Hydrogen Line Observations using the EAARO Microwave Detector
The hydrogen line (1420.40575 MHz) is the precession frequency of neutral hydrogen atoms, the most abundant substance in space.
Hydrogen line radiation is great for observing the structure of the universe, and some of the best and most detailed Milky Way radio maps have been made on the hydrogen line. It is probably the world's most popular radio astronomy frequency, and the International Telecommunications Union (ITU) has the good sense to protect it.
In 1959 two scholars (Philip Morrison at Cornell University and Frank Drake at NRAO) independently recognized that the hydrogen line would be a likely frequency for interstellar beacons. They reasoned that more advanced civilizations would reason that young civilizations (like ours) might already be listening there. Based upon that circular reasoning, Morrison went on to co-author the world's first modern SETI article ("Searching for Interstellar Communications," Nature 184(4690):844-846, September 19, 1959), and Drake conducted a the first modern SETI study, "Project Ozma," a hydrogen line search of two nearby Sun-like stars for possible artificial signals.
Over the past forty years, about three dozen other hydrogen line searches have been conducted. It was on the hydrogen line that in 1977 the Big Ear radio telescope at the Ohio State Radio Observatory detected the so-called "Wow!" signal, the most promising, intriguing and beguiling SETI candidate signal to date. The "Wow!" is also the best known SETI signal, having been featured in the "X-files." After about 100 follow-up attempts over a twenty year period, that signal has never repeated and remains unexplained..
EAARO will be using Hydrogen Line Observations both to map the distribution of hydrogen throughout the galaxy to build an image of our galaxy (the Milky Way) and to listen for signs of advanced civilisations that may be using this frequency band to transmit signals.
EAARO will be recording and logging this data which will be made available to the scientific community.