Triple

T18586771
Position Surface form Disambiguated ID Type / Status
Subject High Resolution Spectrometers in Hall A E454254 entity
Predicate hasPart P35 FINISHED
Object Left High Resolution Spectrometer — NE NERFINISHED

How this triple was built (3 steps)

Every LLM step that produced this triple, in pipeline order — named-entity classification, the disambiguation choices (the exact options shown, with the pick highlighted), and the generated description. The batch + timestamp of each is in the Provenance table below.

NER Named-entity recognition gpt-5-mini
Instruction
Given a phrase, classify it is english named entity (e.g., persons, organizations, works of art) in Latin script, or not (e.g., literals, dates, URLs, verbose phrases). For disambiguation, the statement where the phrase occurs as object is also given. Please return a JSON object with `phrase` (string, the phrase being analyzed) and `is_ne` (boolean, indicating whether the phrase is a Named Entity).
Input
Phrase: Left High Resolution Spectrometer | Statement: [High Resolution Spectrometers in Hall A, hasPart, Left High Resolution Spectrometer]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07 
Target entity: Left High Resolution Spectrometer
Context triple: [High Resolution Spectrometers in Hall A, hasPart, Left High Resolution Spectrometer]
  • A. High Resolution Imaging Science Experiment
    The High Resolution Imaging Science Experiment (HiRISE) is a powerful camera aboard NASA's Mars Reconnaissance Orbiter that captures extremely detailed images of the Martian surface for scientific study and mission planning.
  • B. Low Resolution Imaging Spectrometer
    The Low Resolution Imaging Spectrometer (LRIS) is a versatile optical spectrograph and imager mounted on the Keck I telescope, widely used for deep spectroscopic observations in astronomy and cosmology.
  • C. Europa Ultraviolet Spectrograph
    The Europa Ultraviolet Spectrograph is a scientific instrument designed to study Europa’s tenuous atmosphere, surface composition, and space environment by analyzing ultraviolet light during NASA’s Europa Clipper mission.
  • D. International Extreme Ultraviolet Hitchhiker (IEH)
    The International Extreme Ultraviolet Hitchhiker (IEH) was an astronomy payload flown on the Space Shuttle to study celestial sources in the extreme ultraviolet portion of the spectrum.
  • E. Ultraviolet Spectrometer
    The Ultraviolet Spectrometer was a scientific instrument on the Galileo spacecraft used to analyze ultraviolet light from celestial objects to study their composition, atmospheres, and energy processes.
  • F. None of above. chosen
  • G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07 
Target entity: Left High Resolution Spectrometer
Target entity description: The Left High Resolution Spectrometer is one of the precision magnetic spectrometers in Hall A at Jefferson Lab, used to measure the momentum and angles of scattered particles in nuclear and particle physics experiments.
  • A. High Resolution Imaging Science Experiment
    The High Resolution Imaging Science Experiment (HiRISE) is a powerful camera aboard NASA's Mars Reconnaissance Orbiter that captures extremely detailed images of the Martian surface for scientific study and mission planning.
  • B. Low Resolution Imaging Spectrometer
    The Low Resolution Imaging Spectrometer (LRIS) is a versatile optical spectrograph and imager mounted on the Keck I telescope, widely used for deep spectroscopic observations in astronomy and cosmology.
  • C. Europa Ultraviolet Spectrograph
    The Europa Ultraviolet Spectrograph is a scientific instrument designed to study Europa’s tenuous atmosphere, surface composition, and space environment by analyzing ultraviolet light during NASA’s Europa Clipper mission.
  • D. International Extreme Ultraviolet Hitchhiker (IEH)
    The International Extreme Ultraviolet Hitchhiker (IEH) was an astronomy payload flown on the Space Shuttle to study celestial sources in the extreme ultraviolet portion of the spectrum.
  • E. Ultraviolet Spectrometer
    The Ultraviolet Spectrometer was a scientific instrument on the Galileo spacecraft used to analyze ultraviolet light from celestial objects to study their composition, atmospheres, and energy processes.
  • F. None of above. chosen

Provenance (2 batches)

The batch behind each pipeline step, in order, with when it ran. Timestamps are batch-level — stages were processed in waves, so the object chain (NER → NED1 → NEDg → NED2) reads in order, but predicate / elicitation batches can sit in a different wave.

Step Stage Batch ID Status When
creating Elicitation batch_69d8d38ae7e081908a98df1251842402 completed April 10, 2026, 10:40 a.m.
NER Named-entity recognition batch_69e545b210488190ba62d3bf6e1a595c completed April 19, 2026, 9:14 p.m.
Created at: April 10, 2026, 11:44 a.m.