Triple
T23120733
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Stellar Atmospheres, A Contribution to the Observational Study of High Temperature in the Reversing Layers of Stars |
E576883
|
entity |
| Predicate | titleShort |
P6037
|
FINISHED |
| Object | Stellar Atmospheres |
—
|
NE NERFINISHED |
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: Stellar Atmospheres | Statement: [Stellar Atmospheres, A Contribution to the Observational Study of High Temperature in the Reversing Layers of Stars, titleShort, Stellar Atmospheres]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Stellar Atmospheres Context triple: [Stellar Atmospheres, A Contribution to the Observational Study of High Temperature in the Reversing Layers of Stars, titleShort, Stellar Atmospheres]
-
A.
Stellar Atmospheres
"Stellar Atmospheres" is a landmark astrophysics work that fundamentally advanced understanding of the physical properties and chemical composition of stars.
-
B.
Stellar Atmospheres, A Contribution to the Observational Study of High Temperature in the Reversing Layers of Stars
chosen
"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.
-
C.
Structure and Evolution of the Stars
Structure and Evolution of the Stars is a classic astrophysics textbook by Martin Schwarzschild that systematically develops the theory of stellar interiors and their life cycles.
-
D.
Thermodynamics of the Stars
Thermodynamics of the Stars is a scientific work by astrophysicist Edward Arthur Milne that applies thermodynamic principles to explain the physical structure and energy processes 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 (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_69e245f6c2e881909a228fdcfeb7c7d3 |
completed | April 17, 2026, 2:38 p.m. |
| NER | Named-entity recognition | batch_69f18e4f9be881908307838bfb5edc0c |
completed | April 29, 2026, 4:51 a.m. |
Created at: April 17, 2026, 3:59 p.m.