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metadata
license: cc-by-4.0
pretty_name: FUSE Observation Catalog
language:
  - en
description: >-
  The FUSE Observation Catalog indexes every observation obtained by NASA's Far
  Ultraviolet Spectroscopic Explorer (FUSE), which operated from June 24, 1999
  to October 18, 2007. FUSE was uniquely design
task_categories:
  - tabular-classification
tags:
  - space
  - fuse
  - nasa
  - ultraviolet
  - far-uv
  - spectroscopy
  - astronomy
  - telescope
  - open-data
  - tabular-data
  - parquet
size_categories:
  - 1K<n<10K
configs:
  - config_name: default
    data_files:
      - split: train
        path: data/fuse_observations.parquet
    default: true

FUSE Observation Catalog

Representative view of the UV sky — FUSE covered the 905–1187 Å band uniquely

Credit: NASA/GSFC

Part of a dataset collection on Hugging Face.

Dataset description

The FUSE Observation Catalog indexes every observation obtained by NASA's Far Ultraviolet Spectroscopic Explorer (FUSE), which operated from June 24, 1999 to October 18, 2007. FUSE was uniquely designed to observe the hard-to-reach far-UV band between 905 and 1187 Å, where critical absorption lines from H₂, O VI, and deuterium fall — wavelengths inaccessible to Hubble's instruments. Its four coaligned Rowland-circle spectrographs delivered resolving power R ≈ 20,000, the highest ever achieved in space at these wavelengths.

Each row is one FUSE pointing. The archive totals roughly 5,700 observations — modest in count but extraordinarily high-value because of the unique wavelength coverage. FUSE targets include hot white dwarfs (temperature probes via Lyman series), the diffuse interstellar medium (mapping H₂ and O VI in the Milky Way halo), extragalactic quasars (probing the intergalactic medium via absorption), and early-type stars (stellar winds and mass-loss rates).

This dataset is designed for cross-matching with other UV catalogs (IUE, HST, GALEX), identifying FUSE coverage of any sightline of interest, and as a lookup table for retrieving individual spectra from MAST. It complements the HST, IUE, GALEX, JWST, and Chandra observation catalogs in this collection — FUSE fills the 905–1187 Å band that no other mission in that set covers.

The catalog is derived from MAST's CAOM table dbo.caomobservation (collection = 'FUSE'). The archive is static since 2007, so this dataset refreshes quarterly for any late reprocessing or metadata fixes.

This dataset is suitable for tabular classification tasks.

Schema

Column Type Description Sample Null %
obs_id string FUSE observation identifier (11-char alphanumeric, e.g., 'a0010101000'). Primary key. a0010101000 0.0%
obstype string CAOM observation type: 'S' (simple) or 'C' (composite) S 0.0%
intent string Observation intent: 'science' or 'calibration' science 0.0%
proposal_id string FUSE proposal identifier (e.g., 'A001', 'B234'); cycle-letter + sequence A001 11.7%
proposal_pi string Principal Investigator name (free-form) Werner 11.7%
target_name string Target name as provided by the proposer HE0504-2408 0.0%
target_ra float64 Target right ascension in decimal degrees (ICRS) 76.57566700000001 0.0%
target_dec float64 Target declination in decimal degrees (ICRS) -24.067194 0.0%

Quick stats

  • 5,729 FUSE far-UV spectra (1999–2007)
  • 2,807 distinct target names
  • 238 distinct Principal Investigators
  • Unique wavelength coverage: 905–1187 Å (H₂, O VI, deuterium lines)

Usage

from datasets import load_dataset

ds = load_dataset("juliensimon/fuse-observations", split="train")
df = ds.to_pandas()
from datasets import load_dataset

ds = load_dataset("juliensimon/fuse-observations", split="train")
df = ds.to_pandas()

# Top-observed targets
top = df["target_name"].value_counts().head(20)
print(top)

# Sky distribution
import matplotlib.pyplot as plt
plt.figure(figsize=(12, 6))
plt.scatter(df["target_ra"], df["target_dec"], s=1, alpha=0.5)
plt.xlabel("RA (deg)"); plt.ylabel("Dec (deg)")
plt.gca().invert_xaxis()
plt.title("FUSE target pointings (1999–2007)")
plt.show()

Data source

https://archive.stsci.edu/missions-and-data/fuse

Update schedule

Quarterly (1st of Jan/Apr/Jul/Oct at 16:00 UTC) via GitHub Actions.

Related datasets

If you find this dataset useful, please consider giving it a like on Hugging Face. It helps others discover it.

About the author

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

Citation

@dataset{fuse_observations,
  title = {FUSE Observation Catalog},
  author = {Simon, Julien},
  year = {2026},
  url = {https://huggingface.co/datasets/juliensimon/fuse-observations},
  publisher = {Hugging Face},
  note = {Derived from MAST, Space Telescope Science Institute, https://archive.stsci.edu/missions-and-data/fuse}
}

License

CC-BY-4.0