAASO Collaboration reported the first very-high-energy gamma-ray catalog, containing 90 TeV sources. Among these sources, 1LHAASO J1929+1846u is located 0.3…
Radio Observation of the Pulsar Wind Nebula in SNR G11.2-0.3
Yu Zhang, Yihan Liu, C. -Y. Ng +2
Pulsar wind nebulae (PWNe) are important sources for understanding galactic high-energy processes, but it is controversial until now about how high-energy particles in PWNe are acc…
SNR G54.1+0.3, a PeVatron candidate unveiled by LHAASO
Yihan Shi, Yudong Cui, Lili Yang
Recently, the LHAASO Collaboration presented the first very-high-energy gamma-ray catalog, containing 90 TeV sources. Among these sources, 1LHAASO J1929 +1846u* is located 0.3$^\ci…
A proposed deep sea Neutrino Observatory in the Nanhai
Huiming Zhang, Yudong Cui, Yunlei Huang +7
Over the past ten years, several breakthroughs have been made in multi-messenger astronomy. Thanks to the IceCube Neutrino Observatory, the detection of astrophysical neutrinos was…
The traveling-PWN modeling attempt on the enigmatic LHAASO dumbbell-like structure
Caijin Xie, Yihan Liu, Chengyu Shao +2
The first LHAASO catalog presents six enigmatic ultra-high-energy (UHE) gamma-ray sources with lonely > 25 TeV emission being detected, which are indicated as 1LHAASO: J0007+5659u,…