Ultraviolet and Visual Echelle Spectrograph
E668443
The Ultraviolet and Visual Echelle Spectrograph (UVES) is a high-resolution spectrograph mounted on ESO’s Very Large Telescope, used to obtain detailed spectra of astronomical objects in the ultraviolet and visible wavelength ranges.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Ultraviolet and Visual Echelle Spectrograph canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T7486470 — 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: Ultraviolet and Visual Echelle Spectrograph Context triple: [UVES, fullName, Ultraviolet and Visual Echelle Spectrograph]
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A.
Ultraviolet Spectrometer
The Ultraviolet Spectrometer was a scientific instrument on the Galileo spacecraft used to analyze ultraviolet light from celestial objects to study their composition, atmospheres, and energy processes.
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B.
Ultraviolet Imaging Spectrograph (UVS)
The Ultraviolet Imaging Spectrograph (UVS) is a scientific instrument that observes ultraviolet light to study the composition, structure, and dynamics of Jupiter’s atmosphere and auroras.
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C.
Europa Ultraviolet Spectrograph
The Europa Ultraviolet Spectrograph is a scientific instrument designed to study Europa’s tenuous atmosphere, surface composition, and space environment by analyzing ultraviolet light during NASA’s Europa Clipper mission.
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D.
DEIMOS spectrograph
The DEIMOS spectrograph is a powerful multi-object optical spectrograph designed for wide-field, high-resolution spectroscopy of faint astronomical sources.
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E.
Goddard High Resolution Spectrograph
The Goddard High Resolution Spectrograph was a highly sensitive ultraviolet spectrograph aboard the Hubble Space Telescope used to study the composition, temperature, and motion of astronomical objects.
- 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: Ultraviolet and Visual Echelle Spectrograph Target entity description: The Ultraviolet and Visual Echelle Spectrograph (UVES) is a high-resolution spectrograph mounted on ESO’s Very Large Telescope, used to obtain detailed spectra of astronomical objects in the ultraviolet and visible wavelength ranges.
-
A.
Ultraviolet Spectrometer
The Ultraviolet Spectrometer was a scientific instrument on the Galileo spacecraft used to analyze ultraviolet light from celestial objects to study their composition, atmospheres, and energy processes.
-
B.
Ultraviolet Imaging Spectrograph (UVS)
The Ultraviolet Imaging Spectrograph (UVS) is a scientific instrument that observes ultraviolet light to study the composition, structure, and dynamics of Jupiter’s atmosphere and auroras.
-
C.
Europa Ultraviolet Spectrograph
The Europa Ultraviolet Spectrograph is a scientific instrument designed to study Europa’s tenuous atmosphere, surface composition, and space environment by analyzing ultraviolet light during NASA’s Europa Clipper mission.
-
D.
DEIMOS spectrograph
The DEIMOS spectrograph is a powerful multi-object optical spectrograph designed for wide-field, high-resolution spectroscopy of faint astronomical sources.
-
E.
Goddard High Resolution Spectrograph
The Goddard High Resolution Spectrograph was a highly sensitive ultraviolet spectrograph aboard the Hubble Space Telescope used to study the composition, temperature, and motion of astronomical objects.
- F. None of above. chosen
Statements (43)
| Predicate | Object |
|---|---|
| instanceOf |
VLT instrument
ⓘ
astronomical spectrograph ⓘ echelle spectrograph ⓘ |
| abbreviation | UVES NERFINISHED ⓘ |
| acronym | UVES NERFINISHED ⓘ |
| capability |
detailed chemical abundance analysis
ⓘ
exoplanet host star characterization ⓘ high spectral resolution ⓘ interstellar medium studies ⓘ quasar absorption line spectroscopy ⓘ radial velocity measurements ⓘ stellar spectroscopy ⓘ |
| country | Chile ⓘ |
| dataArchive | ESO Science Archive Facility NERFINISHED ⓘ |
| dataProduct | high-resolution spectra ⓘ |
| fullName | Ultraviolet and Visual Echelle Spectrograph NERFINISHED ⓘ |
| hostFacility | ESO Paranal Observatory NERFINISHED ⓘ |
| locatedOnTelescope | Very Large Telescope NERFINISHED ⓘ |
| mountedOn | UT2 Kueyen NERFINISHED ⓘ |
| observatory | ESO Very Large Telescope NERFINISHED ⓘ |
| observatoryLocation | Cerro Paranal NERFINISHED ⓘ |
| observatorySite | Paranal Observatory NERFINISHED ⓘ |
| operator | European Southern Observatory NERFINISHED ⓘ |
| organization | ESO NERFINISHED ⓘ |
| partOf | ESO VLT instrumentation suite NERFINISHED ⓘ |
| primaryUse | high-resolution spectroscopy of astronomical objects ⓘ |
| scienceFocus |
high-redshift quasars
ⓘ
interstellar absorption systems ⓘ metal-poor stars ⓘ planet-hosting stars ⓘ |
| scientificDomain |
astronomy
ⓘ
astrophysics ⓘ |
| spectralCoverage | near-ultraviolet to red optical ⓘ |
| spectrographType | cross-dispersed echelle ⓘ |
| telescopeAperture | 8.2-metre unit telescope ⓘ |
| usedBy | international astronomical community ⓘ |
| usedFor |
measurements of fundamental physical constants variation tests
ⓘ
precision measurements of spectral line profiles ⓘ studies of chemical evolution of galaxies ⓘ studies of stellar atmospheres ⓘ studies of the intergalactic medium ⓘ |
| wavelengthRange |
ultraviolet
ⓘ
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: Ultraviolet and Visual Echelle Spectrograph Description of subject: The Ultraviolet and Visual Echelle Spectrograph (UVES) is a high-resolution spectrograph mounted on ESO’s Very Large Telescope, used to obtain detailed spectra of astronomical objects in the ultraviolet and visible wavelength ranges.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.