UCLES spectrograph
E653632
The UCLES spectrograph is a high-resolution echelle spectrograph used on the Anglo-Australian Telescope for precise radial-velocity measurements and exoplanet detection.
All labels observed (1)
| Label | Occurrences |
|---|---|
| UCLES spectrograph canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T7272891 — 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.
Target entity: UCLES spectrograph Context triple: [Tau Ceti f, detectionInstruments, UCLES spectrograph]
-
A.
Boller and Chivens spectrograph
The Boller and Chivens spectrograph is an astronomical instrument designed for dispersing and analyzing light from celestial objects to study their physical and chemical properties.
-
B.
iSHELL spectrograph
The iSHELL spectrograph is a high-resolution infrared spectrograph used for detailed astronomical observations, such as studying planetary atmospheres and small bodies in the solar system.
-
C.
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.
-
D.
OSIRIS spectrograph
The OSIRIS spectrograph is a near-infrared integral field spectrograph and imager used on large telescopes to obtain detailed spatial and spectral information from astronomical objects.
-
E.
LRIS spectrograph
The LRIS spectrograph is a powerful optical imaging and multi-object spectrograph used on one of the Keck telescopes for detailed astronomical observations across a wide wavelength range.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: UCLES spectrograph Target entity description: The UCLES spectrograph is a high-resolution echelle spectrograph used on the Anglo-Australian Telescope for precise radial-velocity measurements and exoplanet detection.
-
A.
Boller and Chivens spectrograph
The Boller and Chivens spectrograph is an astronomical instrument designed for dispersing and analyzing light from celestial objects to study their physical and chemical properties.
-
B.
iSHELL spectrograph
The iSHELL spectrograph is a high-resolution infrared spectrograph used for detailed astronomical observations, such as studying planetary atmospheres and small bodies in the solar system.
-
C.
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.
-
D.
OSIRIS spectrograph
The OSIRIS spectrograph is a near-infrared integral field spectrograph and imager used on large telescopes to obtain detailed spatial and spectral information from astronomical objects.
-
E.
LRIS spectrograph
The LRIS spectrograph is a powerful optical imaging and multi-object spectrograph used on one of the Keck telescopes for detailed astronomical observations across a wide wavelength range.
- F. None of above. chosen
Statements (30)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical spectrograph
ⓘ
echelle spectrograph ⓘ |
| associatedWith |
Anglo-Australian Observatory
NERFINISHED
ⓘ
Australian Astronomical Observatory NERFINISHED ⓘ |
| contributedTo | discovery and characterization of exoplanets around nearby stars ⓘ |
| hasCapability |
broad optical wavelength coverage
ⓘ
high spectral resolution ⓘ high-precision radial velocities ⓘ |
| hasDesign | cross-dispersed echelle ⓘ |
| hasInstrumentClass | high-resolution optical spectrograph ⓘ |
| hasSpectralType | high-resolution ⓘ |
| locatedAt | Anglo-Australian Telescope NERFINISHED ⓘ |
| locatedIn |
Australia
ⓘ
New South Wales ⓘ Siding Spring Observatory NERFINISHED ⓘ |
| mountedAt | Coudé focus of the Anglo-Australian Telescope NERFINISHED ⓘ |
| observatoryType | optical ⓘ |
| operatedBy | Anglo-Australian Telescope facility NERFINISHED ⓘ |
| supportsTechnique | Doppler radial-velocity method ⓘ |
| telescopeAperture | 3.9-metre ⓘ |
| usedFor |
chemical abundance studies
ⓘ
exoplanet detection ⓘ precise radial-velocity measurements ⓘ stellar spectroscopy ⓘ time-series spectroscopy ⓘ |
| usedIn |
Galactic chemical evolution studies
ⓘ
binary star orbit determinations ⓘ exoplanet radial-velocity surveys ⓘ studies of stellar oscillations ⓘ |
| usedOn | Anglo-Australian Telescope NERFINISHED ⓘ |
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.
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.
Subject: UCLES spectrograph Description of subject: The UCLES spectrograph is a high-resolution echelle spectrograph used on the Anglo-Australian Telescope for precise radial-velocity measurements and exoplanet detection.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.