Triple
T20499119
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | NGC 2004 |
E503253
|
entity |
| Predicate | partOf |
P40
|
FINISHED |
| Object | LMC bar region (approx) |
—
|
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: LMC bar region (approx) | Statement: [NGC 2004, partOf, LMC bar region (approx)]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: LMC bar region (approx) Context triple: [NGC 2004, partOf, LMC bar region (approx)]
-
A.
LMC bar region
chosen
The LMC bar region is the dense, elongated central structure of the Large Magellanic Cloud galaxy, rich in stars, gas, and active star-forming sites.
-
B.
L1641-N region
The L1641-N region is a dense star-forming clump within the Lynds 1641 molecular cloud in Orion, notable for its embedded young stellar objects and active protostellar outflows.
-
C.
Coalsack Nebula region
The Coalsack Nebula region is a prominent dark molecular cloud complex in the southern Milky Way, known for its dense dust that obscures background starlight and hosts small, star-forming Bok globules.
-
D.
Scorpius tail region
The Scorpius tail region is the southern part of the Scorpius constellation, rich in star clusters and nebulae and often observed in deep-sky surveys.
-
E.
W5 H II region
W5 H II region is a large ionized hydrogen cloud in the Milky Way notable for active star formation and complex nebular structures.
- 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_69e0b4b1e52c8190894281cf7e3283ab |
completed | April 16, 2026, 10:06 a.m. |
| NER | Named-entity recognition | batch_69e69cbff210819089900e9a35911f48 |
completed | April 20, 2026, 9:38 p.m. |
Created at: April 16, 2026, 11:35 a.m.