Docs: state stored units of inputs.csv columns; sync card, Croissant and version.json
Browse files- README.md +20 -16
- croissant.json +103 -4
- version.json +2 -2
README.md
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@@ -79,7 +79,9 @@ The release includes:
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- `archives/dataset.tar.gz`: the ThousandWorlds dataset.
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- `archives/results-baselines-*.tar.gz`: baseline predictions for the 3
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subsets.
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- `croissant.json`: Croissant metadata
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- `archives/*.sha256`: checksum sidecars.
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## Dataset Contents
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includes `is_target_gcm`, `in_target_physical_domain`, `planet_id`, and
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`source`.
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## Outputs
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The package includes loaders and metrics for two benchmark protocols:
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- **Standard**: the main test protocol.
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- **Shared-planets**: evaluate on planets
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a model gets to the epistemic uncertainty floor of the problem.
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Headline baselines are `train_mean`, `knn`, `pca_gbt`, `coord_mlp`, `coord_deeponet`, `pca_mlp`, `conv_decoder`, `sfno`, `ppca_icm`, and `gplfr`. PCA-Ridge (`pca_ridge`) is the nonlinearity ablation. The baseline archives include predictions,
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the config each run used, and metrics JSON files.
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## Versions
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v2.0.0 replaces v1.0.0. It is a small update to the dataset to fix a couple
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bugs in some simulations and add a few more; the full list is in
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[changelog](https://github.com/edstevenson/ThousandWorlds/blob/main/CHANGELOG.md).
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v1.0.0 remains available for reproducing earlier work.
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- `archives/dataset.tar.gz`: the ThousandWorlds dataset.
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- `archives/results-baselines-*.tar.gz`: baseline predictions for the 3
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subsets.
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- [`croissant.json`](croissant.json): full-dataset Croissant metadata, including
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Responsible AI fields and provenance links. Use this custom file for the full
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benchmark; Hugging Face's automatic Croissant export covers only the input table.
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- `archives/*.sha256`: checksum sidecars.
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## Dataset Contents
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includes `is_target_gcm`, `in_target_physical_domain`, `planet_id`, and
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`source`.
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`inputs.csv` stores radius in metres, surface pressure in pascals, and CO2 and
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CH4 as volume fractions between 0 and 1.
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| Parameter | Range | Column in `inputs.csv` (stored unit) |
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| --- | --- | --- |
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| Radius (Earth radii) | [0.7, 1.75] | `radius` (m) |
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| Surface gravity (m s^-2) | [6.0, 17.0] | `gravity` (m s^-2) |
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| Rotation period (days) | [1.0, 200.0] | `rotation_period` (days) |
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| Surface pressure (bar) | [0.5, 5] | `surface_pressure` (Pa) |
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| CO2 volume fraction (%) | [0, 100] | `co2` (volume fraction, 0–1) |
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| CH4 volume fraction (%) | [0, 5] | `ch4` (volume fraction, 0–1) |
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| Incident stellar flux (W m^-2) | [500, 1500] | `stellar_flux` (W m^-2) |
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| Stellar temperature (K) | [2500, 5800] | `stellar_temperature` (K) |
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## Outputs
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The package includes loaders and metrics for two benchmark protocols:
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- **Standard**: the main test protocol.
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- **Shared-planets**: evaluate on planets simulated by both target GCMs
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(UM and ExoCAM), reporting emulator scores relative to inter-GCM disagreement.
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Headline baselines are `train_mean`, `knn`, `pca_gbt`, `coord_mlp`, `coord_deeponet`, `pca_mlp`, `conv_decoder`, `sfno`, `ppca_icm`, and `gplfr`. PCA-Ridge (`pca_ridge`) is the nonlinearity ablation. The baseline archives include predictions,
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the config each run used, and metrics JSON files.
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## Versions
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v2.0.0 replaces v1.0.0. It is a small update to the dataset to fix a couple
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+
bugs in some simulations and add a few more simulations; the full list is in
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the [changelog](https://github.com/edstevenson/ThousandWorlds/blob/main/CHANGELOG.md).
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v1.0.0 remains available for reproducing earlier work.
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croissant.json
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},
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"parentField": "cr:parentField",
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"path": "cr:path",
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"rai": "http://mlcommons.org/croissant/RAI/",
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"recordSet": "cr:recordSet",
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"references": "cr:references",
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],
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"description": "Baseline prediction NPZ files inside the baseline result archives.",
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"encodingFormat": "application/x-numpy",
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"includes": "results/models/
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"name": "results/models/
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},
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{
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"@id": "baseline-metadata",
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],
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"license": "https://creativecommons.org/licenses/by/4.0/",
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"name": "ThousandWorlds",
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"rai:dataBiases": "The dataset reflects simulator, parameter-design, and preprocessing choices: ExoCAM and UM are target GCMs, auxiliary simulations are not uniformly represented across all benchmark subsets, and model behavior can depend on the released variable coverage and missing-field patterns.",
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"rai:dataLimitations": "ThousandWorlds is a benchmark built from numerical exoplanet climate simulations, not observed planets. It is restricted to the released target physical domain, GCM choices, variables, spatial grid, temporal sampling, and benchmark split definitions, and should not be used as direct evidence for habitability, mission planning, or validated climate prediction outside those regimes.",
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"rai:dataSocialImpact": "Potential benefits include reproducible comparison of climate-emulation methods and broader access to expensive simulation-derived benchmark data. Main risks are overinterpreting benchmark scores or synthetic simulation outputs as observational truth; mitigations include explicit split definitions, public baseline artifacts, documented limitations, and open release metadata.",
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"@id": "inputs/co2",
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"@type": "cr:Field",
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"dataType": "sc:Float",
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"description": "Atmospheric CO2
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"name": "co2",
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"source": {
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"extract": {
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"@id": "inputs/ch4",
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"@type": "cr:Field",
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"dataType": "sc:Float",
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"description": "Atmospheric CH4
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"name": "ch4",
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"source": {
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"extract": {
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},
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"parentField": "cr:parentField",
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"path": "cr:path",
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"prov": "http://www.w3.org/ns/prov#",
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"rai": "http://mlcommons.org/croissant/RAI/",
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"recordSet": "cr:recordSet",
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"references": "cr:references",
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],
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"description": "Baseline prediction NPZ files inside the baseline result archives.",
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"encodingFormat": "application/x-numpy",
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"includes": "results/models/*/*/predictions*.npz",
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"name": "results/models/*/*/predictions*.npz"
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},
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{
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"@id": "baseline-metadata",
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],
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"license": "https://creativecommons.org/licenses/by/4.0/",
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"name": "ThousandWorlds",
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"prov:wasDerivedFrom": [
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{
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"@type": "prov:Entity",
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"name": "Mak et al. [2024]",
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"url": "https://doi.org/10.1093/mnras/stae741"
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},
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{
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"@type": "prov:Entity",
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"name": "Sergeev et al. [2022]",
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"url": "https://doi.org/10.3847/PSJ/ac6cf2"
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},
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{
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"@type": "prov:Entity",
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"name": "Hammond et al. [2025]",
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"url": "https://doi.org/10.3847/1538-4357/adc73b"
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},
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{
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"@type": "prov:Entity",
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"name": "Haqq-Misra et al. [2022]",
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"url": "https://doi.org/10.3847/PSJ/ac9479"
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},
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{
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"@type": "prov:Entity",
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"name": "Wolf et al. [2025]",
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"url": "https://doi.org/10.3847/PSJ/ae031e"
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},
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{
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"@type": "prov:Entity",
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"name": "Komacek and Abbot [2019]",
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"url": "https://doi.org/10.3847/1538-4357/aafb33"
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},
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{
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"@type": "prov:Entity",
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"name": "kumar Kopparapu et al. [2016]",
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"url": "https://doi.org/10.3847/0004-637X/819/1/84"
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},
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{
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"@type": "prov:Entity",
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"name": "kumar Kopparapu et al. [2017]",
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"url": "https://doi.org/10.3847/1538-4357/aa7cf9"
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},
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{
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"@type": "prov:Entity",
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"name": "Wolf et al. [2019]",
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"url": "https://doi.org/10.3847/1538-4357/ab184a"
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},
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{
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"@type": "prov:Entity",
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"name": "Wolf [2017]",
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"url": "https://doi.org/10.3847/2041-8213/aa693a"
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},
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{
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"@type": "prov:Entity",
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"name": "Suissa et al. [2020]",
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"url": "https://doi.org/10.3847/1538-3881/aba4b4"
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},
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{
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"@type": "prov:Entity",
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"name": "Macdonald et al. [2025]",
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"url": "https://doi.org/10.3847/1538-4357/adb0cb"
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},
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{
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"@type": "prov:Entity",
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"name": "Paradise et al. [2021]",
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"url": "https://doi.org/10.1016/j.icarus.2020.114301"
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},
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{
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"@type": "prov:Entity",
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"name": "Paradise et al. [2022a]",
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"url": "https://doi.org/10.1093/mnras/stac172"
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},
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{
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"@type": "prov:Entity",
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"name": "Paradise et al. [2022b]",
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"url": "https://doi.org/10.1093/mnras/stac724"
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},
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{
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"@type": "prov:Entity",
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"name": "Woodward et al. [in preparation]",
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"url": "https://arxiv.org/abs/2606.18338"
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},
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{
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"@type": "prov:Entity",
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"name": "this work",
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"url": "https://arxiv.org/abs/2606.18338"
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}
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],
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"prov:wasGeneratedBy": {
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"@type": "prov:Activity",
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"description": "Time-averaged outputs from ExoCAM, ExoCAM-pre-2022, UM, LFRic, and ExoPlaSim were collected from the cited studies and unpublished contributions, alongside 424 bespoke simulations selected using a weighted space-filling design. Source entities match the source labels in inputs.csv; their URLs document the underlying simulation collections, rather than claiming separate raw-data archives. The ThousandWorlds paper documents the bespoke and in-preparation contributions. Fields were regridded to a 32 x 64 horizontal grid and ten relative pressure levels, symmetrized about the equator (antisymmetrized for north-south wind), and fields with partial spatial coverage were marked wholly unobserved. T21 spherical-harmonic coefficients and predefined train/test splits were exported, with planets kept together across GCMs to prevent leakage. The paper describes the simulation settings and processing; the dataset documentation describes the released files; the code defines model-input/output transforms; the changelog records v2.0.0 corrections.",
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"name": "ThousandWorlds simulation collection and benchmark construction",
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"url": [
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"https://arxiv.org/abs/2606.18338",
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"https://github.com/astroautomata/ThousandWorlds/blob/main/dataset/README.md",
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"https://github.com/astroautomata/ThousandWorlds/blob/main/thousandworlds/preprocessing.py",
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"https://github.com/astroautomata/ThousandWorlds/blob/main/CHANGELOG.md"
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]
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},
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"rai:dataBiases": "The dataset reflects simulator, parameter-design, and preprocessing choices: ExoCAM and UM are target GCMs, auxiliary simulations are not uniformly represented across all benchmark subsets, and model behavior can depend on the released variable coverage and missing-field patterns.",
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| 482 |
"rai:dataLimitations": "ThousandWorlds is a benchmark built from numerical exoplanet climate simulations, not observed planets. It is restricted to the released target physical domain, GCM choices, variables, spatial grid, temporal sampling, and benchmark split definitions, and should not be used as direct evidence for habitability, mission planning, or validated climate prediction outside those regimes.",
|
| 483 |
"rai:dataSocialImpact": "Potential benefits include reproducible comparison of climate-emulation methods and broader access to expensive simulation-derived benchmark data. Main risks are overinterpreting benchmark scores or synthetic simulation outputs as observational truth; mitigations include explicit split definitions, public baseline artifacts, documented limitations, and open release metadata.",
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"@id": "inputs/co2",
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"@type": "cr:Field",
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"dataType": "sc:Float",
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"description": "Atmospheric CO2 volume fraction (0 to 1) used by the simulation.",
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"name": "co2",
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"source": {
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"extract": {
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"@id": "inputs/ch4",
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"@type": "cr:Field",
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"dataType": "sc:Float",
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"description": "Atmospheric CH4 volume fraction (0 to 1) used by the simulation.",
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"name": "ch4",
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"source": {
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"extract": {
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version.json
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"name": "ThousandWorlds",
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"release_status": "released",
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"source_files": {
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-
"README.md": "
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-
"croissant.json": "
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"imgs/MASCOT.png": "6060a16f7361686d29b7b7998544a4edbb41ee853ccc3eacf84964e7639c0ed8",
|
| 88 |
"imgs/OVERVIEW.png": "223d32ead45379fe1a422a26aa805b28857b803d85643e021e1b67dec6f797ab",
|
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"inputs.csv": "31f355893974960f8d25a27d5a02bb1a70886387360a86b8880ea567eb11de95"
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|
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"name": "ThousandWorlds",
|
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"release_status": "released",
|
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"source_files": {
|
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+
"README.md": "5b105026d2531961c8cb94178fe3369c50023e979bcabdb914011e62d6bbf6a3",
|
| 86 |
+
"croissant.json": "a3fb549c702896707cec6f9957c54ec0e16f517cc8d28600a3ad1ae1a3288b87",
|
| 87 |
"imgs/MASCOT.png": "6060a16f7361686d29b7b7998544a4edbb41ee853ccc3eacf84964e7639c0ed8",
|
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"imgs/OVERVIEW.png": "223d32ead45379fe1a422a26aa805b28857b803d85643e021e1b67dec6f797ab",
|
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"inputs.csv": "31f355893974960f8d25a27d5a02bb1a70886387360a86b8880ea567eb11de95"
|