Triple
T23344598
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | UV Ceti |
E591821
|
entity |
| Predicate | prototypeOf |
P43658
|
FINISHED |
| Object | UV Ceti-type flare stars |
—
|
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: UV Ceti-type flare stars | Statement: [UV Ceti, prototypeOf, UV Ceti-type flare stars]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: UV Ceti-type flare stars Context triple: [UV Ceti, prototypeOf, UV Ceti-type flare stars]
-
A.
Stellar Atmospheres
"Stellar Atmospheres" is a landmark astrophysics work that fundamentally advanced understanding of the physical properties and chemical composition of stars.
-
B.
RR Lyrae variable stars
RR Lyrae variable stars are old, low-mass pulsating stars used as standard candles to measure distances within the Milky Way and nearby galaxies.
-
C.
UV Ceti
chosen
UV Ceti is a nearby red dwarf flare star in the constellation Cetus, famous as the prototype of UV Ceti-type flare stars that exhibit sudden, dramatic increases in brightness.
-
D.
Anomalous Cepheids
Anomalous Cepheids are a rare type of pulsating variable star, typically found in old, metal-poor stellar populations, that are brighter and more massive than expected for their period compared to classical and Type II Cepheids.
-
E.
New Catalogue of Suspected Variable Stars
The New Catalogue of Suspected Variable Stars is an astronomical reference listing stars that are suspected, but not yet confirmed, to exhibit variability in their brightness.
- 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_69e25d20e3d08190bcede87673cafb25 |
completed | April 17, 2026, 4:17 p.m. |
| NER | Named-entity recognition | batch_69f198358fb8819094c74cfd53cbab44 |
completed | April 29, 2026, 5:33 a.m. |
Created at: April 17, 2026, 5:19 p.m.