Kast double spectrograph
E716454
The Kast double spectrograph is an astronomical instrument used at Lick Observatory to obtain detailed spectra of celestial objects across two wavelength ranges simultaneously.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Kast double spectrograph canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T8178603 — 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: Kast double spectrograph Context triple: [Lick Observatory, hasInstrument, Kast double 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.
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B.
SpeX spectrograph
The SpeX spectrograph is a near-infrared spectrograph and imager used for astronomical observations, particularly of planets, stars, and small bodies in the solar system.
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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.
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.
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E.
Grille spectrometer
The Grille spectrometer is a spaceborne infrared spectrometer designed to study the composition and structure of planetary and Earth atmospheres by analyzing their emitted and absorbed radiation.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Kast double spectrograph Target entity description: The Kast double spectrograph is an astronomical instrument used at Lick Observatory to obtain detailed spectra of celestial objects across two wavelength ranges simultaneously.
-
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.
SpeX spectrograph
The SpeX spectrograph is a near-infrared spectrograph and imager used for astronomical observations, particularly of planets, stars, 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.
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.
-
E.
Grille spectrometer
The Grille spectrometer is a spaceborne infrared spectrometer designed to study the composition and structure of planetary and Earth atmospheres by analyzing their emitted and absorbed radiation.
- F. None of above. chosen
Statements (45)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical spectrograph
ⓘ
double spectrograph ⓘ optical instrument ⓘ |
| associatedWithInstitution | University of California, Santa Cruz NERFINISHED ⓘ |
| capability | simultaneous two-arm spectroscopy ⓘ |
| country |
United States of America
ⓘ
surface form:
United States
|
| dataFormat | digital CCD spectra ⓘ |
| dataProduct | optical spectra ⓘ |
| designedFor | optical spectroscopy of astronomical objects ⓘ |
| detectorType |
CCD detector on blue arm
ⓘ
CCD detector on red arm ⓘ |
| feature |
dichroic beam splitter
ⓘ
multiple grisms and gratings ⓘ slit spectrograph design ⓘ |
| hasComponent |
blue arm
ⓘ
red arm ⓘ |
| locatedAt | Lick Observatory NERFINISHED ⓘ |
| mountType | Cassegrain focus instrument ⓘ |
| namedAfter | Reinhard Kast NERFINISHED ⓘ |
| notableFor | simultaneous blue and red spectral coverage ⓘ |
| observatoryCode | LICK NERFINISHED ⓘ |
| observatoryLocation | Mount Hamilton, California NERFINISHED ⓘ |
| observatoryOperatedBy | University of California Observatories NERFINISHED ⓘ |
| observingMode | long-slit spectroscopy ⓘ |
| operationalStatus | in use for optical spectroscopy at Lick Observatory ⓘ |
| scienceField |
astrophysics
ⓘ
observational astronomy ⓘ |
| scientificContribution |
spectroscopic surveys of galaxies
ⓘ
studies of Type Ia supernovae ⓘ studies of core-collapse supernovae ⓘ |
| scientificUse |
active galactic nucleus spectroscopy
ⓘ
galaxy spectroscopy ⓘ quasar spectroscopy ⓘ stellar spectroscopy ⓘ supernova spectroscopy ⓘ |
| spectralResolution | moderate resolution optical spectroscopy ⓘ |
| telescopeAperture | 3-meter ⓘ |
| usedFor |
classification of supernovae
ⓘ
follow-up of transient astronomical events ⓘ measurement of absorption line properties ⓘ measurement of emission line properties ⓘ measurement of redshifts ⓘ |
| usedOnTelescope | Shane 3-meter telescope NERFINISHED ⓘ |
| wavelengthCoverage |
blue optical wavelengths
ⓘ
red optical wavelengths ⓘ |
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: Kast double spectrograph Description of subject: The Kast double spectrograph is an astronomical instrument used at Lick Observatory to obtain detailed spectra of celestial objects across two wavelength ranges simultaneously.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.