Channel 37

Channel 37 is an unused television channel in countries using the M and N broadcast television system standards. Channel 37 occupies a band of UHF frequencies from 608 to 614 MHz, frequencies that are particularly important to radio astronomy because they allow observations at a frequency between the dedicated frequency allocations near 410 MHz and 1.4 GHz. One radio astronomy application in this band is for very-long-baseline interferometry.

Channel 37

Channel 37 is an unused television channel in countries using the M and N broadcast television system standards. Channel 37 occupies a band of UHF frequencies from 608 to 614 MHz, frequencies that are particularly important to radio astronomy because they allow observations at a frequency between the dedicated frequency allocations near 410 MHz and 1.4 GHz. One radio astronomy application in this band is for very-long-baseline interferometry.