Spectro-Polarimetric High-contrast Exoplanet REsearch
E668444
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.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Spectro-Polarimetric High-contrast Exoplanet REsearch canonical | 2 |
How this entity was disambiguated
This entity first appeared as the object of triple T7486564 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Spectro-Polarimetric High-contrast Exoplanet REsearch Context triple: [SPHERE, fullName, Spectro-Polarimetric High-contrast Exoplanet REsearch]
-
A.
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.
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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.
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.
-
D.
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.
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E.
Wide Angle Search for Planets
Wide Angle Search for Planets (WASP) is a ground-based exoplanet survey project that uses wide-field cameras to detect transiting planets around bright stars.
- 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: Spectro-Polarimetric High-contrast Exoplanet REsearch Target entity description: 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.
-
A.
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.
-
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.
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.
-
D.
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.
-
E.
Wide Angle Search for Planets
Wide Angle Search for Planets (WASP) is a ground-based exoplanet survey project that uses wide-field cameras to detect transiting planets around bright stars.
- F. None of above. chosen
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
VLT instrument
ⓘ
astronomical instrument ⓘ |
| abbreviation | SPHERE NERFINISHED ⓘ |
| country | Chile ⓘ |
| fieldOfStudy |
circumstellar environments
ⓘ
exoplanet science ⓘ planet formation ⓘ |
| hasCapability |
angular differential imaging
ⓘ
differential imaging ⓘ polarimetric differential imaging ⓘ spectral differential imaging ⓘ |
| hasSubsystem |
IFS
NERFINISHED
ⓘ
IRDIS NERFINISHED ⓘ SAXO NERFINISHED ⓘ ZIMPOL NERFINISHED ⓘ |
| hostTelescope | Very Large Telescope NERFINISHED ⓘ |
| hostTelescopeAperture | 8.2 m ⓘ |
| locatedAt | Paranal Observatory NERFINISHED ⓘ |
| locatedIn | Very Large Telescope NERFINISHED ⓘ |
| locationRegion | Atacama Desert NERFINISHED ⓘ |
| observatoryAltitude | ~2635 m ⓘ |
| observatorySite | Cerro Paranal NERFINISHED ⓘ |
| operator | European Southern Observatory NERFINISHED ⓘ |
| primaryPurpose |
characterization of exoplanets
ⓘ
direct imaging of exoplanets ⓘ imaging of circumstellar disks ⓘ |
| scienceGoal |
measurement of exoplanet atmospheres
ⓘ
measurement of exoplanet orbits ⓘ measurement of exoplanet photometry ⓘ measurement of exoplanet spectra ⓘ study of circumstellar dust disks ⓘ study of young giant exoplanets ⓘ |
| scientificDiscipline |
astronomy
ⓘ
astrophysics ⓘ |
| subsystemFullName |
Infra-Red Dual-beam Imager and Spectrograph
NERFINISHED
ⓘ
Integral Field Spectrograph NERFINISHED ⓘ SPHERE AO for eXoplanet Observation NERFINISHED ⓘ Zurich IMaging POLarimeter NERFINISHED ⓘ |
| telescopeUnit | VLT Unit Telescope 3 NERFINISHED ⓘ |
| telescopeUnitName | Melipal NERFINISHED ⓘ |
| usesTechnique |
adaptive optics
ⓘ
coronagraphy ⓘ high-contrast imaging ⓘ integral field spectroscopy ⓘ polarimetry ⓘ |
| wavelengthRange |
near-infrared
ⓘ
visible ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
Instruction
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Input
Subject: Spectro-Polarimetric High-contrast Exoplanet REsearch Description of subject: 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.
Referenced by (2)
Full triples — surface form annotated when it differs from this entity's canonical label.