Triple
T18771719
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | H II region |
E459029
|
entity |
| Predicate | relatedTo |
P37
|
FINISHED |
| Object |
Strömgren sphere
A Strömgren sphere is a region of ionized hydrogen gas surrounding a hot, young star, formed where the star’s ultraviolet radiation balances the recombination of electrons and protons in the surrounding interstellar medium.
|
E1341707
|
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: Strömgren sphere | Statement: [H II region, relatedTo, Strömgren sphere]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Strömgren sphere Context triple: [H II region, relatedTo, Strömgren sphere]
-
A.
Milne–Eddington approximation
The Milne–Eddington approximation is a simplified model of stellar atmospheres that assumes constant physical properties with depth to make the radiative transfer equations analytically tractable.
-
B.
Eddington limit
The Eddington limit is the maximum luminosity a star or accreting object can have before radiation pressure overcomes gravity and drives away its outer layers.
-
C.
Rosseland
Rosseland is a Norwegian surname most notably associated with astrophysicist Svein Rosseland, a pioneer in theoretical astrophysics and radiative transfer.
-
D.
Bonnor–Ebert mass
The Bonnor–Ebert mass is the maximum mass a pressure-confined, self-gravitating gas sphere can have while remaining in stable hydrostatic equilibrium before collapsing under its own gravity.
-
E.
Schwarzschild criterion
The Schwarzschild criterion is a condition in astrophysics that determines when a star’s interior becomes convectively unstable, leading to energy transport by bulk motion of stellar material.
- 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: Strömgren sphere Triple: [H II region, relatedTo, Strömgren sphere]
Generated description
A Strömgren sphere is a region of ionized hydrogen gas surrounding a hot, young star, formed where the star’s ultraviolet radiation balances the recombination of electrons and protons in the surrounding interstellar medium.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Strömgren sphere Target entity description: A Strömgren sphere is a region of ionized hydrogen gas surrounding a hot, young star, formed where the star’s ultraviolet radiation balances the recombination of electrons and protons in the surrounding interstellar medium.
-
A.
Milne–Eddington approximation
The Milne–Eddington approximation is a simplified model of stellar atmospheres that assumes constant physical properties with depth to make the radiative transfer equations analytically tractable.
-
B.
Eddington limit
The Eddington limit is the maximum luminosity a star or accreting object can have before radiation pressure overcomes gravity and drives away its outer layers.
-
C.
Rosseland
Rosseland is a Norwegian surname most notably associated with astrophysicist Svein Rosseland, a pioneer in theoretical astrophysics and radiative transfer.
-
D.
Bonnor–Ebert mass
The Bonnor–Ebert mass is the maximum mass a pressure-confined, self-gravitating gas sphere can have while remaining in stable hydrostatic equilibrium before collapsing under its own gravity.
-
E.
Schwarzschild criterion
The Schwarzschild criterion is a condition in astrophysics that determines when a star’s interior becomes convectively unstable, leading to energy transport by bulk motion of stellar material.
- 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_69d8d395dba0819087568404508590cb |
completed | April 10, 2026, 10:40 a.m. |
| NER | Named-entity recognition | batch_69e59336a6b08190819595a55177264e |
completed | April 20, 2026, 2:45 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_6a053d46f1b88190b51ed8af4004c880 |
completed | May 14, 2026, 3:11 a.m. |
| NEDg | Description generation | batch_6a053ee038708190a242cb62fee15302 |
completed | May 14, 2026, 3:17 a.m. |
| NED2 | Entity disambiguation (via description) | batch_6a053fba29208190ac0ee5a05522a7e2 |
completed | May 14, 2026, 3:21 a.m. |
Created at: April 10, 2026, 11:52 a.m.