Triple
T23527815
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Pegasus |
E576479
|
entity |
| Predicate | containsStar |
P1393
|
FINISHED |
| Object |
V391 Pegasi
V391 Pegasi is a pulsating subdwarf B star in the constellation Pegasus, notable for earlier claims that it might host a planetary companion detected via its oscillations.
|
E1592225
|
NE FINISHED |
How this triple was built (3 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: V391 Pegasi | Statement: [Pegasus, containsStar, V391 Pegasi]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: V391 Pegasi Context triple: [Pegasus, containsStar, V391 Pegasi]
-
A.
Zeta Pegasi
Zeta Pegasi, traditionally named Homam, is a bright blue-white star in the constellation Pegasus that forms part of the Great Square asterism.
-
B.
IM Pegasi
IM Pegasi is a nearby RS Canum Venaticorum-type binary star system in the constellation Pegasus, notable for its strong radio emissions and use as the guide star for the Gravity Probe B relativity experiment.
-
C.
Gamma Pegasi
Gamma Pegasi, traditionally named Algenib, is a hot blue subgiant star in the constellation Pegasus that forms one corner of the Great Square asterism.
-
D.
Eta Pegasi
Eta Pegasi, traditionally named Matar, is a bright binary star system in the constellation Pegasus visible to the naked eye.
-
E.
Epsilon Pegasi
Epsilon Pegasi, traditionally named Enif, is the brightest star in the constellation Pegasus and a prominent orange supergiant visible to the naked eye.
- 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: V391 Pegasi Triple: [Pegasus, containsStar, V391 Pegasi]
Generated description
V391 Pegasi is a pulsating subdwarf B star in the constellation Pegasus, notable for earlier claims that it might host a planetary companion detected via its oscillations.
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_69e245f5a8848190a2ba42e271c6c31f |
completed | April 17, 2026, 2:38 p.m. |
| NER | Named-entity recognition | batch_69f1ac758038819098f5f597be39274e |
completed | April 29, 2026, 7 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_6a0cdf53c66c819087f1e9481dcfc8ee |
completed | May 19, 2026, 10:08 p.m. |
| NEDg | Description generation | batch_6a0ce4602a408190b4357d98cf16477a |
completed | May 19, 2026, 10:29 p.m. |
| NED2 | Entity disambiguation (via description) | batch_6a0d721bdae08190a06f48a6073c5351 |
completed | May 20, 2026, 8:34 a.m. |
Created at: April 17, 2026, 6:09 p.m.