Datasets:
Update X-ray binary catalog: 305 sources
Browse files- README.md +200 -0
- data/xray-binaries.parquet +3 -0
README.md
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| 1 |
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---
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| 2 |
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license: cc-by-4.0
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pretty_name: "X-ray Binary Catalog"
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language:
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- en
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description: "Merged catalog of high-mass and low-mass X-ray binaries from HEASARC (Liu et al. 2006/2007)"
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task_categories:
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- tabular-classification
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tags:
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- space
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- x-ray-binary
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- hmxb
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- lmxb
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- x-ray
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- astronomy
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- compact-object
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- neutron-star
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- black-hole
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- open-data
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- tabular-data
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- parquet
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size_categories:
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- n<1K
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configs:
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- config_name: default
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data_files:
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- split: train
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path: data/xray-binaries.parquet
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default: true
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---
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# X-ray Binary Catalog
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*Part of the [Astronomy Datasets](https://huggingface.co/collections/juliensimon/astronomy-datasets-69c24caf2f17e36128946743) and [Stellar Catalogs](https://huggingface.co/collections/juliensimon/stellar-catalogs-69c24caf2f17e36128946744) collections on Hugging Face.*
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Merged catalog of **305** X-ray binaries (116 high-mass, 189 low-mass) from NASA HEASARC,
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combining the HMXB catalog (Liu, van Paradijs & van den Heuvel 2006) and the LMXB catalog (Liu, van Paradijs & van den Heuvel 2007).
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## Dataset description
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X-ray binaries are stellar systems in which a compact object (neutron star or black hole) accretes matter from a
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companion star, producing intense X-ray emission. They are divided into two classes based on the mass of the donor star:
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- **High-Mass X-ray Binaries (HMXBs)**: The donor is a massive O or B star (typically >10 solar masses). Accretion
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occurs via stellar wind or Roche lobe overflow. HMXBs are found in star-forming regions and include Be/X-ray
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binaries (the largest subclass) and supergiant X-ray binaries.
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- **Low-Mass X-ray Binaries (LMXBs)**: The donor is a low-mass star (typically <1 solar mass). Accretion proceeds
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through Roche lobe overflow, forming a bright accretion disk. LMXBs are concentrated toward the Galactic center
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and globular clusters. They include the Z and Atoll sources (classified by their X-ray color-color diagrams) and
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the soft X-ray transients.
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X-ray binaries are natural laboratories for studying accretion physics, strong gravity, and the equation of state of
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ultra-dense matter. Their X-ray variability (pulsations, quasi-periodic oscillations, thermonuclear bursts) encodes
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information about the compact object's mass, spin, and magnetic field. Several black hole mass measurements come from
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dynamical studies of X-ray binary orbits.
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This dataset merges the two standard reference catalogs maintained at HEASARC, providing a unified view of the known
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Galactic X-ray binary population with positions, X-ray fluxes, orbital periods, and companion star classifications.
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## Schema
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| Column | Type |
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|--------|------|
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| `__row` | string |
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| `name` | string |
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| `xray_type` | string |
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| `ra` | float |
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| `dec` | float |
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| `lii` | string |
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| `bii` | string |
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| `position_type` | string |
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| `optical_name` | string |
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| `ref_optical` | string |
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| `vmag_limit` | string |
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| `vmag` | string |
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| `vmag_min` | string |
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| `vmag_flag` | string |
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| `bv_color` | string |
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| `bv_color_flag` | string |
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| `bv_color_max` | string |
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| `ub_color` | string |
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| `reddening` | string |
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| `reddening_max` | string |
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| `reddening_flag` | string |
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| `ref_photometry` | string |
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| `jmag` | string |
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| `hmag_limit` | string |
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| `hmag` | string |
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| `kmag_limit` | string |
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| `kmag` | string |
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| `fx_limit` | string |
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| `fx` | string |
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| `fx_max` | string |
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| `fx_range` | string |
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| `ref_fx` | string |
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| `porb` | string |
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| `porb_flag` | string |
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| `pulse_per` | string |
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| `pulse_per_flag` | string |
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| `ref_periods` | string |
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| `spect_type` | string |
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| `alt_name_1` | string |
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| `alt_name_1_flag` | string |
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| `alt_name_2` | string |
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| `alt_name_3` | string |
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| `class` | string |
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| `__x_ra_dec` | string |
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| `__y_ra_dec` | string |
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| `__z_ra_dec` | string |
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| `binary_type` | string |
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| `ref_optical_name` | string |
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| `reddening_limit` | string |
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| `flux_limit` | string |
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| `flux` | float |
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| `flux_max` | string |
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| `flux_range` | string |
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| `ref_flux` | string |
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| `pulse_period` | string |
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| `lmxb_notes` | string |
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## Quick stats
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- **305** X-ray binaries total
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- **116** High-Mass X-ray Binaries (HMXB)
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- **189** Low-Mass X-ray Binaries (LMXB)
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## Usage
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```python
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from datasets import load_dataset
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ds = load_dataset("juliensimon/xray-binary-catalog", split="train")
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df = ds.to_pandas()
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# Count by type
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print(df["binary_type"].value_counts())
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# HMXBs vs LMXBs
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hmxb = df[df["binary_type"] == "HMXB"]
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lmxb = df[df["binary_type"] == "LMXB"]
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print(f"{len(hmxb):,} HMXBs, {len(lmxb):,} LMXBs")
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# Sky distribution
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import matplotlib.pyplot as plt
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fig, ax = plt.subplots(figsize=(12, 6))
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for btype, group in df.groupby("binary_type"):
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ax.scatter(group["ra"], group["dec"], s=5, alpha=0.7, label=btype)
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ax.set_xlabel("RA (deg)")
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ax.set_ylabel("Dec (deg)")
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ax.legend()
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ax.set_title("X-ray Binary Sky Distribution")
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```
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## Data source
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All data comes from the HEASARC X-ray binary catalogs:
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- [HMXB Catalog (hmxbcat)](https://heasarc.gsfc.nasa.gov/W3Browse/all/hmxbcat.html) — Liu, van Paradijs & van den Heuvel (2006)
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- [LMXB Catalog (lmxbcat)](https://heasarc.gsfc.nasa.gov/W3Browse/all/lmxbcat.html) — Liu, van Paradijs & van den Heuvel (2007)
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Accessed via the HEASARC TAP protocol.
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## Update schedule
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Quarterly (February, May, August, November 1st at 08:00 UTC) via [GitHub Actions](https://github.com/juliensimon/space-datasets).
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## Related datasets
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- [pulsar-catalog](https://huggingface.co/datasets/juliensimon/pulsar-catalog) — ATNF Pulsar Catalog
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| 173 |
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- [mcgill-magnetar-catalog](https://huggingface.co/datasets/juliensimon/mcgill-magnetar-catalog) — McGill Magnetar Catalog
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- [chandra-x-ray-sources](https://huggingface.co/datasets/juliensimon/chandra-x-ray-sources) — Chandra Source Catalog
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| 175 |
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- [gravitational-wave-events](https://huggingface.co/datasets/juliensimon/gravitational-wave-events) — LIGO/Virgo GW Events
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## Pipeline
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Source code: [juliensimon/space-datasets](https://github.com/juliensimon/space-datasets)
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## Support
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If you find this dataset useful, please give it a heart on the [dataset page](https://huggingface.co/datasets/juliensimon/xray-binary-catalog) and share feedback in the Community tab! Also consider giving a star to the [space-datasets](https://github.com/juliensimon/space-datasets) repo.
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## Citation
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```bibtex
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@dataset{xray_binary_catalog,
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author = {Simon, Julien},
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title = {X-ray Binary Catalog},
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year = {2026},
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publisher = {Hugging Face},
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url = {https://huggingface.co/datasets/juliensimon/xray-binary-catalog},
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note = {Based on HEASARC HMXB (Liu et al. 2006) and LMXB (Liu et al. 2007) catalogs}
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}
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```
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## License
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| 199 |
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[CC-BY-4.0](https://creativecommons.org/licenses/by/4.0/)
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data/xray-binaries.parquet
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version https://git-lfs.github.com/spec/v1
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oid sha256:8cbcd45a224801745507fabe1e8370587f45ddee3a2e744e4fd6f9870201f715
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size 90505
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