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Hanzhang Zhao

Publications and source records attributed to Hanzhang Zhao.

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DATE-LM: Benchmarking Data Attribution Evaluation for Large Language Models

Data attribution methods quantify the influence of training data on model outputs and are becoming increasingly relevant for a wide range of LLM research and applications, including dataset curation, model interpretability, data valuation. However, there remain critical gaps in systematic LLM-centric evaluation of data attribution methods. To this end, we introduce DATE-LM (Data Attribution Evaluation in Language Models), a unified benchmark for evaluating data attribution methods through real-world LLM applications. DATE-LM measures attribution quality through three key tasks -- training data selection, toxicity/bias filtering, and factual attribution. Our benchmark is designed for ease of use, enabling researchers to configure and run large-scale evaluations across diverse tasks and LLM architectures. Furthermore, we use DATE-LM to conduct a large-scale evaluation of existing data attribution methods. Our findings show that no single method dominates across all tasks, data attribution methods have trade-offs with simpler baselines, and method performance is sensitive to task-specific evaluation design. Finally, we release a public leaderboard for quick comparison of methods and to facilitate community engagement, with the motivation that DATE-LM can serve as a foundation for future data attribution research in LLMs.

cs.CL

How time weathers galaxies: The temporal impact of the cluster environment on galaxy formation and evolution

We illuminate the altered evolution of galaxies in clusters compared to the field by tracking galaxies in the IllustrisTNG300 simulation as they enter isolated clusters of mass $10^{13} < M_{\rm 200, mean} / {\rm M}_\odot < 10^{15}$ (at $z=0$). We demonstrate significant trends in galaxy properties with residence time (time since first infall) and that there is a population of galaxies that remain star-forming even many Gyrs after their infall. By comparing the properties of galaxies at their infall time to their properties at $z=0$, we show how scaling relations, like the stellar-to-halo mass ratio, shift as galaxies live in the cluster environment. Galaxies with a residence time of 10 Gyr increase their stellar-to-halo mass ratio, by around 1 dex. As measurements of the steepest slope of the galaxy cluster number density profile ($R_{\rm st}$), frequently used as a proxy for the splashback radius, have been shown to depend strongly on galaxy selection, we show how $R_{\rm st}$ depends on galaxy residence time. Using galaxies with residence times less than one cluster crossing time ($\approx 5$ Gyr) to measure $R_{\rm st}$ leads to significant offsets relative to using the entire galaxy population. Galaxies must have had the opportunity to `splash back' to the first caustic to trace out a representative value of $R_{\rm st}$, potentially leading to issues for galaxy surveys using UV-selected galaxies. Our wok demonstrates that the evolution of cluster galaxies continues well into their lifetime in the cluster and departs from a typical field galaxy evolutionary path.

astro-ph.GA