A High Sensitivity Fourier Transform Spectrometer for Cosmic Microwave Back-ground Observations
The QUIJOTE Experiment was developed to study the polarization in the Cosmic Microwave Background (CMB) over the frequency range of 10-50 GHz. Its first instrument, the Multi-Frequency-Instrument (MFI), measures in the range 10-20 GHz which coincides with one of the naturally transparent windows in the atmosphere. The Tenerife Microwave
de Miguel-Hernández, J. et al.
Advertised on:
10
2019