activity
20142024
most citedDoppler images of the eclipsing binary ER Vulpeculae

14 citations · 29 across the 8 of their papers we have counts for

collaborators

8 papers

cs.CL2024

SimulBench: Evaluating Language Models with Creative Simulation Tasks

Qi Jia, Xiang Yue, Tianyu Zheng +2

We introduce SimulBench, a benchmark designed to evaluate large language models (LLMs) across a diverse collection of creative simulation scenarios, such as acting as a Linux termi…

astro-ph.EP20245 cited

A method of photometric data extraction for asteroids from time-domain surveys

Xiaoyun Xu, Xiaobing Wang, Karri Muinonen +9

The lightcurves of asteroids are essential for determining their physical characteristics, including shape, spin, size, and surface composition. However, most asteroids are missing…

astro-ph.SR2024

Stellar cycle and evolution of polar spots in an M+WD binary

Xinlin Zhao, Song Wang, Xue Li +4

Stellar activity cycles reveal continuous relaxation and induction of magnetic fields. The activity cycle is typically traced through the observation of cyclic variations in total…

astro-ph.SR2023

First Chromospheric Activity and Doppler Imaging Study of PW And Using a New Doppler Imaging Code: SpotDIPy

Engin Bahar, Hakan V. Şenavcı, Emre Işık +4

Measuring coverage of dark spots on cool stars is important in understanding how stellar magnetic activity scales with the rotation rate and convection zone depth. In this respect,…

cs.LG20232 cited

Cerberus: A Deep Learning Hybrid Model for Lithium-Ion Battery Aging Estimation and Prediction Based on Relaxation Voltage Curves

Yue Xiang, Bo Jiang, Haifeng Dai

The degradation process of lithium-ion batteries is intricately linked to their entire lifecycle as power sources and energy storage devices, encompassing aspects such as performan…

astro-ph.SR20231 cited

Magnetic topologies of two weak-line T Tauri stars TAP 4 and TAP 40

Yue Xiang, Shenghong Gu, J. -F. Donati +3

We present a Zeeman-Doppler imaging study of two weak-line T Tauri stars TAP 4 and TAP 40, based on the high-resolution spectropolarimetric observations with ESPaDOnS at the Canada…