|
gptkb:Visible_and_Infrared_Mapping_Spectrometer
|
up to 352 channels
|
|
gptkb:Spectro-Photometer_for_the_History_of_the_Universe,_Epoch_of_Reionization,_and_Ices_Explorer
|
R=35-130
|
|
gptkb:International_Ultraviolet_Explorer
|
0.1 to 0.6 nm
|
|
gptkb:CrIS
|
0.625 cm⁻¹
|
|
gptkb:Cosmic_Origins_Spectrograph
|
gptkb:medium
|
|
gptkb:IASI
|
0.5 cm⁻¹
|
|
gptkb:Apollo_16_Far_Ultraviolet_Camera/Spectrograph
|
2 angstroms
|
|
gptkb:TANSO-FTS
|
0.2 cm-1
|
|
gptkb:Infrared_Atmospheric_Sounding_Interferometer_(IASI)
|
0.5 cm⁻¹
|
|
gptkb:Far_Infrared_Absolute_Spectrophotometer_(FIRAS)
|
high
|
|
gptkb:Wide_Field_Instrument
|
R~100 for prism, R~600 for grism
|
|
gptkb:Sloan_Digital_Sky_Survey
|
1800-2200
|
|
gptkb:MATISSE
|
up to 5000
|
|
gptkb:Cosmic_Origins_Spectrograph
|
high
|
|
gptkb:Atmospheric_Infrared_Ultraspectral_Sensor
|
ultraspectral
|
|
gptkb:Cosmic_Origins_Spectrograph
|
low
|
|
gptkb:Large_Sky_Area_Multi-Object_Fiber_Spectroscopic_Telescope_(LAMOST)
|
R~5000
|
|
gptkb:Cross-track_Infrared_Sounder_(CrIS)
|
high
|
|
gptkb:TES_(Thermal_Emission_Spectrometer)_on_Mars_Global_Surveyor
|
143 channels
|
|
gptkb:FLAMINGOS-2
|
R~1300 to 3000
|