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---
license: mit
dataset_info:
- config_name: distributions
  features:
  - name: image
    dtype: image
  - name: id
    dtype: int64
  - name: data
    list: float64
  - name: true_params
    dtype: string
  splits:
  - name: dist_easy
    num_bytes: 1190665
    num_examples: 50
  - name: dist_hard
    num_bytes: 2389492
    num_examples: 100
  - name: dist_astro
    num_bytes: 824106
    num_examples: 50
  download_size: 4367800
  dataset_size: 4404263
- config_name: timeseries
  features:
  - name: image
    dtype: image
  - name: id
    dtype: int64
  - name: dates
    list: timestamp[s]
  - name: data
    list: float64
  splits:
  - name: ts_easy
    num_bytes: 3202262
    num_examples: 50
  - name: ts_hard
    num_bytes: 7169969
    num_examples: 110
  - name: ts_astro
    num_bytes: 5424118
    num_examples: 50
  download_size: 15807487
  dataset_size: 15796349
configs:
- config_name: distributions
  data_files:
  - split: dist_easy
    path: distributions/dist_easy-*
  - split: dist_hard
    path: distributions/dist_hard-*
  - split: dist_astro
    path: distributions/dist_astro-*
- config_name: timeseries
  data_files:
  - split: ts_easy
    path: timeseries/ts_easy-*
  - split: ts_hard
    path: timeseries/ts_hard-*
  - split: ts_astro
    path: timeseries/ts_astro-*

---

# DAWN Dataset

DAWN benchmarks AI agents on two core data science tasks: distribution fitting and time series modeling. Both domains are organized into Easy, Hard, and Astro splits, with synthetically generated data to allow robust measurement of model fit.

## VESTA: Visual Exploration with Statistical Tool Agents 
We propose and benchmark AI agents on DAWN in our arxiv paper: https://arxiv.org/abs/2606.00384 

Fitting quantitative models to data is a central step in scientific workflows, yet it
remains one of the least automated. Recent agent-based systems leverage language
and vision-language models (VLMs) to iteratively propose and refine statistical
models, but these systems struggle on more challenging modeling tasks. To address
these limitations, we introduce VESTA (Visual Exploration with Statistical Tool
Agents), a framework that equips VLMs with a dynamically growing exploration
toolkit to guide model refinement through data transformations, hypothesis-driven
visualizations, and robust statistical tests. Unlike prior systems that rely on iterative
critique alone, VESTA actively explores data before and during refinement by
selecting or creating diagnostic tools, which accumulate in the model’s context and
can be reused later. We evaluate VESTA against established baselines in three toolkit
configurations: no tools, static expert-written tools, and dynamic model-written
tools. To support this evaluation, we introduce DAWN (Dataset for Automated
Workflows and Numerical Modeling), a benchmark targeting distribution fitting
and time series modeling with varying difficulty tiers, and culminating in real-world
astronomy tasks including modeling initial mass functions and gravitational-wave
chirp signals. We find that VESTA’s dynamic tool creation outperforms prior agentic
pipelines, with the largest gains on complex and domain-specific tasks. We further
show that dynamically generated tools are substantially more sophisticated than
those produced by existing visual tool-creation systems, covering more diagnostic
categories per function and strongly preferring visual outputs that the VLM critic
can reason over directly.

## Distribution Fitting

- **dist_easy**: Identify the family and parameters of a unimodal distribution. Families include gaussian, lognormal, student-t, exponential, uniform, weibull, laplace, cauchy, and pareto, with priors and sample sizes randomly sampled.
- **dist_hard**: Mixtures of exactly two distributions from the families above, reflecting real-world phenomena such as gaussian-laplace mixtures (speech signal processing) and lognormal-exponential mixtures (survival analysis).
- **dist_astro**: Initial mass functions (IMF), describing the distribution of stellar masses at birth. Includes five functional forms: Salpeter (single power law), Kroupa (piecewise power law), Chabrier (log-normal plus power law), and two freeform variants (tight and wide breaks).

## Time Series Modeling

- **ts_easy**: Sequences with simple linear trends (increasing, decreasing, flat) and standard periodic seasonal components, with minimal noise.
- **ts_hard**: More complex dynamics including random walks (ARIMA processes), sigmoidal (S-curve) functions, ECG heartbeat signals, and sales-forecasting-style seasonality with increasing averages. Requires multi-periodic and Gaussian process modeling (e.g. Matérn, RBF kernels).
- **ts_astro**: Time series inspired by gravitational wave chirps, where frequency continuously increases as binary star systems converge, including a variant where amplitude additionally decays over time.

## Dataset Statistics

Each dataset $D_i$ contains $n \in [600, 1500]$ points sampled from a ground-truth distribution or time series, with parameters drawn uniformly from fixed ranges. For each domain and difficulty split, 50 (Easy/Astro) or 100 (Hard) examples are generated, for a total of 200 distributions and 200 time series.

## Citation

If you use DAWN, please cite:

```bibtex
@misc{rudman2026vestavisualexplorationstatistical,
      title={VESTA: Visual Exploration with Statistical Tool Agents}, 
      author={William Rudman and Abhishek Divekar and Kanishk Jain and Sebastian Joseph and Stella S. R. Offner and Matthew Lease and Kyle Mahowald and Greg Durrett and Junyi Jessy Li},
      year={2026},
      eprint={2606.00384},
      archivePrefix={arXiv},
      primaryClass={cs.AI},
      url={https://arxiv.org/abs/2606.00384},
}
```