Triple

T18956327
Position Surface form Disambiguated ID Type / Status
Subject Vela E463788 entity
Predicate contains P35 FINISHED
Object VelaJuniorSupernovaRemnant NE NERFINISHED

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: VelaJuniorSupernovaRemnant | Statement: [Vela, contains, VelaJuniorSupernovaRemnant]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: VelaJuniorSupernovaRemnant
Context triple: [Vela, contains, VelaJuniorSupernovaRemnant]
  • A. VelaSupernovaRemnant chosen
    VelaSupernovaRemnant is the expansive cloud of gas and dust left behind by a supernova explosion in the Vela constellation, notable for its complex filamentary structure and associated pulsar.
  • B. Tycho's Supernova Remnant
    Tycho's Supernova Remnant is the expanding shell of gas and dust left behind by the Type Ia supernova observed by Tycho Brahe in 1572, located in the constellation Cassiopeia.
  • C. Monoceros Loop supernova remnant
    The Monoceros Loop supernova remnant is a large, faint shell of gas and dust in the constellation Monoceros, believed to be the remains of an ancient supernova explosion.
  • D. supernova remnant 1E 0102.2-7219
    Supernova remnant 1E 0102.2-7219 is a young, oxygen-rich stellar explosion remnant in the Small Magellanic Cloud, notable for its bright X-ray and optical emission and frequent use as a calibration and study target in high-energy astrophysics.
  • E. Cassiopeia A
    Cassiopeia A is a well-studied, relatively young supernova remnant in the constellation Cassiopeia and one of the strongest radio and X-ray sources in the sky.
  • F. None of above.
  • G. Unsure - the case is ambiguous/there is not enough information to decide.

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_69d8dcffc278819086792a4ebfddfafa completed April 10, 2026, 11:20 a.m.
NER Named-entity recognition batch_69e5d5cdf2d08190a0aecd3fa5335a75 completed April 20, 2026, 7:29 a.m.
Created at: April 10, 2026, noon