Triple

T4080473
Position Surface form Disambiguated ID Type / Status
Subject Very Large Array E87465 entity
Predicate hasUpgrade P5357 FINISHED
Object Expanded Very Large Array project E407183 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: Expanded Very Large Array project | Statement: [Very Large Array, hasUpgrade, Expanded Very Large Array project]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07 
Target entity: Expanded Very Large Array project
Context triple: [Very Large Array, hasUpgrade, Expanded Very Large Array project]
  • A. Expanded Very Large Array chosen
    The Expanded Very Large Array is a major upgrade of the original radio telescope array in New Mexico, featuring enhanced sensitivity, bandwidth, and imaging capabilities for cutting-edge astronomical research.
  • B. Very Long Baseline Array
    The Very Long Baseline Array is a continent-spanning network of ten radio telescopes used for high-resolution astronomical observations through very long baseline interferometry.
  • C. Very Long Baseline Interferometry
    Very Long Baseline Interferometry is a radio astronomy technique that combines signals from widely separated antennas to achieve extremely high angular resolution and precisely measure geodetic and astronomical parameters.
  • D. Very Large Array (VLA) Radio Telescope
    The Very Large Array (VLA) Radio Telescope is a world-renowned radio astronomy observatory in New Mexico, consisting of 27 large dish antennas arranged in a Y-shaped configuration to study distant cosmic phenomena.
  • E. Long Wavelength Array collaboration
    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.
  • 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_69aed9435cf48190ad1da737c962d19d completed March 9, 2026, 2:29 p.m.
NER Named-entity recognition batch_69aefc5204d881909829de15015aa50d completed March 9, 2026, 4:58 p.m.
NED1 Entity disambiguation (via context triple) batch_69b562c0ecb48190b3def058eaf49dd3 completed March 14, 2026, 1:29 p.m.
Created at: March 9, 2026, 3:39 p.m.