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Error code: DatasetGenerationError
Exception: ArrowInvalid
Message: Column 0: In chunk 0: Invalid: Struct child array #6 invalid: Invalid: List child array invalid: Invalid: Struct child array #6 has length smaller than expected for struct array (120 < 230)
Traceback: Traceback (most recent call last):
File "/usr/local/lib/python3.12/site-packages/datasets/builder.py", line 1893, in _prepare_split_single
writer.write_table(table)
File "/usr/local/lib/python3.12/site-packages/datasets/arrow_writer.py", line 765, in write_table
self._write_table(pa_table, writer_batch_size=writer_batch_size)
File "/usr/local/lib/python3.12/site-packages/datasets/arrow_writer.py", line 775, in _write_table
pa_table = embed_table_storage(pa_table)
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/usr/local/lib/python3.12/site-packages/datasets/table.py", line 2263, in embed_table_storage
return pa.Table.from_arrays(arrays, schema=features.arrow_schema)
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "pyarrow/table.pxi", line 4912, in pyarrow.lib.Table.from_arrays
File "pyarrow/table.pxi", line 4256, in pyarrow.lib.Table.validate
File "pyarrow/error.pxi", line 92, in pyarrow.lib.check_status
pyarrow.lib.ArrowInvalid: Column 0: In chunk 0: Invalid: Struct child array #6 invalid: Invalid: List child array invalid: Invalid: Struct child array #6 has length smaller than expected for struct array (120 < 230)
The above exception was the direct cause of the following exception:
Traceback (most recent call last):
File "/src/services/worker/src/worker/job_runners/config/parquet_and_info.py", line 1347, in compute_config_parquet_and_info_response
parquet_operations = convert_to_parquet(builder)
^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/src/services/worker/src/worker/job_runners/config/parquet_and_info.py", line 980, in convert_to_parquet
builder.download_and_prepare(
File "/usr/local/lib/python3.12/site-packages/datasets/builder.py", line 884, in download_and_prepare
self._download_and_prepare(
File "/usr/local/lib/python3.12/site-packages/datasets/builder.py", line 947, in _download_and_prepare
self._prepare_split(split_generator, **prepare_split_kwargs)
File "/usr/local/lib/python3.12/site-packages/datasets/builder.py", line 1739, in _prepare_split
for job_id, done, content in self._prepare_split_single(
^^^^^^^^^^^^^^^^^^^^^^^^^^^
File "/usr/local/lib/python3.12/site-packages/datasets/builder.py", line 1925, in _prepare_split_single
raise DatasetGenerationError("An error occurred while generating the dataset") from e
datasets.exceptions.DatasetGenerationError: An error occurred while generating the datasetNeed help to make the dataset viewer work? Make sure to review how to configure the dataset viewer, and open a discussion for direct support.
config dict | difficulty_details unknown | engine string | has_gp_noise bool | hf_split string | instrument_labels list | median_sigma_ms float64 | meta unknown | num_instruments int64 | num_observations int64 | num_planets int64 | observation_span_days float64 | observations dict | rv_range_ms float64 | source_file string | star_mass_solar float64 | subset string | task_family string | task_id string | task_summary string | truth_difficulty int64 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": -33252,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 7
},
{
"gamma_ms": -33166.4198075,
"label": "inst_B",
"sigma_jitter_ms": 0,
"sigma_white_ms": 0.23
},
{
"gamma_ms": 11.... | {
"n_obs": 639,
"real_data": true
} | keplerian | false | train | [
"inst_A",
"inst_B",
"inst_C",
"inst_D",
"inst_E",
"inst_F"
] | 2.52 | {
"gamma_subtracted_per_instrument_ms": {
"inst_A": -33252,
"inst_B": -33166.4198075,
"inst_C": 11.63455714,
"inst_D": 19.675,
"inst_E": -4.98,
"inst_F": 1.79
},
"rv_semantics": "rv_only"
} | 6 | 639 | 1 | 7,237.393404 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 193.145 | real_001.json | 1.11 | real | radial-velocity-planet-detection | real_001 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 1 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 0,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 7
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
"per... | {
"n_obs": 48,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 7 | {
"rv_semantics": "rv_only"
} | 1 | 48 | 2 | 2,571.0101 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 215 | real_002.json | 0.95 | real | radial-velocity-planet-detection | real_002 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 9 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 0,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 1.1
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
"p... | {
"n_obs": 119,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 1.1 | {
"rv_semantics": "rv_only"
} | 1 | 119 | 4 | 1,569.759477 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 39.96 | real_003.json | 0.31 | real | radial-velocity-planet-detection | real_003 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 10 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 0,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 1.97
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
"... | {
"n_obs": 162,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 1.97 | {
"rv_semantics": "rv_only"
} | 1 | 162 | 4 | 4,600.64464 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 599.53 | real_004.json | 0.334 | real | radial-velocity-planet-detection | real_004 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 8 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 0,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 0.525
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
... | {
"n_obs": 190,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 0.525 | {
"rv_semantics": "rv_only"
} | 1 | 190 | 5 | 2,428.194514 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
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"inst_A",
"inst_A",
"inst_A",
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"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 33.53 | real_005.json | 1.06 | real | radial-velocity-planet-detection | real_005 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 6 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 0,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 0.525
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
... | {
"n_obs": 190,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 0.525 | {
"rv_semantics": "rv_only"
} | 1 | 190 | 7 | 2,428.194514 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
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"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 33.53 | real_006.json | 1.06 | real | radial-velocity-planet-detection | real_006 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 10 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 9.55,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 1.4
},
{
"gamma_ms": -8.2,
"label": "inst_B",
"sigma_jitter_ms": 0,
"sigma_white_ms": 5.4
}
],
"integrator_preference": "whfast... | {
"n_obs": 106,
"real_data": true
} | keplerian | false | train | [
"inst_A",
"inst_B"
] | 1.5 | {
"rv_semantics": "rv_only"
} | 2 | 106 | 2 | 3,571.31555 | {
"instruments": [
"inst_B",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_B",
"inst_A",
"inst_A",
"inst_A",
"inst_B",
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"inst_B",
"inst_B",
"inst_B",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 185.5 | real_007.json | 1.07 | real | radial-velocity-planet-detection | real_007 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 4 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 22.15,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 3
},
{
"gamma_ms": -9343.3,
"label": "inst_B",
"sigma_jitter_ms": 0,
"sigma_white_ms": 1.2
},
{
"gamma_ms": 23.7,
... | {
"n_obs": 380,
"real_data": true
} | keplerian | false | train | [
"inst_A",
"inst_B",
"inst_C"
] | 2.65 | {
"rv_semantics": "rv_only"
} | 3 | 380 | 4 | 6,317.5886 | {
"instruments": [
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"... | 9,480.4 | real_008.json | 1.08 | real | radial-velocity-planet-detection | real_008 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 9 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 10.3,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 4.7
},
{
"gamma_ms": -5.2,
"label": "inst_B",
"sigma_jitter_ms": 0,
"sigma_white_ms": 5.3
}
],
"integrator_preference": "whfast... | {
"n_obs": 88,
"real_data": true
} | keplerian | false | train | [
"inst_A",
"inst_B"
] | 5 | {
"rv_semantics": "rv_only"
} | 2 | 88 | 1 | 2,668.840892 | {
"instruments": [
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_A",
"inst_A",
"inst_A",
"... | 250.5 | real_009.json | 1.24 | real | radial-velocity-planet-detection | real_009 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 2 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": -2232,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 3.4
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
... | {
"n_obs": 33,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 3.4 | {
"rv_semantics": "rv_only"
} | 1 | 33 | 1 | 41.9567 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 408.4 | real_010.json | 0.823 | real | radial-velocity-planet-detection | real_010 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 2 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 0,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 0.23
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
"... | {
"n_obs": 187,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 0.23 | {
"rv_semantics": "rv_only"
} | 1 | 187 | 3 | 2,609.9315 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 7.74 | real_011.json | 0.7 | real | radial-velocity-planet-detection | real_011 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 7 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": -9.5,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 3.6
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
... | {
"n_obs": 85,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 3.6 | {
"rv_semantics": "rv_only"
} | 1 | 85 | 1 | 2,029.5777 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 178.8 | real_012.json | 1.148 | real | radial-velocity-planet-detection | real_012 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 1 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 12.85,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 0.89
},
{
"gamma_ms": -0.82,
"label": "inst_B",
"sigma_jitter_ms": 0,
"sigma_white_ms": 0.61
}
],
"integrator_preference": "wh... | {
"n_obs": 373,
"real_data": true
} | keplerian | false | train | [
"inst_A",
"inst_B"
] | 0.66 | {
"rv_semantics": "rv_only"
} | 2 | 373 | 2 | 4,850.806954 | {
"instruments": [
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"... | 28.82 | real_013.json | 0.77 | real | radial-velocity-planet-detection | real_013 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 7 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 11.35,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 1.3
},
{
"gamma_ms": -7.5,
"label": "inst_B",
"sigma_jitter_ms": 0,
"sigma_white_ms": 4.5
}
],
"integrator_preference": "whfas... | {
"n_obs": 207,
"real_data": true
} | keplerian | false | train | [
"inst_A",
"inst_B"
] | 3.9 | {
"rv_semantics": "rv_only"
} | 2 | 207 | 1 | 3,694.004547 | {
"instruments": [
"inst_B",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_B",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 358 | real_014.json | 1.02 | real | radial-velocity-planet-detection | real_014 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 3 |
{
"engine": "keplerian",
"instruments": [
{
"gamma_ms": 0,
"label": "inst_A",
"sigma_jitter_ms": 0,
"sigma_white_ms": 3.1
}
],
"integrator_preference": "whfast",
"los_axis": "x",
"metadata": {},
"noise": {
"gp": {
"Q0": 1,
"dQ": 0.1,
"f": 0.5,
"p... | {
"n_obs": 52,
"real_data": true
} | keplerian | false | train | [
"inst_A"
] | 3.1 | {
"rv_semantics": "rv_only"
} | 1 | 52 | 2 | 3,063.68 | {
"instruments": [
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"inst_A",
"... | 102.72 | real_015.json | 0.85 | real | radial-velocity-planet-detection | real_015 | Infer the planetary system from radial-velocity observations, including planet count and orbital parameters. | 4 |
Dataset Card for Stargazer
Stargazer is a scalable environment for evaluating AI agents on dynamic, iterative physics-grounded model-fitting tasks using inference on radial-velocity (RV) time series data.
- Paper: Stargazer: A Scalable Model-Fitting Benchmark Environment for AI Agents under Astrophysical Constraints
- Project Page: https://aips-uoft.github.io/Stargazer/
- Repository: https://github.com/AIPS-UofT/Stargazer
Overview
Stargazer comprises 120 tasks across three difficulty tiers, including 20 real archival cases, covering diverse scenarios ranging from high-SNR single-planet systems to complex multi-planetary configurations requiring involved low-SNR analysis.
- Total tasks: 120
- License:
cc-by-4.0
This release includes benchmark tasks built from both generated systems and archival RV systems, presented as one benchmark collection. Each row is one benchmark task with the original task payload preserved.
Usage
To run a single task by ID using the official repository:
python run_agent_batch_hard_timeout.py \
--model gpt-5-mini \
--task-ids seed22_diff4 \
--verbose \
--output-dir results_debug
To run all difficulty-1 tasks with 10 parallel workers:
python run_agent_batch_hard_timeout.py \
--model gpt-5-mini \
--count 1000 \
--difficulties 1 \
--workers 10 \
--output-dir results_diff1
What Each Row Contains
Each row keeps the original benchmark structure:
configobservationsdifficulty_detailsmeta
It also adds a few summary fields for filtering in the Hugging Face viewer:
task_idtruth_difficultynum_observationsnum_instrumentsnum_planetsenginehas_gp_noise
Notes
- Tasks in this release may contain up to 7 planets
- This is a benchmark release, not a training corpus
- Ground-truth configuration fields are included, so they should not be exposed to the evaluated agent
Citation
@article{liu2026stargazer,
title = {Stargazer: A Scalable Model-Fitting Benchmark Environment for AI Agents under Astrophysical Constraints},
author = {Liu, Xinge and Zhang, Terry Jingchen and Sch{\"o}lkopf, Bernhard and Jin, Zhijing and Menou, Kristen},
year = {2026},
journal = {arXiv preprint arXiv:2604.15664},
url = {https://arxiv.org/abs/2604.15664}
}
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