Here's a breakdown:
* Horn antenna: This was the primary tool. It was a large, 20-foot diameter horn antenna designed for communication with satellites. Its sensitivity allowed them to detect faint radio signals coming from all directions.
* Radiometer: They used a highly sensitive radiometer connected to the antenna. This device measured the intensity of radio waves coming from the sky.
* Calibration: They carefully calibrated their equipment to eliminate any potential sources of noise from the antenna itself or other known sources.
* Sky observations: They observed the sky at different times and directions to rule out any possible sources of the persistent background noise.
Their discovery was unintentional - they stumbled upon the cosmic background radiation while trying to eliminate noise in their antenna. This "noise" turned out to be the faint afterglow of the Big Bang, a groundbreaking discovery that revolutionized our understanding of the universe.