Triple
T20326738
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Tucana |
E492358
|
entity |
| Predicate | contains |
P35
|
FINISHED |
| Object |
47 Tuc X-9
47 Tuc X-9 is a bright X-ray source in the globular cluster 47 Tucanae, thought to be an accreting compact object such as a neutron star or black hole.
|
E1424391
|
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: 47 Tuc X-9 | Statement: [Tucana, contains, 47 Tuc X-9]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: 47 Tuc X-9 Context triple: [Tucana, contains, 47 Tuc X-9]
-
A.
NGC 5408 X-1
NGC 5408 X-1 is an ultraluminous X-ray source in the dwarf galaxy NGC 5408, thought to be powered by accretion onto a stellar-mass or intermediate-mass black hole.
-
B.
Scorpius X-1
Scorpius X-1 is a bright low-mass X-ray binary system and one of the strongest persistent X-ray sources in the sky, located in the constellation Scorpius.
-
C.
Holmberg II X-1
Holmberg II X-1 is an ultraluminous X-ray source in the dwarf galaxy Holmberg II, believed to be powered by accretion onto a compact object such as a black hole.
-
D.
Cygnus X-2
Cygnus X-2 is a bright low-mass X-ray binary system in the constellation Cygnus, consisting of a neutron star accreting matter from a companion star and serving as an important source for studying X-ray emission and compact objects.
-
E.
X Persei
X Persei is a Be/X-ray binary system in the constellation Perseus, consisting of a Be-type star and a neutron star that produces variable X-ray emissions.
- 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: 47 Tuc X-9 Triple: [Tucana, contains, 47 Tuc X-9]
Generated description
47 Tuc X-9 is a bright X-ray source in the globular cluster 47 Tucanae, thought to be an accreting compact object such as a neutron star or black hole.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: 47 Tuc X-9 Target entity description: 47 Tuc X-9 is a bright X-ray source in the globular cluster 47 Tucanae, thought to be an accreting compact object such as a neutron star or black hole.
-
A.
NGC 5408 X-1
NGC 5408 X-1 is an ultraluminous X-ray source in the dwarf galaxy NGC 5408, thought to be powered by accretion onto a stellar-mass or intermediate-mass black hole.
-
B.
Scorpius X-1
Scorpius X-1 is a bright low-mass X-ray binary system and one of the strongest persistent X-ray sources in the sky, located in the constellation Scorpius.
-
C.
Holmberg II X-1
Holmberg II X-1 is an ultraluminous X-ray source in the dwarf galaxy Holmberg II, believed to be powered by accretion onto a compact object such as a black hole.
-
D.
Cygnus X-2
Cygnus X-2 is a bright low-mass X-ray binary system in the constellation Cygnus, consisting of a neutron star accreting matter from a companion star and serving as an important source for studying X-ray emission and compact objects.
-
E.
X Persei
X Persei is a Be/X-ray binary system in the constellation Perseus, consisting of a Be-type star and a neutron star that produces variable X-ray emissions.
- 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_69e0b4a0134081909113563e1c3ba68a |
completed | April 16, 2026, 10:06 a.m. |
| NER | Named-entity recognition | batch_69e677e4130081909ec54f131939e442 |
completed | April 20, 2026, 7 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_6a08612f90b08190a6b700906944fc27 |
completed | May 16, 2026, 12:21 p.m. |
| NEDg | Description generation | batch_6a086231b440819087671c5c61adcdc6 |
completed | May 16, 2026, 12:25 p.m. |
| NED2 | Entity disambiguation (via description) | batch_6a08635869148190992d75a8806f767c |
completed | May 16, 2026, 12:30 p.m. |
Created at: April 16, 2026, 11:21 a.m.