Triple

T19730187
Position Surface form Disambiguated ID Type / Status
Subject Messier 4 E473829 entity
Predicate locatedInDirectionOf P29992 FINISHED
Object Scorpius tail region — NE NERFINISHED

How this triple was built (3 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: Scorpius tail region | Statement: [Messier 4, locatedInDirectionOf, Scorpius tail region]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07 
Target entity: Scorpius tail region
Context triple: [Messier 4, locatedInDirectionOf, Scorpius tail region]
  • A. Perseus region
    The Perseus region is a prominent star-forming complex in the Perseus arm of the Milky Way, rich in young stars, molecular clouds, and nebulae.
  • B. Chamaeleon star-forming region
    The Chamaeleon star-forming region is a nearby complex of dark molecular clouds rich in young stellar objects and protostars, making it an important site for studying low-mass star formation.
  • C. Sagittarius Star Cloud
    The Sagittarius Star Cloud is a bright, densely populated region of the Milky Way rich in stars and nebulae, prominently visible in the constellation Sagittarius.
  • D. Orion Belt region
    The Orion Belt region is a prominent area of the Orion constellation centered on its three aligned belt stars, rich in young massive stars and active star-forming nebulae.
  • E. Scutum Star Cloud
    The Scutum Star Cloud is a dense, bright region of the Milky Way in the constellation Scutum, rich in stars, clusters, and interstellar material.
  • F. None of above. chosen
  • G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07 
Target entity: Scorpius tail region
Target entity description: The Scorpius tail region is the southern part of the Scorpius constellation, rich in star clusters and nebulae and often observed in deep-sky surveys.
  • A. Perseus region
    The Perseus region is a prominent star-forming complex in the Perseus arm of the Milky Way, rich in young stars, molecular clouds, and nebulae.
  • B. Chamaeleon star-forming region
    The Chamaeleon star-forming region is a nearby complex of dark molecular clouds rich in young stellar objects and protostars, making it an important site for studying low-mass star formation.
  • C. Sagittarius Star Cloud
    The Sagittarius Star Cloud is a bright, densely populated region of the Milky Way rich in stars and nebulae, prominently visible in the constellation Sagittarius.
  • D. Orion Belt region
    The Orion Belt region is a prominent area of the Orion constellation centered on its three aligned belt stars, rich in young massive stars and active star-forming nebulae.
  • E. Scutum Star Cloud
    The Scutum Star Cloud is a dense, bright region of the Milky Way in the constellation Scutum, rich in stars, clusters, and interstellar material.
  • F. None of above. chosen

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_69d8e517ebd48190979ee76723bcfadf completed April 10, 2026, 11:55 a.m.
NER Named-entity recognition batch_69e649fbeaf081909e9356229eaf84dd completed April 20, 2026, 3:45 p.m.
Created at: April 10, 2026, 1:47 p.m.