Triple
T12175617
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | NGC 3372 |
E290078
|
entity |
| Predicate | containsObject |
P11236
|
FINISHED |
| Object | Herbig–Haro objects |
E290083
|
NE FINISHED |
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: Herbig–Haro objects | Statement: [NGC 3372, containsObject, Herbig–Haro objects]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Herbig–Haro objects Context triple: [NGC 3372, containsObject, Herbig–Haro objects]
-
A.
Herbig–Haro objects
chosen
Herbig–Haro objects are small, bright patches of nebulosity formed when jets of gas from newborn stars collide with surrounding interstellar material.
-
B.
Herbig Ae/Be stars
Herbig Ae/Be stars are young, intermediate-mass pre-main-sequence stars that are still contracting toward the main sequence and are often surrounded by gas and dust disks.
-
C.
Pleiades reflection nebulae
The Pleiades reflection nebulae are faint, blue-tinged clouds of interstellar dust that visibly reflect the light of the young, hot stars in the Pleiades star cluster.
-
D.
Quasi-Stellar Objects
Quasi-Stellar Objects, commonly known as quasars, are extremely luminous and distant active galactic nuclei powered by supermassive black holes accreting matter at the centers of young galaxies.
-
E.
R Coronae Australis
R Coronae Australis is a young variable star embedded in the Corona Australis star-forming region, notable for its irregular brightness changes and association with reflection nebulosity.
- F. None of above.
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Provenance (3 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_69d6ab4d6c00819095a9a7c35de83cfb |
completed | April 8, 2026, 7:23 p.m. |
| NER | Named-entity recognition | batch_69d915dc71788190bdaadf7be9d8d6ce |
completed | April 10, 2026, 3:23 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69f5f6a9482481909500c216f23fceb4 |
completed | May 2, 2026, 1:05 p.m. |
Created at: April 8, 2026, 9:50 p.m.