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.