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 7

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf astronomical spectrograph ⓘ
echelle spectrograph ⓘ
high-resolution spectrograph ⓘ
abbreviation UVES ⓘ
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 ESO VLT ⓘ
hostOrganization ESO ⓘ
lightSource celestial objects ⓘ
locatedAtTelescope Very Large Telescope ⓘ
mountedOn 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 Cerro Paranal Observatory ⓘ
linked to: Paranal Observatory
usesDispersingElement echelle grating ⓘ
wavelengthCoverage ultraviolet ⓘ
visible ⓘ

How these facts were elicited

Referenced by (7)

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