Triple
T22412684
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Beta Persei B |
E554031
|
entity |
| Predicate | instanceOf |
P0
|
FINISHED |
| Object | K-type subgiant star |
C6901
|
CONCEPT FINISHED |
How this triple was built (1 step)
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.
CD
Concept disambiguation
gpt-5-mini-2025-08-07
Target class: K-type subgiant star Context triple: [Beta Persei B, instanceOf, K-type subgiant star]
-
A.
G-type giant star
A G-type giant star is an evolved, luminous star of spectral type G that has exhausted hydrogen in its core and expanded to a much larger radius and brightness than a main-sequence G-type star.
-
B.
B-type main-sequence star
A B-type main-sequence star is a hot, massive, blue-white star fusing hydrogen in its core, characterized by strong helium lines and high luminosity.
-
C.
A-type main-sequence star
An A-type main-sequence star is a hot, white or bluish-white hydrogen-fusing star with strong hydrogen absorption lines and a surface temperature typically between about 7,500 and 10,000 K.
-
D.
subgiant star
chosen
A subgiant star is a stellar object that has exhausted hydrogen in its core and is transitioning off the main sequence, expanding and cooling as it begins to burn hydrogen in a surrounding shell.
-
E.
F-type star
An F-type star is a moderately hot, yellow-white main-sequence star with surface temperatures around 6,000–7,600 K, more massive and luminous than the Sun, and characterized by strong hydrogen lines and ionized metal absorption features in its spectrum.
- F. None of above.
Provenance (1 batch)
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_69e11e4e6ce8819085a1e06d886bf21c |
completed | April 16, 2026, 5:37 p.m. |
Created at: April 16, 2026, 8:46 p.m.