Datasets:
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README.md
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The StarEmbed benchmark data set is available here in huggingface datasets format.
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The ~40,000 multi-band ZTF light
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The train/validation/test splits are included alongside the additional anom split used for the OOD benchmarking.
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## Available columns
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Each star in data set has the following fields:
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**Top-level columns**
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| Column
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| ------------
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| `sourceid`
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| `bands_data`
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| `objid` | string | object identifier, same as `item_id` (`{sourceid}_{band}`) |
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| `csdr1_id` | string | Catalina Surveys DR1 (CSDR1) cross-match id, e.g. `CSS_J082956.4-044426` |
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| `class_str` | string | variable-star class label; one of `EW`, `EA`, `RRab`, `RRc`, `RRd`, `RS CVn`, `LPV` |
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**Per-band fields inside each band of `bands_data` (`g` / `r`)**
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| Field | Type | Description |
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| ------------------------ | -------------- | ------------------------------------------------------------------- |
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| `target` | list of floats | magnitude, measure of brightness (AB system) — the raw light curve |
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| `mjd` | list of floats | observation time in Modified Julian Date, aligned with `target` |
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| `length` | int64 | number of observations in this band's light curve |
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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
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---
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The StarEmbed benchmark data set is available here in huggingface datasets format.
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The ~40,000 multi-band ZTF light curves are available at `StarEmbed/data`.
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The train/validation/test splits are included alongside the additional anom split used for the OOD benchmarking.
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## Available columns
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Each star in data set has the following fields:
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**Top-level columns**
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| Column | Type | Description |
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| ------------ | ---------------------------------- | -------------------------------------------------------------------------------------------------------- |
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| `sourceid` | string | Catalina Surveys DR1 (CSDR1) source id of the variable star (e.g. `CSS_J082956.4-044426`) |
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| `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.|
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| `period` | float64 | catalog period of the variable star, in days (range ≈ 0.13 – 885) |
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| `class_str` | string | variable-star class label; one of `EW`, `EA`, `RRab`, `RRc`, `RRd`, `RS CVn`, `LPV` |
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| `ra` | float64 | right ascension (J2000) in decimal degrees |
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| `dec` | float64 | declination (J2000) in decimal degrees |
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**Per-band fields inside each band of `bands_data` (`g` / `r` / `i`)**
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| Field | Type | Description |
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| ------------------------ | -------------- | ------------------------------------------------------------------- |
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| `target` | list of floats | magnitude, measure of brightness (AB system) — the raw light curve |
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| `mjd` | list of floats | observation time in Modified Julian Date, aligned with `target` |
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| `length` | int64 | number of observations in this band's light curve |
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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.
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