Datasets:
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}
}