SAXO

E668445

SAXO is an advanced adaptive optics system designed to correct atmospheric distortions and sharpen astronomical images for the SPHERE instrument on the Very Large Telescope.

All labels observed (1)

Label Occurrences
SAXO canonical 2

How this entity was disambiguated

Statements (38)

Predicate Object
instanceOf adaptive optics system
astronomical instrumentation subsystem
acronymFor SPHERE Adaptive optics for eXoplanet Observation
applicationDomain circumstellar disk studies
exoplanet science
stellar astrophysics
correctionType extreme adaptive optics
designedFor SPHERE instrument
developmentContext VLT second-generation instrumentation
enablesCapability coronagraphic imaging
polarimetric differential imaging
spectral differential imaging
fieldOfUse ground-based astronomy
fullName SPHERE Adaptive optics for eXoplanet Observation
hostInstrumentMode SPHERE/IFS
linked to: SPHERE

SPHERE/IRDIS
hostInstrumentMode SPHERE/ZIMPOL
linked to: ZIMPOL
hostTelescope VLT UT3 Melipal
installedAt Paranal Observatory
installedOn Very Large Telescope
locatedOnTelescopeUnit VLT Unit Telescope 3
observatory ESO Paranal Observatory
linked to: Paranal Observatory
observingWavelengthRange near-infrared
visible
operatedBy European Southern Observatory
optimizedFor exoplanet detection
high-contrast imaging
partOf SPHERE
primaryPurpose correct atmospheric distortions
sharpen astronomical images
scienceGoal direct imaging of exoplanets
high-contrast imaging of circumstellar environments
telescopeAperture 8.2-metre class
usesComponent high-order deformable mirror
real-time computer
tip-tilt mirror
wavefront sensor
wavefrontSensorType Shack–Hartmann wavefront sensor

How these facts were elicited

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.