IRDIS

E668446

IRDIS is the dual-band infrared imaging and spectroscopy sub-instrument of the SPHERE exoplanet imager on the Very Large Telescope, optimized for high-contrast observations of exoplanets and circumstellar environments.

All labels observed (1)

Label Occurrences
IRDIS canonical 3

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Statements (47)

Predicate Object
instanceOf astronomical instrument
infrared imaging instrument
spectrograph
acronymFor Infra-Red Dual-beam Imager and Spectrograph
commissionedAt Very Large Telescope
commissioningCompleted 2014
coronagraphType apodized pupil Lyot coronagraph
country Chile
designedFor extreme adaptive optics corrected observations
detectorType infrared array detector
fieldOfView approximately 11 arcseconds by 12.5 arcseconds
firstLight 2014
fullName Infra-Red Dual-beam Imager and Spectrograph
hasCapability dual-band imaging
dual-polarization imaging
long-slit spectroscopy
hasFilter H band
J band
K band
Y band
hasMode dual-band imaging mode
dual-polarization imaging mode
long-slit spectroscopy mode
hostInstrument SPHERE
isSubInstrumentOf SPHERE exoplanet imager
locatedAt Paranal Observatory
Very Large Telescope
mountedOn VLT Nasmyth platform
observatory ESO Paranal Observatory
linked to: Paranal Observatory
observesInBand near-infrared
operatedBy European Southern Observatory
optimizedFor circumstellar environment studies
exoplanet detection
high-contrast imaging
partOf SPHERE
scienceGoal characterization of exoplanet atmospheres
direct imaging of exoplanets
imaging of circumstellar disks
study of brown dwarfs
sharesInstrumentPlatformWith SPHERE-IFS
linked to: SPHERE

ZIMPOL
telescopeUnit VLT Unit Telescope 3 Melipal
usesCoronagraph yes
usesTechnique differential imaging
polarimetric differential imaging
spectral differential imaging
wavelengthRange 0.95–2.32 micrometres

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Referenced by (3)

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