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juliensimon/hot-subdwarf-stars

Hot Subdwarf Star Catalog Credit: NASA/ESA/Hubble Part of a dataset collection on Hugging Face. Dataset description The Catalogue of Hot Subdwarf Stars (Kilkenny, Heber & Drilling 1988), retrieved from VizieR III/137. The compendium remains the historical reference for the population of spectroscopically identified subdwarf B (sdB) and subdwarf O (sdO) stars — evolved low-mass stars that occupy the extreme horizontal branch of the Hertzsprung-Russell… See the full description on the dataset page: https://huggingface.co/datasets/juliensimon/hot-subdwarf-stars.

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Dataset Card

Hot Subdwarf Star Catalog

<div align="center"> <img src="banner.jpg" alt="A youthful globular star cluster observed by the Hubble Space Telescope" width="400"> <p><em>Credit: NASA/ESA/Hubble</em></p> </div>

Part of a [dataset collection](https://huggingface.co/collections/juliensimon/stellar-catalogs-69c792b1a52ab2757b0eaa57) on Hugging Face.

Dataset description

The Catalogue of Hot Subdwarf Stars (Kilkenny, Heber & Drilling 1988), retrieved from VizieR III/137. The compendium remains the historical reference for the population of spectroscopically identified subdwarf B (sdB) and subdwarf O (sdO) stars — evolved low-mass stars that occupy the extreme horizontal branch of the Hertzsprung-Russell diagram.

Hot subdwarfs are believed to be the bare helium-burning cores of red giants that lost almost all of their hydrogen envelopes near the tip of the giant branch. The dominant formation channel is binary interaction (Roche-lobe overflow or common-envelope ejection), making sdB stars a key laboratory for testing binary stellar evolution theory and the origin of single hot subdwarfs via mergers. They are also major contributors to the ultraviolet excess (UV upturn) observed in elliptical galaxies. Each entry in this catalog records the J2000 sky position, primary designation, V-band photometry, color indices, spectral classification, and the atmospheric parameters effective temperature and surface gravity (log g) when available.

This dataset complements juliensimon/gaia-dr3-white-dwarfs (the post-AGB end-state into which some hot subdwarfs evolve), juliensimon/cataclysmic-variable-catalog and juliensimon/xray-binary-catalog (compact binary systems formed by similar evolutionary pathways), and juliensimon/brown-dwarf-catalog and juliensimon/cns5-nearby-stars for broader stellar-population context.

This dataset is suitable for tabular classification tasks.

Schema

ColumnTypeDescriptionSampleNull %
catalog_numberint64Sequence number in the Kilkenny-Heber-Drilling catalog; entries 1-N are listed in spectral-type order20.0%
rafloat64Right ascension (degrees, J2000, 0-360)44.644958333333330.0%
decfloat64Declination (degrees, J2000, -90 to +90)3.1812222222222220.0%
namestrPrimary star designation (e.g. 'PB 6958', 'PG 0044+097', 'EC 11481-2303'); compiled from the discovery surveyPB 69580.0%
v_magnitude_referencestrBibliographic reference code for the V-band photometry7563.7%
v_magnitudefloat64Apparent V-band magnitude (Johnson V); brighter sources have smaller values15.0863.6%
color_index_1float64Color index 1 (U-B or B-V depending on photometric system; Johnson UBV by default)-0.1564.2%
color_index_2float64Color index 2 (typically B-V or Stromgren b-y)-1.1464.2%
color_index_3float64Color index 3 (third photometric color, system-dependent)-0.0887.6%
spectral_typestrSpectral classification (e.g. 'sdB', 'sdO', 'sdB+F'); 'sd' denotes subdwarf; the secondary letter (B or O) marks the underlying spectral class; '+X' suffix indicates a composite spectrum with cool companion of type XsdB15.2%
spectral_type_referencestrBibliographic reference code for the spectral classification7515.4%
effective_temperature_kfloat64Effective temperature (Kelvin); sdB stars cluster around 25,000-35,000 K, sdO stars at 40,000-80,000 K4.7490.0%
log_gfloat64Logarithm (base 10) of surface gravity in cgs units (cm/s^2); hot subdwarfs occupy log_g = 5-6, intermediate between main-sequence (4-5) and white dwarfs (7-9)4.092.9%
log_g_referencestrBibliographic reference code for the log_g determination7690.0%

Quick stats

  • —1,714 spectroscopically identified hot subdwarf stars
  • —770 sdB-type + 470 sdO-type entries
  • —22 composite-spectrum binaries (e.g. sdB+F, sdO+K)
  • —Effective temperatures span 3 to 5 K
  • —Surface gravities (log g) cluster between 3.30 and 7.00 cgs

Usage

python
from datasets import load_dataset

ds = load_dataset("juliensimon/hot-subdwarf-stars", split="train")
df = ds.to_pandas()
python
from datasets import load_dataset
import matplotlib.pyplot as plt

df = load_dataset("juliensimon/hot-subdwarf-stars", split="train").to_pandas()

# Kiel diagram (Teff vs log g) — the standard plane for hot subdwarf analysis
mask = df["effective_temperature_k"].notna() & df["log_g"].notna()
fig, ax = plt.subplots(figsize=(8, 6))
ax.scatter(df.loc[mask, "effective_temperature_k"], df.loc[mask, "log_g"],
           c=df.loc[mask, "v_magnitude"], s=30, cmap="viridis_r")
ax.invert_xaxis()  # hot on the left
ax.invert_yaxis()  # large gravity on the bottom
ax.set_xscale("log")
ax.set_xlabel("Effective temperature (K)")
ax.set_ylabel("log g (cgs)")
ax.set_title("Kiel diagram of hot subdwarfs — sdB cluster vs sdO tail")
plt.tight_layout()
plt.show()

# Spectral-type breakdown
print(df["spectral_type"].value_counts().head(20))

Data source

https://cdsarc.cds.unistra.fr/viz-bin/cat/III/137

Related datasets

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About the author

Created by Julien Simon — AI Operating Partner at Fortino Capital. Part of the Space Datasets collection.

Citation

bibtex
@dataset{hot_subdwarf_stars,
  title = {Hot Subdwarf Star Catalog},
  author = {Simon, Julien},
  year = {2026},
  url = {https://huggingface.co/datasets/juliensimon/hot-subdwarf-stars},
  publisher = {Hugging Face},
  note = {Derived from CDS Archive, Centre de Données astronomiques de Strasbourg, https://cdsarc.cds.unistra.fr/viz-bin/cat/III/137}
}

License

VizieR Scientific-Use Terms