Triple
T18842572
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | HD 24534 |
E460832
|
entity |
| Predicate | hasAlternativeName |
P39
|
FINISHED |
| Object |
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.
|
E1347732
|
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: X Persei | Statement: [HD 24534, hasAlternativeName, X Persei]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: X Persei Context triple: [HD 24534, hasAlternativeName, X Persei]
-
A.
GK Persei
GK Persei is a well-known cataclysmic variable star and classical nova in the constellation Perseus, famous for its dramatic 1901 nova outburst and expanding nebular remnant.
-
B.
B Cassiopeiae
B Cassiopeiae is the historic supernova observed in 1572 in the constellation Cassiopeia, famously studied by Tycho Brahe and crucial to early modern astronomy.
-
C.
Gamma Cassiopeiae
Gamma Cassiopeiae is a bright, variable Be-type star in the constellation Cassiopeia, known for its rapid rotation, circumstellar disk, and irregular outbursts.
-
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.
Cassiopeia A
Cassiopeia A is a well-studied, relatively young supernova remnant in the constellation Cassiopeia and one of the strongest radio and X-ray sources in the sky.
- 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: X Persei Triple: [HD 24534, hasAlternativeName, X Persei]
Generated description
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.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: X Persei Target entity description: 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.
-
A.
GK Persei
GK Persei is a well-known cataclysmic variable star and classical nova in the constellation Perseus, famous for its dramatic 1901 nova outburst and expanding nebular remnant.
-
B.
B Cassiopeiae
B Cassiopeiae is the historic supernova observed in 1572 in the constellation Cassiopeia, famously studied by Tycho Brahe and crucial to early modern astronomy.
-
C.
Gamma Cassiopeiae
Gamma Cassiopeiae is a bright, variable Be-type star in the constellation Cassiopeia, known for its rapid rotation, circumstellar disk, and irregular outbursts.
-
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.
Cassiopeia A
Cassiopeia A is a well-studied, relatively young supernova remnant in the constellation Cassiopeia and one of the strongest radio and X-ray sources in the sky.
- 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_69d8dcfa11e4819090ab1ef5bdcd2b2e |
completed | April 10, 2026, 11:20 a.m. |
| NER | Named-entity recognition | batch_69e5b8eb32548190b2313e877f6ff179 |
completed | April 20, 2026, 5:26 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_6a0582a3bd7881908dcd97ece5f576a8 |
completed | May 14, 2026, 8:06 a.m. |
| NEDg | Description generation | batch_6a0584717b3c81908049e6590f7f96ec |
completed | May 14, 2026, 8:14 a.m. |
| NED2 | Entity disambiguation (via description) | batch_6a05852c2bbc8190ae7b8658817b5972 |
completed | May 14, 2026, 8:17 a.m. |
Created at: April 10, 2026, 11:56 a.m.