|
gptkb:Triboluminescence
|
Visible light
|
|
gptkb:Rosetta_OSIRIS_camera
|
250–1000 nm
|
|
gptkb:Fabry-Perot_Laser
|
gptkb:Infrared
|
|
gptkb:Mars_Color_Imager_(MARCI)
|
ultraviolet to visible
|
|
gptkb:IRAS_catalogue
|
100 microns
|
|
gptkb:1000BASE-LH
|
1550 nm
|
|
gptkb:Incandescence
|
Infrared to visible light
|
|
gptkb:SPHERE_instrument
|
near-infrared
|
|
gptkb:Chandra
|
0.1–10 keV
|
|
gptkb:ALMA_Observatory,_Chile
|
submillimeter
|
|
gptkb:blue_noise
|
higher frequencies dominate
|
|
gptkb:Spektr-R
|
1.35 cm to 92 cm
|
|
gptkb:VCSEL
|
near-infrared
|
|
gptkb:Parkes_Catalogue
|
5 GHz
|
|
gptkb:Spectro-Polarimetric_High-contrast_Exoplanet_REsearch
|
near-infrared
|
|
gptkb:Composite_Infrared_Spectrometer_(CIRS)
|
7 to 1000 micrometers
|
|
gptkb:Visible_spectrum
|
400 THz to 790 THz
|
|
gptkb:Wide_Field_Channel
|
visible light
|
|
gptkb:Near_Infrared_Spectrograph
|
0.6 to 5 micrometers
|
|
gptkb:Violet
|
380–450 nm
|