output
20202026
most citedSN 2019ehk: A Double-Peaked Ca-rich Transient with Luminous X-ray Emission and Shock-Ionized Spectral Features

70 citations

42 papers

nucl-ex2026

Indirect Measurement of the Factor for at Gamow Energies via the Trojan Horse Method with Near-0 degree Spectator Detection

Chengbo Li, Huiming Jia, Qungang Wen +8

The astrophysical S*(E) factor for the 12C+12C reaction within the Gamow window plays a pivotal role in modeling stellar carbon burning and explosive nucleosynthesis scenarios. How…

nucl-ex2026

measurement of the reaction at astrophysical energies via the Trojan horse method with quasi-free breakup

Chengbo Li, Huiming Jia, Qungang Wen +9

The 12C(12C,a)20Ne reaction at astrophysical energies is crucial for understanding the carbon burning process in massive star and explosive astrophysical scenarios like Type Ia sup…

cs.AI2026

SymDiag: Explainable Diagnosis for LLM Reasoning via Neuro-Symbolic Verification

Wenyao Cui, Huaping Zhang, Yongyi Huang +6

Large language models (LLMs) increasingly serve as data-driven reasoners, yet their chains-of-thought (CoT) can be unfaithful even when final answers are correct. Most existing ``v…

cs.RO2026

Disentangling Visuo-Tactile Foresight: Oracle-Guided Interface Discovery for World Action Models

Zihang Yao, Chaoyue Ding, Yingying Yu

Contact-rich manipulation remains challenging because successful control depends on physical interaction cues that are often weakly observable from vision alone. Recent tactile wor…

astro-ph.GA2026

The complex kinematics of the young stars orbiting the supermassive black hole in the Galactic center can be explained by the presence of an intermediate mass companion of Sgr A

Xiaochen Zheng, Long Wang, Douglas N. C. Lin +2

The sub-parsec proximity around the Sgr A supermassive black hole (SMBH) in the center of the Milky Way contains an inner cluster of eccentric S-stars with randomly oriente…

astro-ph.SR2026

GSC 08227-00723: An Unusually Large PSH Excess AH Pic Candidate

Xin Li, Yongkang Sun

Nova-like variables are high-accretion-rate cataclysmic variables (CVs) that, in contrast to dwarf novae, do not undergo outbursts caused by thermal-viscous instability. However, a…