Triple
T7486565
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | SPHERE |
E176895
|
entity |
| Predicate | acronymFor |
P590
|
FINISHED |
| Object | Spectro-Polarimetric High-contrast Exoplanet REsearch |
E668444
|
NE FINISHED |
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: Spectro-Polarimetric High-contrast Exoplanet REsearch | Statement: [SPHERE, acronymFor, Spectro-Polarimetric High-contrast Exoplanet REsearch]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Spectro-Polarimetric High-contrast Exoplanet REsearch Context triple: [SPHERE, acronymFor, Spectro-Polarimetric High-contrast Exoplanet REsearch]
-
A.
Spectro-Polarimetric High-contrast Exoplanet REsearch
chosen
Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) is a high-performance instrument on the Very Large Telescope designed to directly image and characterize exoplanets and circumstellar disks using advanced adaptive optics and polarimetry.
-
B.
SCExAO
SCExAO (Subaru Coronagraphic Extreme Adaptive Optics) is a high-performance adaptive optics and coronagraphic instrument on the Subaru Telescope designed for direct imaging and characterization of exoplanets and circumstellar environments.
-
C.
SAXO – SPHERE AO for eXoplanet Observation
SAXO – SPHERE AO for eXoplanet Observation is the extreme adaptive optics system of the SPHERE instrument on the Very Large Telescope, designed to correct atmospheric turbulence and enable high-contrast imaging of exoplanets.
-
D.
Metis coronagraph
Metis coronagraph is a specialized telescope instrument designed to block the Sun’s bright disk so it can image and study the faint outer solar corona in visible and ultraviolet light.
-
E.
Lyot coronagraphs
Lyot coronagraphs are optical devices used in telescopes to block out the bright light of a star so that faint nearby objects, such as exoplanets or circumstellar disks, can be imaged.
- F. None of above.
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Provenance (3 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_69c69f24ac508190bb98fe927c0bd065 |
completed | March 27, 2026, 3:15 p.m. |
| NER | Named-entity recognition | batch_69c6f5582adc81908b68439762965d88 |
completed | March 27, 2026, 9:23 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69c845fd62dc8190a64f5464a204c0d2 |
completed | March 28, 2026, 9:19 p.m. |
Created at: March 27, 2026, 3:42 p.m.