Triple
T20665793
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Antlia 2 Dwarf Galaxy |
E507881
|
entity |
| Predicate | publication |
P80
|
FINISHED |
| Object | Torrealba et al. 2019 MNRAS paper |
—
|
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: Torrealba et al. 2019 MNRAS paper | Statement: [Antlia 2 Dwarf Galaxy, publication, Torrealba et al. 2019 MNRAS paper]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Torrealba et al. 2019 MNRAS paper Context triple: [Antlia 2 Dwarf Galaxy, publication, Torrealba et al. 2019 MNRAS paper]
-
A.
AAS Open Research
AAS Open Research is an open-access publishing platform of the American Astronomical Society that supports rapid, transparent dissemination and peer review of research in astronomy and astrophysics.
-
B.
Faber–Jackson relation paper
The Faber–Jackson relation paper is a landmark astrophysics publication that established a correlation between the luminosity and stellar velocity dispersion of elliptical galaxies, providing key insights into their structure and evolution.
-
C.
Tolman surface brightness test
The Tolman surface brightness test is an observational cosmology method that checks whether the universe is expanding by examining how the surface brightness of distant galaxies diminishes with redshift.
-
D.
Bahcall–Soneira model of the Milky Way
The Bahcall–Soneira model of the Milky Way is a pioneering analytic model of our Galaxy’s structure that describes the spatial distribution of stars in its disk and halo, widely used before more detailed modern surveys.
-
E.
Revised Shapley–Ames Catalog
The Revised Shapley–Ames Catalog is an astronomical catalog that lists bright galaxies, providing standardized data and classifications widely used in extragalactic astronomy.
- 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: Torrealba et al. 2019 MNRAS paper Target entity description: The Torrealba et al. 2019 MNRAS paper is the study that reported the discovery and characterization of Antlia 2, an extremely diffuse and low-surface-brightness dwarf galaxy satellite of the Milky Way.
-
A.
AAS Open Research
AAS Open Research is an open-access publishing platform of the American Astronomical Society that supports rapid, transparent dissemination and peer review of research in astronomy and astrophysics.
-
B.
Faber–Jackson relation paper
The Faber–Jackson relation paper is a landmark astrophysics publication that established a correlation between the luminosity and stellar velocity dispersion of elliptical galaxies, providing key insights into their structure and evolution.
-
C.
Tolman surface brightness test
The Tolman surface brightness test is an observational cosmology method that checks whether the universe is expanding by examining how the surface brightness of distant galaxies diminishes with redshift.
-
D.
Bahcall–Soneira model of the Milky Way
The Bahcall–Soneira model of the Milky Way is a pioneering analytic model of our Galaxy’s structure that describes the spatial distribution of stars in its disk and halo, widely used before more detailed modern surveys.
-
E.
Revised Shapley–Ames Catalog
The Revised Shapley–Ames Catalog is an astronomical catalog that lists bright galaxies, providing standardized data and classifications widely used in extragalactic astronomy.
- 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_69e0b4c059bc81908ea762cd73ea4424 |
completed | April 16, 2026, 10:06 a.m. |
| NER | Named-entity recognition | batch_69e6b5c2c6d48190bbfe505cf7d973f9 |
completed | April 20, 2026, 11:24 p.m. |
Created at: April 16, 2026, 11:44 a.m.