ZTF_40k / README.md
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metadata
license: mit
dataset_info:
  features:
    - name: sourceid
      dtype: string
    - name: bands_data
      struct:
        - name: g
          struct:
            - name: feat_dynamic_real
              list: float64
            - name: length
              dtype: int64
            - name: mjd
              list: float64
            - name: past_feat_dynamic_real
              list: float64
            - name: target
              list: float64
        - name: i
          struct:
            - name: feat_dynamic_real
              list: float64
            - name: length
              dtype: int64
            - name: mjd
              list: float64
            - name: past_feat_dynamic_real
              list: float64
            - name: target
              list: float64
        - name: r
          struct:
            - name: feat_dynamic_real
              list: float64
            - name: length
              dtype: int64
            - name: mjd
              list: float64
            - name: past_feat_dynamic_real
              list: float64
            - name: target
              list: float64
    - name: period
      dtype: float64
    - name: class_str
      dtype: string
    - name: ra
      dtype: float64
    - name: dec
      dtype: float64
  splits:
    - name: train
      num_bytes: 874152765
      num_examples: 29047
    - name: validation
      num_bytes: 125721375
      num_examples: 4150
    - name: test
      num_bytes: 247388574
      num_examples: 8301
    - name: anom
      num_bytes: 32708516
      num_examples: 1087
  download_size: 557951471
  dataset_size: 1279971230
configs:
  - config_name: default
    data_files:
      - split: train
        path: data/train-*
      - split: validation
        path: data/validation-*
      - split: test
        path: data/test-*
      - split: anom
        path: data/anom-*

StarEmbed Benchmark Data set

The StarEmbed benchmark data set is available here in huggingface datasets format.

The ~40,000 multi-band ZTF light curves are available at StarEmbed/data. The train/validation/test splits are included alongside the additional anom split used for the OOD benchmarking.

Available columns

Each star in data set has the following fields:

Top-level columns

Column Type Description
sourceid string Catalina Surveys DR1 (CSDR1) source id of the variable star (e.g. CSS_J082956.4-044426)
bands_data dict / struct (keys g, i, r) per-band light curves; each band is a struct (or null if absent) holding the arrays in the table below.
period float64 catalog period of the variable star, in days (range ≈ 0.13 – 885)
class_str string variable-star class label; one of EW, EA, RRab, RRc, RRd, RS CVn, LPV
ra float64 right ascension (J2000) in decimal degrees
dec float64 declination (J2000) in decimal degrees

Per-band fields inside each band of bands_data (g / r / i)

Field Type Description
target list of floats magnitude, measure of brightness (AB system) — the raw light curve
past_feat_dynamic_real list of floats mag_err, 1σ uncertainty on magnitude, aligned with target
feat_dynamic_real list of floats delta_t, time gap (days) between each two consecutive observations
mjd list of floats observation time in Modified Julian Date, aligned with target
length int64 number of observations in this band's light curve

All four splits (train, validation, test, anom) share the identical schema described above. The train/validation/test splits contain the seven in-distribution classes listed under class_str, whereas the anom split is an anomaly-detection holdout whose class_str values are a disjoint set of out-of-distribution classes — Beta_Lyrae, Blazhko, ACEP, Cep-II, HADS, LADS, ELL, Hump, PCEB, EA_UP — that never appear in training.


Citation

This work was accepted to the main track of ICML 2026 as well as the AI4Physics workshop. If you use or refer to this dataset please cite our work.

@article{StarEmbed,
       author = {{Li}, Weijian and {Chen}, Hong-Yu and {Rehemtulla}, Nabeel and {Shah}, Ved G. and {Wu}, Dennis and {Kim}, Dongho and {Lin}, Qinjie and {Miller}, Adam A. and {Liu}, Han},
        title = "{StarEmbed: Benchmarking Time Series Foundation Models on Astronomical Observations of Variable Stars}",
      journal = {arXiv e-prints},
     keywords = {Solar and Stellar Astrophysics, Instrumentation and Methods for Astrophysics, Artificial Intelligence},
         year = 2025,
        month = oct,
          eid = {arXiv:2510.06200},
        pages = {arXiv:2510.06200},
          doi = {10.48550/arXiv.2510.06200},
archivePrefix = {arXiv},
       eprint = {2510.06200},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv251006200L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

The StarEmbed data set is curated from ZTF observations and the Catalina Surveys Periodic Variable Star Catalog. If you use the StarEmbed data please also cite the works below.

@article{bellm2018zwicky,
  title={The Zwicky Transient Facility: system overview, performance, and first results},
  author={Bellm, Eric C and Kulkarni, Shrinivas R and Graham, Matthew J and Dekany, Richard and Smith, Roger M and Riddle, Reed and Masci, Frank J and Helou, George and Prince, Thomas A and Adams, Scott M and others},
  journal={Publications of the Astronomical Society of the Pacific},
  volume={131},
  number={995},
  pages={018002},
  year={2018},
  publisher={IOP Publishing}
}

@article{drake2014catalina,
  title={The catalina surveys periodic variable star catalog},
  author={Drake, AJ and Graham, MJ and Djorgovski, SG and Catelan, M and Mahabal, AA and Torrealba, G and Garc{\'\i}a-{\'A}lvarez, D and Donalek, C and Prieto, JL and Williams, R and others},
  journal={The Astrophysical Journal Supplement Series},
  volume={213},
  number={1},
  pages={9},
  year={2014},
  publisher={IOP Publishing}
}025}
}