Triple

T518662
Position Surface form Disambiguated ID Type / Status
Subject Eddington–Finkelstein coordinates E10764 entity
Predicate namedAfter P63 FINISHED
Object 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.
E64598 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: Arthur Stanley Eddington | Statement: [Eddington–Finkelstein coordinates, namedAfter, Arthur Stanley Eddington]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Arthur Stanley Eddington
Context triple: [Eddington–Finkelstein coordinates, namedAfter, Arthur Stanley Eddington]
  • A. 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.
  • B. Robert Hanbury Brown
    Robert Hanbury Brown was a British physicist and radio astronomer best known for pioneering intensity interferometry, which led to the Hanbury Brown and Twiss effect and advanced the measurement of stellar diameters.
  • C. Subrahmanyan Chandrasekhar
    Subrahmanyan Chandrasekhar was an Indian-American astrophysicist and Nobel laureate renowned for his work on stellar structure and evolution, particularly the Chandrasekhar limit for white dwarfs.
  • D. 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.
  • E. Lord Rayleigh
    Lord Rayleigh, born John William Strutt, was a British physicist and Nobel laureate renowned for his foundational work in wave theory, optics, and the discovery of argon.
  • 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: Arthur Stanley Eddington
Triple: [Eddington–Finkelstein coordinates, namedAfter, Arthur Stanley Eddington]
Generated description
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.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07
Target entity: Arthur Stanley Eddington
Target entity description: 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.
  • A. 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.
  • B. Robert Hanbury Brown
    Robert Hanbury Brown was a British physicist and radio astronomer best known for pioneering intensity interferometry, which led to the Hanbury Brown and Twiss effect and advanced the measurement of stellar diameters.
  • C. Subrahmanyan Chandrasekhar
    Subrahmanyan Chandrasekhar was an Indian-American astrophysicist and Nobel laureate renowned for his work on stellar structure and evolution, particularly the Chandrasekhar limit for white dwarfs.
  • D. 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.
  • E. Lord Rayleigh
    Lord Rayleigh, born John William Strutt, was a British physicist and Nobel laureate renowned for his foundational work in wave theory, optics, and the discovery of argon.
  • 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_69a2e84a0d08819087e01863fcd9abf1 completed Feb. 28, 2026, 1:06 p.m.
NER Named-entity recognition batch_69a2f19ee6748190916603ef3a9e27f3 completed Feb. 28, 2026, 1:46 p.m.
NED1 Entity disambiguation (via context triple) batch_69a4a42d1a348190abc23d22bda5d9a2 completed March 1, 2026, 8:40 p.m.
NEDg Description generation batch_69a4a4a83cb48190a5d80557c5573ab2 completed March 1, 2026, 8:42 p.m.
NED2 Entity disambiguation (via description) batch_69a4a52e4ae081909f880462479fc51f completed March 1, 2026, 8:44 p.m.
Created at: Feb. 28, 2026, 1:12 p.m.