Triple
T12271345
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | SOHO |
E292476
|
entity |
| Predicate | hasInstrument |
P35
|
FINISHED |
| Object |
Large Angle and Spectrometric Coronagraph
The Large Angle and Spectrometric Coronagraph (LASCO) is a space-based solar coronagraph instrument that images the Sun’s outer atmosphere to study coronal mass ejections and other solar phenomena.
|
E975804
|
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: Large Angle and Spectrometric Coronagraph | Statement: [SOHO, hasInstrument, Large Angle and Spectrometric Coronagraph]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Large Angle and Spectrometric Coronagraph Context triple: [SOHO, hasInstrument, Large Angle and Spectrometric Coronagraph]
-
A.
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.
-
B.
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.
-
C.
Coronagraph Instrument
The Coronagraph Instrument is a high-contrast imaging and spectroscopy tool on the Nancy Grace Roman Space Telescope designed to directly observe and characterize exoplanets and faint circumstellar material near bright stars.
-
D.
JWST coronagraphy with MIRI
JWST coronagraphy with MIRI is an observing mode of the James Webb Space Telescope’s Mid-Infrared Instrument that uses specialized masks and optics to block starlight and enable high-contrast imaging of faint structures such as exoplanets and circumstellar disks in the mid-infrared.
-
E.
Spectro-Polarimetric High-contrast Exoplanet REsearch
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.
- 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: Large Angle and Spectrometric Coronagraph Triple: [SOHO, hasInstrument, Large Angle and Spectrometric Coronagraph]
Generated description
The Large Angle and Spectrometric Coronagraph (LASCO) is a space-based solar coronagraph instrument that images the Sun’s outer atmosphere to study coronal mass ejections and other solar phenomena.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Large Angle and Spectrometric Coronagraph Target entity description: The Large Angle and Spectrometric Coronagraph (LASCO) is a space-based solar coronagraph instrument that images the Sun’s outer atmosphere to study coronal mass ejections and other solar phenomena.
-
A.
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.
-
B.
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.
-
C.
Coronagraph Instrument
The Coronagraph Instrument is a high-contrast imaging and spectroscopy tool on the Nancy Grace Roman Space Telescope designed to directly observe and characterize exoplanets and faint circumstellar material near bright stars.
-
D.
JWST coronagraphy with MIRI
JWST coronagraphy with MIRI is an observing mode of the James Webb Space Telescope’s Mid-Infrared Instrument that uses specialized masks and optics to block starlight and enable high-contrast imaging of faint structures such as exoplanets and circumstellar disks in the mid-infrared.
-
E.
Spectro-Polarimetric High-contrast Exoplanet REsearch
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.
- 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_69d6ab6856488190b5d31178d5015f8e |
completed | April 8, 2026, 7:24 p.m. |
| NER | Named-entity recognition | batch_69d91cee7158819093fff74db6867896 |
completed | April 10, 2026, 3:53 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69f61e6981b48190a0fc5a571c425be1 |
completed | May 2, 2026, 3:55 p.m. |
| NEDg | Description generation | batch_69f622de74f0819096c5f5bf6f938fe7 |
completed | May 2, 2026, 4:14 p.m. |
| NED2 | Entity disambiguation (via description) | batch_69f62379746c8190bc9da48775b86dfa |
completed | May 2, 2026, 4:16 p.m. |
Created at: April 8, 2026, 9:52 p.m.