Triple

T18817638
Position Surface form Disambiguated ID Type / Status
Subject SCUBA E460178 entity
Predicate fullName P16 FINISHED
Object Submillimetre Common-User Bolometer Array 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: Submillimetre Common-User Bolometer Array | Statement: [SCUBA, fullName, Submillimetre Common-User Bolometer Array]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Submillimetre Common-User Bolometer Array
Context triple: [SCUBA, fullName, Submillimetre Common-User Bolometer Array]
  • A. Submillimeter Array
    The Submillimeter Array is a radio interferometer of eight 6-meter telescopes that observes the universe at submillimeter wavelengths, enabling high-resolution studies of cold gas, dust, and star-forming regions in space.
  • B. Heterodyne Instrument for the Far Infrared
    The Heterodyne Instrument for the Far Infrared (HIFI) is a high-resolution spectrometer aboard the Herschel Space Observatory designed to study the chemical composition and physical conditions of interstellar gas and dust in the far-infrared and submillimeter range.
  • C. Caltech Submillimeter Observatory
    The Caltech Submillimeter Observatory was a pioneering radio telescope facility specializing in submillimeter-wavelength astronomy, contributing significantly to the study of cold dust, gas, and star formation in the universe.
  • D. SPT-SZ camera
    The SPT-SZ camera is a millimeter-wave imaging instrument designed to survey the cosmic microwave background and detect galaxy clusters via the Sunyaev–Zel’dovich effect.
  • E. Cooled Mid-Infrared Camera and Spectrometer
    The Cooled Mid-Infrared Camera and Spectrometer (COMICS) is an astronomical instrument designed for high-sensitivity imaging and spectroscopy in the mid-infrared wavelength range, typically used on large ground-based telescopes to study dust, gas, and thermal emission in various celestial objects.
  • 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: Submillimetre Common-User Bolometer Array
Target entity description: Submillimetre Common-User Bolometer Array is a highly sensitive submillimetre-wavelength camera used on the James Clerk Maxwell Telescope to observe cold dust and gas in the universe.
  • A. Submillimeter Array
    The Submillimeter Array is a radio interferometer of eight 6-meter telescopes that observes the universe at submillimeter wavelengths, enabling high-resolution studies of cold gas, dust, and star-forming regions in space.
  • B. Heterodyne Instrument for the Far Infrared
    The Heterodyne Instrument for the Far Infrared (HIFI) is a high-resolution spectrometer aboard the Herschel Space Observatory designed to study the chemical composition and physical conditions of interstellar gas and dust in the far-infrared and submillimeter range.
  • C. Caltech Submillimeter Observatory
    The Caltech Submillimeter Observatory was a pioneering radio telescope facility specializing in submillimeter-wavelength astronomy, contributing significantly to the study of cold dust, gas, and star formation in the universe.
  • D. SPT-SZ camera
    The SPT-SZ camera is a millimeter-wave imaging instrument designed to survey the cosmic microwave background and detect galaxy clusters via the Sunyaev–Zel’dovich effect.
  • E. Cooled Mid-Infrared Camera and Spectrometer
    The Cooled Mid-Infrared Camera and Spectrometer (COMICS) is an astronomical instrument designed for high-sensitivity imaging and spectroscopy in the mid-infrared wavelength range, typically used on large ground-based telescopes to study dust, gas, and thermal emission in various celestial objects.
  • 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_69d8dcf94c288190a06dea029ae4b223 completed April 10, 2026, 11:20 a.m.
NER Named-entity recognition batch_69e5a6b7e75c81909bc65cfc61cbe1c6 completed April 20, 2026, 4:08 a.m.
Created at: April 10, 2026, 11:55 a.m.