Triple

T20479757
Position Surface form Disambiguated ID Type / Status
Subject Whiting 1 E502419 entity
Predicate orbitalAssociation P62451 FINISHED
Object Sagittarius dwarf galaxy debris 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: Sagittarius dwarf galaxy debris | Statement: [Whiting 1, orbitalAssociation, Sagittarius dwarf galaxy debris]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Sagittarius dwarf galaxy debris
Context triple: [Whiting 1, orbitalAssociation, Sagittarius dwarf galaxy debris]
  • A. Canis Major Dwarf Galaxy candidate
    The Canis Major Dwarf Galaxy candidate is a proposed nearby satellite galaxy of the Milky Way, identified as an overdensity of stars in the constellation Canis Major and debated as either a distinct dwarf galaxy or a feature of the Galactic disk.
  • B. Milky Way–Sagittarius dwarf interaction system chosen
    The Milky Way–Sagittarius dwarf interaction system is the ongoing gravitational encounter between our Galaxy and the Sagittarius Dwarf Spheroidal Galaxy, which is being tidally disrupted and absorbed, leaving streams of stars and clusters throughout the Milky Way halo.
  • C. Sagittarius dwarf galaxy globular cluster system
    The Sagittarius dwarf galaxy globular cluster system is a collection of globular star clusters gravitationally bound to and associated with the Sagittarius Dwarf Spheroidal Galaxy, a satellite of the Milky Way.
  • D. Triangulum–Andromeda overdensity
    The Triangulum–Andromeda overdensity is a large, diffuse stellar structure in the outer regions of the Milky Way, thought to be the remnant of a disrupted dwarf galaxy or tidal stream.
  • E. Milky Way dark matter halo
    The Milky Way dark matter halo is the vast, roughly spherical, invisible mass of dark matter surrounding our galaxy that dominates its gravitational potential and governs the motions of its stars, gas, and satellite galaxies.
  • 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_69e0b4af32848190aea80682b44d5d6e completed April 16, 2026, 10:06 a.m.
NER Named-entity recognition batch_69e69b55d7a881909dfe3ea0e74b742b completed April 20, 2026, 9:32 p.m.
Created at: April 16, 2026, 11:34 a.m.