Triple

T2126370
Position Surface form Disambiguated ID Type / Status
Subject Schwarzschild–Milne equations E46433 entity
Predicate namedAfter P63 FINISHED
Object Edward Arthur Milne
Edward Arthur Milne was a British astrophysicist and mathematician known for his influential work on stellar structure, radiative transfer, and alternative cosmological models in the early 20th century.
E236568 NE FINISHED

How this triple was built (4 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: Edward Arthur Milne | Statement: [Schwarzschild–Milne equations, namedAfter, Edward Arthur Milne]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Edward Arthur Milne
Context triple: [Schwarzschild–Milne equations, namedAfter, Edward Arthur Milne]
  • A. Arthur Stanley Eddington
    Arthur Stanley Eddington was a pioneering 20th-century British astrophysicist and mathematician known for his work on general relativity, stellar structure, and the 1919 eclipse expedition that confirmed Einstein’s theory of gravity.
  • B. Richard C. Tolman
    Richard C. Tolman was an American physicist and physical chemist known for his contributions to statistical mechanics, thermodynamics, and cosmology, as well as his scientific advisory roles during World War II.
  • C. Henry Norris Russell
    Henry Norris Russell was an influential American astronomer best known for co-developing the Hertzsprung–Russell diagram, a fundamental tool in stellar astrophysics.
  • D. Howard P. Robertson
    Howard P. Robertson was an American mathematician and physicist known for his foundational contributions to relativistic cosmology and the formulation of the Robertson–Walker metric used in modern cosmological models.
  • E. Martin Schwarzschild
    Martin Schwarzschild was a German-American astrophysicist renowned for his pioneering work on stellar structure and evolution, as well as for introducing the use of high-altitude balloon observations in astronomy.
  • F. None of above. chosen
  • G. Unsure - the case is ambiguous/there is not enough information to decide.
NEDg Description generation gpt-5.1
Instruction
Generate a one-sentence description of the target entity. 
You are given a context triple in the form (subject, predicate, object), where the object is the target entity. 
# Instructions
Use the triple to infer relevant information about the entity. Describe the entity based on what is most defining, well-known. 
Avoid repeating the information from the triple, unless really essential.
# Response Format
Return only the sentence: "Description: [one-sentence description of the target entity]"
Input
Entity: Edward Arthur Milne
Triple: [Schwarzschild–Milne equations, namedAfter, Edward Arthur Milne]
Generated description
Edward Arthur Milne was a British astrophysicist and mathematician known for his influential work on stellar structure, radiative transfer, and alternative cosmological models in the early 20th century.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07
Target entity: Edward Arthur Milne
Target entity description: Edward Arthur Milne was a British astrophysicist and mathematician known for his influential work on stellar structure, radiative transfer, and alternative cosmological models in the early 20th century.
  • A. Arthur Stanley Eddington
    Arthur Stanley Eddington was a pioneering 20th-century British astrophysicist and mathematician known for his work on general relativity, stellar structure, and the 1919 eclipse expedition that confirmed Einstein’s theory of gravity.
  • B. Richard C. Tolman
    Richard C. Tolman was an American physicist and physical chemist known for his contributions to statistical mechanics, thermodynamics, and cosmology, as well as his scientific advisory roles during World War II.
  • C. Henry Norris Russell
    Henry Norris Russell was an influential American astronomer best known for co-developing the Hertzsprung–Russell diagram, a fundamental tool in stellar astrophysics.
  • D. Howard P. Robertson
    Howard P. Robertson was an American mathematician and physicist known for his foundational contributions to relativistic cosmology and the formulation of the Robertson–Walker metric used in modern cosmological models.
  • E. Martin Schwarzschild
    Martin Schwarzschild was a German-American astrophysicist renowned for his pioneering work on stellar structure and evolution, as well as for introducing the use of high-altitude balloon observations in astronomy.
  • F. None of above. chosen

Provenance (5 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_69a88a1626548190ae59a5028c3baa8e completed March 4, 2026, 7:37 p.m.
NER Named-entity recognition batch_69abbb59182081908470f9be97e272c8 completed March 7, 2026, 5:44 a.m.
NED1 Entity disambiguation (via context triple) batch_69ae51a0e8ac8190992588bf2bf496ab completed March 9, 2026, 4:50 a.m.
NEDg Description generation batch_69ae521c7810819086b88bb5f062597e completed March 9, 2026, 4:52 a.m.
NED2 Entity disambiguation (via description) batch_69ae52e79c788190bbe6eb5baba08a71 completed March 9, 2026, 4:56 a.m.
Created at: March 4, 2026, 7:44 p.m.