Triple
T20161469
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | GCl 111 |
E491712
|
entity |
| Predicate | OosterhoffType |
P94583
|
FINISHED |
| Object |
Oosterhoff type II
Oosterhoff type II is a classification of globular clusters characterized by relatively metal-poor RR Lyrae variable stars with longer pulsation periods than those in Oosterhoff type I clusters.
|
E1415017
|
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: Oosterhoff type II | Statement: [GCl 111, OosterhoffType, Oosterhoff type II]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Oosterhoff type II Context triple: [GCl 111, OosterhoffType, Oosterhoff type II]
-
A.
Cepheid variables
Cepheid variables are pulsating stars whose regular brightness variations make them crucial standard candles for measuring cosmic distances and mapping galactic structure.
-
B.
Delta Scuti
Delta Scuti is a variable star in the constellation Scutum, serving as the prototype of the Delta Scuti class of short-period pulsating stars.
-
C.
Cepheid
Cepheid is a molecular diagnostics company known for its rapid, automated PCR-based testing systems used in clinical and research settings.
-
D.
RV Tauri
RV Tauri is a class of luminous pulsating variable stars, typically post-asymptotic giant branch objects, characterized by alternating deep and shallow minima in their light curves.
-
E.
Beta Cephei
Beta Cephei is a class of hot, massive B-type pulsating variable stars whose brightness variations are driven by pressure and gravity mode oscillations.
- 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: Oosterhoff type II Triple: [GCl 111, OosterhoffType, Oosterhoff type II]
Generated description
Oosterhoff type II is a classification of globular clusters characterized by relatively metal-poor RR Lyrae variable stars with longer pulsation periods than those in Oosterhoff type I clusters.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Oosterhoff type II Target entity description: Oosterhoff type II is a classification of globular clusters characterized by relatively metal-poor RR Lyrae variable stars with longer pulsation periods than those in Oosterhoff type I clusters.
-
A.
Cepheid variables
Cepheid variables are pulsating stars whose regular brightness variations make them crucial standard candles for measuring cosmic distances and mapping galactic structure.
-
B.
Delta Scuti
Delta Scuti is a variable star in the constellation Scutum, serving as the prototype of the Delta Scuti class of short-period pulsating stars.
-
C.
Cepheid
Cepheid is a molecular diagnostics company known for its rapid, automated PCR-based testing systems used in clinical and research settings.
-
D.
RV Tauri
RV Tauri is a class of luminous pulsating variable stars, typically post-asymptotic giant branch objects, characterized by alternating deep and shallow minima in their light curves.
-
E.
Beta Cephei
Beta Cephei is a class of hot, massive B-type pulsating variable stars whose brightness variations are driven by pressure and gravity mode oscillations.
- 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_69da6266c6888190bc1a3ecf24814d34 |
completed | April 11, 2026, 3:01 p.m. |
| NER | Named-entity recognition | batch_69e667e43940819080f6a0b7331aaab0 |
completed | April 20, 2026, 5:52 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_6a08347b41d8819086bd36e5e04c69ad |
completed | May 16, 2026, 9:10 a.m. |
| NEDg | Description generation | batch_6a08359866c481908aa30ac61e18bcb0 |
completed | May 16, 2026, 9:15 a.m. |
| NED2 | Entity disambiguation (via description) | batch_6a08361f64a08190af3305685a50f001 |
completed | May 16, 2026, 9:17 a.m. |
Created at: April 11, 2026, 11:34 p.m.