Triple
T19831549
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | W3/W4/W5 complex |
E476471
|
entity |
| Predicate | partOf |
P40
|
FINISHED |
| Object | Perseus spiral arm star-forming complexes |
—
|
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: Perseus spiral arm star-forming complexes | Statement: [W3/W4/W5 complex, partOf, Perseus spiral arm star-forming complexes]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Perseus spiral arm star-forming complexes Context triple: [W3/W4/W5 complex, partOf, Perseus spiral arm star-forming complexes]
-
A.
Milky Way spiral arms
The Milky Way spiral arms are the galaxy’s prominent, curved regions of enhanced star formation and stellar density that wind outward from its central bar.
-
B.
Perseus molecular cloud complex
chosen
The Perseus molecular cloud complex is a prominent nearby star-forming region rich in cold gas and dust, known for hosting numerous young stellar objects and protostars.
-
C.
massive star-forming complex NGC 2403-I
Massive star-forming complex NGC 2403-I is a prominent, intensely active stellar nursery region within the spiral galaxy NGC 2403, hosting large clusters of young, massive stars and associated nebular gas.
-
D.
Galactic Anticenter Stellar Structure
The Galactic Anticenter Stellar Structure is a vast, ring-like stream of stars encircling the Milky Way’s outer disk, thought to be the remnant of a disrupted dwarf galaxy or a warped extension of the Galactic disk.
-
E.
Milky Way bulge and bar
The Milky Way bulge and bar is the dense, elongated central stellar structure of our Galaxy, composed of an old, metal-rich stellar population that dominates its inner gravitational potential and strongly influences its overall dynamics.
- 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_69d8e51c7c188190b926f3a2a7b5f881 |
completed | April 10, 2026, 11:55 a.m. |
| NER | Named-entity recognition | batch_69e656ce68b48190aa25b29d0b6ea021 |
completed | April 20, 2026, 4:39 p.m. |
Created at: April 10, 2026, 1:50 p.m.