Triple
T22400725
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Abell 262 |
E553750
|
entity |
| Predicate | hasAlternativeName |
P39
|
FINISHED |
| Object | RXC J0152.0+3609 |
—
|
NE NERFINISHED |
How this triple was built (3 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: RXC J0152.0+3609 | Statement: [Abell 262, hasAlternativeName, RXC J0152.0+3609]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: RXC J0152.0+3609 Context triple: [Abell 262, hasAlternativeName, RXC J0152.0+3609]
-
A.
RX J0720.4-3125
RX J0720.4-3125 is an isolated, thermally emitting neutron star in the constellation Puppis, notable for its soft X-ray emission and use in studying neutron star cooling and magnetic fields.
-
B.
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.
-
C.
PKS 1322-428
PKS 1322-428 is a radio source designation for NGC 5128, the nearby active galaxy better known as Centaurus A.
-
D.
HIPASS J1321-36
HIPASS J1321-36 is a nearby lenticular galaxy in the constellation Centaurus, better known as NGC 5102, notable for its relatively recent star formation and prominent neutral hydrogen content.
-
E.
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.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: RXC J0152.0+3609 Target entity description: RXC J0152.0+3609 is a galaxy cluster, also cataloged as Abell 262, located in the constellation Andromeda and known for its role in studies of large-scale structure and intracluster gas.
-
A.
RX J0720.4-3125
RX J0720.4-3125 is an isolated, thermally emitting neutron star in the constellation Puppis, notable for its soft X-ray emission and use in studying neutron star cooling and magnetic fields.
-
B.
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.
-
C.
PKS 1322-428
PKS 1322-428 is a radio source designation for NGC 5128, the nearby active galaxy better known as Centaurus A.
-
D.
HIPASS J1321-36
HIPASS J1321-36 is a nearby lenticular galaxy in the constellation Centaurus, better known as NGC 5102, notable for its relatively recent star formation and prominent neutral hydrogen content.
-
E.
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.
- F. None of above. chosen
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_69e11e4da7048190b4387d422a9a0de5 |
completed | April 16, 2026, 5:37 p.m. |
| NER | Named-entity recognition | batch_69f158b39c908190a735aa860d733869 |
completed | April 29, 2026, 1:02 a.m. |
Created at: April 16, 2026, 8:46 p.m.