spectralResolution
P7238
predicate
Indicates the fineness with which a system can distinguish or separate different wavelengths or frequencies within a spectrum.
All labels observed (8)
| Label | Occurrences |
|---|---|
| spectralResolution canonical | 47 |
| energyResolution | 3 |
| hasSpectralResolution | 3 |
| spectralResolutionMode | 2 |
| rearCameraSpectrumResolution | 1 |
| resolvingPower | 1 |
| spectralResolutionType | 1 |
| typicalEnergyResolution | 1 |
Description generation (PDg)
The one-sentence description above was generated by prompting gpt-5.1 with the predicate name and this instruction.
Instruction
Given a predicate that represents a relationship or action between entities, generate a one-sentence description explaining its meaning. # Instructions Focus on describing the relationship, not the entities themselves. # Response Format Begin the description with \' Indicates...\'
Input
Predicate: spectralResolution
Generated description
Indicates the fineness with which a system can distinguish or separate different wavelengths or frequencies within a spectrum.
Sample triples (59)
| Subject | Object |
|---|---|
|
Magellan Echellette Spectrograph
linked to:
Magellan Echellette Spectrograph (MagE)
|
R~4100 ⓘ |
| FIRE | moderate resolution ⓘ |
| MagE | medium ⓘ |
| Faint Object Spectrograph | low to medium resolution ⓘ |
| Cosmic Origins Spectrograph | medium resolution ⓘ |
| Cosmic Origins Spectrograph | low resolution ⓘ |
| Goddard High Resolution Spectrograph | high ⓘ |
| NIRSpec | R ~ 100 ⓘ |
| NIRSpec | R ~ 1000 ⓘ |
| NIRSpec | R ~ 2700 ⓘ |
|
NuSTAR
linked to:
NuSTAR Nuclear Spectroscopic Telescope Array
|
about 400 eV at 10 keV via predicate surface "energyResolution" ⓘ |
| HARPS spectrograph | about 115000 ⓘ |
| FEROS spectrograph | R ≈ 48,000 ⓘ |
| FLAMINGOS-2 | up to a few thousand ⓘ |
|
MIKE
linked to:
MIKE (Magellan Inamori Kyocera Echelle)
|
up to R ~ 65,000 depending on slit ⓘ |
| Silicon Drift Detector | better than 150 eV at 5.9 keV (for X-rays) via predicate surface "typicalEnergyResolution" ⓘ |
| UVES | up to about 110000 ⓘ |
| X-shooter | R ~ 4000–17000 ⓘ |
| IR G102 grism | low ⓘ |
| Far Ultraviolet Spectroscopic Explorer | high resolution ⓘ |
| ACE-FTS | high-resolution ⓘ |
| Far Ultraviolet Camera/Spectrograph | about 30 Å ⓘ |
| GHRS | high ⓘ |
| CES | high ⓘ |
| CES | high-dispersion via predicate surface "spectralResolutionType" ⓘ |
| Fiber-fed Extended Range Optical Spectrograph | high via predicate surface "hasSpectralResolution" ⓘ |
| FEROS | R≈48000 ⓘ |
| Dark Energy Spectroscopic Instrument | R ~ 2000–5000 ⓘ |
|
PRISMA
linked to:
PRISMA Earth observation mission
|
high spectral resolution ⓘ |
| Advanced CCD Imaging Spectrometer | spectroscopic-quality X-ray energy resolution via predicate surface "energyResolution" ⓘ |
| GRACES | up to R ~ 67,500 (approximate) ⓘ |
| GRACES | high-resolution mode via predicate surface "spectralResolutionMode" ⓘ |
| GRACES | medium-resolution mode via predicate surface "spectralResolutionMode" ⓘ |
|
GNIRS
linked to:
GNIRS (Gemini Near-Infrared Spectrograph)
|
high-resolution capability ⓘ |
|
GNIRS
linked to:
GNIRS (Gemini Near-Infrared Spectrograph)
|
medium-resolution capability ⓘ |
|
GNIRS
linked to:
GNIRS (Gemini Near-Infrared Spectrograph)
|
low-resolution capability ⓘ |
| FLAMINGOS | moderate ⓘ |
| TANSO-FTS | high ⓘ |
| IGRINS | R ~ 45,000 ⓘ |
| PACS | medium spectral resolution in far-infrared ⓘ |
|
CRISM
linked to:
CRISM instrument
|
about 6.55 nanometers ⓘ |
| HDS | high ⓘ |
| ESPaDOnS | up to about 65,000 via predicate surface "resolvingPower" ⓘ |
| SITELLE | adjustable spectral resolution ⓘ |
| HIRES spectrograph | high via predicate surface "hasSpectralResolution" ⓘ |
| DEIMOS spectrograph | high ⓘ |
| iSHELL spectrograph | R ~ 70,000 ⓘ |
| CRISM | ~6.55 nanometers ⓘ |
| Low Dispersion Survey Spectrograph 3 | low ⓘ |
| FOcal Reducer and low dispersion Spectrograph 2 | low ⓘ |