activity
20242026
collaborators

8 papers

cs.RO2026

Evolve Vision-Language-Action Model into an Agent with On-the-fly Tool-use

Yi Ding, Yanzhao Yu, Xili Dai +5

This paper integrates end-to-end Visual-Language-Action (VLA) models with agentic tool-use to propose Agentic Robot with Tool-use (ART). ART is a tool-injection framework that tune…

astro-ph.GA2026

The cosmic ray ionization rate from H3+ observations can be overestimated due to neglect of time-dependent chemistry

Ka Wai Ho, Munan Gong, Kedron Silsbee +1

The cosmic ray ionization rate (CRIR) is a key parameter governing the physical, chemical and thermal evolution of the interstellar medium. The primary technique for measuring the…

astro-ph.GA2026

modeling of Galactic dust polarized CMB foreground

Alexei G. Kritsuk, Ka Wai Ho, Ka Ho Yuen +1

We present the analysis of high-resolution synthetic dust polarization maps derived from large-scale simulations of magnetized multiphase interstellar turbulence carried out with t…

astro-ph.GA2025

Statistical signatures of interstellar turbulence in dust polarization maps

Ka Wai Ho, Ka Ho Yuen, Raphael Flauger +1

We present results from a high-resolution interstellar turbulence simulation and show that it closely reproduces recent measurements. Our model captures the scaling of $EE…

astro-ph.GA2025

The stable "Unstable Natural Media" due to the presence of turbulence

Ka Wai Ho, Ka Ho Yuen, Alex Lazarian

The term "unstable neutral media" (UNM) has traditionally been used to describe the transient phase formed between the warm and cold neutral hydrogen (HI) phases and has not been t…

astro-ph.GA2024

Tracing magnetic field in super-Alfvenic turbulence with Gradient Technique

Ka Wai Ho, Alex Lazarian

Super-Alfvenic turbulence is important for many astrophysical objects, particularly galaxy clusters. In this paper, we explore the accuracy of Synchrotron Intensity Gradients (SIGs…