Gravitational lensing is a powerful astrophysical and cosmological probe and is particularly valuable at
submillimeter wavelengths for the study of the statistical and individual properties of dusty star - forming galaxies.
Not exact matches
This site provides the exceptionally dry atmospheric conditions necessary
for astronomical observations at millimeter and
submillimeter wavelengths (
wavelengths between the radio and far - infrared spectral regions).
With these high - precision components, ALMA will open up new possibility
for observations with surprisingly high resolution at
submillimeter wavelengths, which will make a great contribution to the study of the formation of galaxies and planetary systems as well as the evolution of interstellar matters.