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.