The Q&U Bolometric Interferometer for Cosmology, that began in 2008 is located in Puna de Atacama and utilizes two frequencies of 150 as well as 220 gigahertz.
The Q&U Bolometric Interferometer for Cosmology, that began in 2008 is located in Puna de Atacama and utilizes two frequencies of 150 as well as 220 gigahertz.