Triple

T9756622
Position Surface form Disambiguated ID Type / Status
Subject Edward Arthur Milne E236568 entity
Predicate knownFor P22 FINISHED
Object Milne–Eddington model in stellar atmospheres E327446 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: Milne–Eddington model in stellar atmospheres | Statement: [Edward Arthur Milne, knownFor, Milne–Eddington model in stellar atmospheres]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07 
Target entity: Milne–Eddington model in stellar atmospheres
Context triple: [Edward Arthur Milne, knownFor, Milne–Eddington model in stellar atmospheres]
  • A. Stellar Atmospheres, A Contribution to the Observational Study of High Temperature in the Reversing Layers of Stars
    "Stellar Atmospheres, A Contribution to the Observational Study of High Temperature in the Reversing Layers of Stars" is the groundbreaking 1925 doctoral thesis in which Cecilia Payne-Gaposchkin demonstrated that stars are composed primarily of hydrogen and helium, fundamentally transforming astrophysics.
  • B. Stellar Atmospheres
    "Stellar Atmospheres" is a landmark astrophysics work that fundamentally advanced understanding of the physical properties and chemical composition of stars.
  • C. Eddington standard model of stars chosen
    The Eddington standard model of stars is a theoretical framework in stellar astrophysics that describes the internal structure and energy transport of stars under simplifying assumptions of radiative equilibrium and constant opacity.
  • D. Numerical models of stellar interiors
    Numerical models of stellar interiors is a seminal astrophysics work by Martin Schwarzschild that developed theoretical and computational methods for understanding the internal structure and evolution of stars.
  • E. An Introduction to the Study of Stellar Structure
    An Introduction to the Study of Stellar Structure is a foundational astrophysics monograph by Subrahmanyan Chandrasekhar that rigorously develops the theory of the internal structure and evolution of stars.
  • 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_69ca84d4eddc8190996fec1417d2bae8 completed March 30, 2026, 2:12 p.m.
NER Named-entity recognition batch_69cd9fb2889481908fba4a449d5007fe completed April 1, 2026, 10:44 p.m.
NED1 Entity disambiguation (via context triple) batch_69d1b02ff0f4819080410d4e7e809a24 completed April 5, 2026, 12:43 a.m.
Created at: March 30, 2026, 8:24 p.m.