Triple

T14318644
Position Surface form Disambiguated ID Type / Status
Subject Long Wavelength Array station E355021 entity
Predicate partOf P40 FINISHED
Object Long Wavelength Array project E355023 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: Long Wavelength Array project | Statement: [Long Wavelength Array station, partOf, Long Wavelength Array project]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07 
Target entity: Long Wavelength Array project
Context triple: [Long Wavelength Array station, partOf, Long Wavelength Array project]
  • A. Long Wavelength Array collaboration chosen
    The Long Wavelength Array collaboration is a scientific consortium that operates low-frequency radio telescope arrays to study the universe at meter and decameter wavelengths, including phenomena such as the early universe, cosmic rays, and solar and planetary radio emissions.
  • B. Long Wavelength Array station
    The Long Wavelength Array station is a low-frequency radio astronomy installation used to observe the universe at meter and decameter wavelengths, particularly for studying phenomena like the early universe, the Sun, and transient radio sources.
  • C. Telescope Array Project
    The Telescope Array Project is a large-scale international observatory in Utah designed to detect and study ultra-high-energy cosmic rays entering Earth’s atmosphere.
  • D. Square Kilometre Array project
    The Square Kilometre Array project is an international effort to build the world’s largest and most sensitive radio telescope array, designed to explore fundamental questions about the universe.
  • E. Atacama Compact Array
    The Atacama Compact Array is a subset of smaller, closely spaced radio telescopes within the ALMA observatory designed to improve imaging of extended astronomical objects at millimeter and submillimeter wavelengths.
  • 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_69d8278ed42c8190b9f882dcce611347 completed April 9, 2026, 10:26 p.m.
NER Named-entity recognition batch_69de883a93548190ac671b001d15d0bd completed April 14, 2026, 6:32 p.m.
NED1 Entity disambiguation (via context triple) batch_69fd468a3b788190812ff0eed84fd139 completed May 8, 2026, 2:12 a.m.
Created at: April 10, 2026, 1:13 a.m.