Triple
T10454812
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Far Ultraviolet Camera/Spectrograph |
E246523
|
entity |
| Predicate | alsoKnownAs |
P39
|
FINISHED |
| Object | Far-UV Camera/Spectrograph |
E246523
|
NE FINISHED |
How this triple was built (2 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: Far-UV Camera/Spectrograph | Statement: [Far Ultraviolet Camera/Spectrograph, alsoKnownAs, Far-UV Camera/Spectrograph]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Far-UV Camera/Spectrograph Context triple: [Far Ultraviolet Camera/Spectrograph, alsoKnownAs, Far-UV Camera/Spectrograph]
-
A.
Far Ultraviolet Camera/Spectrograph
chosen
The Far Ultraviolet Camera/Spectrograph was a pioneering lunar-based telescope that captured ultraviolet images and spectra of stars, Earth, and the interplanetary medium from the Moon’s surface.
-
B.
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.
-
C.
Ultraviolet Imaging Spectrograph (UVS)
The Ultraviolet Imaging Spectrograph (UVS) is a scientific instrument that observes ultraviolet light to study the composition, structure, and dynamics of Jupiter’s atmosphere and auroras.
-
D.
Ultraviolet and Visual Echelle Spectrograph
The Ultraviolet and Visual Echelle Spectrograph (UVES) is a high-resolution spectrograph mounted on ESO’s Very Large Telescope, used to obtain detailed spectra of astronomical objects in the ultraviolet and visible wavelength ranges.
-
E.
Wide Field Instrument
The Wide Field Instrument is the primary camera and spectrograph on NASA’s Nancy Grace Roman Space Telescope, designed to capture large-area, high-resolution images for studies of dark energy, exoplanets, and infrared astrophysics.
- F. None of above.
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Provenance (3 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_69d381c04fe08190957c26c526a3b05a |
completed | April 6, 2026, 9:49 a.m. |
| NER | Named-entity recognition | batch_69d4fe47fee48190b38ec0466ff0165a |
completed | April 7, 2026, 12:53 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69d87f10b45c81908f1d3128c65750f8 |
completed | April 10, 2026, 4:39 a.m. |
Created at: April 6, 2026, 12:17 p.m.