Triple

T12953722
Position Surface form Disambiguated ID Type / Status
Subject EQUULEUS E309956 entity
Predicate payload P12202 FINISHED
Object PHOENIX extreme ultraviolet imager E323693 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: PHOENIX extreme ultraviolet imager | Statement: [EQUULEUS, payload, PHOENIX extreme ultraviolet imager]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07 
Target entity: PHOENIX extreme ultraviolet imager
Context triple: [EQUULEUS, payload, PHOENIX extreme ultraviolet imager]
  • A. Extreme Ultraviolet Imager chosen
    The Extreme Ultraviolet Imager is a solar telescope instrument that captures high-resolution images of the Sun’s outer atmosphere in extreme ultraviolet wavelengths to study its structure and dynamics.
  • B. Far Ultraviolet Camera/Spectrograph
    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.
  • 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. Extreme Ultraviolet Variability Experiment
    The Extreme Ultraviolet Variability Experiment is a solar observation instrument that measures the Sun’s extreme ultraviolet irradiance to study its variability and impact on Earth’s upper atmosphere and space weather.
  • E. Ultraviolet Coronagraph Spectrometer
    The Ultraviolet Coronagraph Spectrometer is a space-based solar observatory instrument designed to study the Sun’s extended corona by measuring its ultraviolet emission and outflowing solar wind.
  • 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_69d7bdfb57a88190836b743e2825feca completed April 9, 2026, 2:55 p.m.
NER Named-entity recognition batch_69d97e1edcdc8190a702c2a5ea58cc67 completed April 10, 2026, 10:47 p.m.
NED1 Entity disambiguation (via context triple) batch_69f6af7a10f48190b7e0d32725f83fb6 completed May 3, 2026, 2:14 a.m.
Created at: April 9, 2026, 5:44 p.m.