spectralResolution

P7238

predicate

Indicates the fineness with which a system can distinguish or separate different wavelengths or frequencies within a spectrum.

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All labels observed (8)

Label	Occurrences
spectralResolution canonical	47
energyResolution	3
hasSpectralResolution	3
spectralResolutionMode	2
rearCameraSpectrumResolution	1
resolvingPower	1
spectralResolutionType	1
typicalEnergyResolution	1

Sample triples (59)

Subject	Object
Magellan Echellette Spectrograph (MagE) surface form: Magellan Echellette Spectrograph	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 Nuclear Spectroscopic Telescope Array surface form: NuSTAR	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 (Magellan Inamori Kyocera Echelle) surface form: MIKE	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 Earth observation mission surface form: PRISMA	high spectral resolution ⓘ
Advanced CCD Imaging Spectrometer	spectroscopic-quality X-ray energy resolution via predicate surface "energyResolution" ⓘ
GRACES (Gemini Remote Access to CFHT ESPaDOnS Spectrograph) surface form: GRACES	up to R ~ 67,500 (approximate) ⓘ
GRACES (Gemini Remote Access to CFHT ESPaDOnS Spectrograph) surface form: GRACES	high-resolution mode via predicate surface "spectralResolutionMode" ⓘ
GRACES (Gemini Remote Access to CFHT ESPaDOnS Spectrograph) surface form: GRACES	medium-resolution mode via predicate surface "spectralResolutionMode" ⓘ
GNIRS (Gemini Near-Infrared Spectrograph) surface form: GNIRS	high-resolution capability ⓘ
GNIRS (Gemini Near-Infrared Spectrograph) surface form: GNIRS	medium-resolution capability ⓘ
GNIRS (Gemini Near-Infrared Spectrograph) surface form: GNIRS	low-resolution capability ⓘ
FLAMINGOS	moderate ⓘ
TANSO-FTS	high ⓘ
IGRINS	R ~ 45,000 ⓘ
PACS	medium spectral resolution in far-infrared ⓘ
CRISM instrument surface form: CRISM	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 ⓘ
Compact Reconnaissance Imaging Spectrometer for Mars surface form: CRISM	~6.55 nanometers ⓘ
Low Dispersion Survey Spectrograph 3	low ⓘ
FOcal Reducer and low dispersion Spectrograph 2	low ⓘ