UVES

E176893

UVES (Ultraviolet and Visual Echelle Spectrograph) is a high-resolution spectrograph used in optical and ultraviolet astronomy to analyze the light from celestial objects in great detail.

All labels observed (1)

Label Occurrences
UVES canonical 4

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Statements (47)

Predicate Object
instanceOf astronomical spectrograph
echelle spectrograph
high-resolution spectrograph
abbreviation UVES self-link
altitudeOfSite about 2635 m above sea level
commissionedBy European Southern Observatory
country Chile
dataProduct high-resolution spectra
detectorType CCD
enables detailed line profile analysis
isotopic ratio measurements
metallicity determinations
precision radial velocity studies
field optical astronomy
ultraviolet astronomy
fullName Ultraviolet and Visual Echelle Spectrograph
geographicHemisphere Southern Hemisphere
hasMode dichroic mode
single-arm mode
hasSpectralArms blue arm
red arm
hostFacility Very Large Telescope
surface form: ESO VLT
hostOrganization European Southern Observatory
surface form: ESO
lightSource celestial objects
locatedAtTelescope Very Large Telescope
mountedOn Very Large Telescope
surface form: VLT Unit Telescope 2 Kueyen
observatorySite Paranal Observatory
observes exoplanet host stars
galaxies
nebulae
quasars
stars
operatedBy European Southern Observatory
operationalStatus in operation
partOf VLT instrumentation suite
scienceUse chemical abundance studies of stars
exoplanet atmosphere characterization
high-resolution spectroscopy of astronomical sources
interstellar medium studies
measurement of fundamental constants variability
quasar absorption line studies
radial velocity measurements
spectralResolution up to about 110000
telescopeLocation Paranal Observatory
surface form: Cerro Paranal Observatory
usesDispersingElement echelle grating
wavelengthCoverage ultraviolet
visible

How these facts were elicited

Referenced by (4)

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