Visit the ATA
Want to learn more about the ATA? Visit the telescope itself by going to the Hat Creek Radio Observatory!
At a Glance: Allen Telescope Array (ATA)
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The Allen Telescope Array (ATA) is a radio telescope in Hat Creek, California that the SETI Institute uses to search for alien radio signals or "radio technosignatures." The ATA is made up of 42 individual dishes which all work together to collect radio waves from space, using a technique called interferometry. The ATA uses interferometry to make radio photographs of the sky (known as imaging), and also “zoom in” to particular regions to collect data from specific parts of the sky (known as beamforming).
The ATA’s primary science goal is to search for radio technosignatures, trying to better understand the prevalence of technologically-capable life in the galaxy and the universe. We search for technosignatures from known planetary systems, from places and times of particular interest (such as the ecliptic, the region of the sky where the Earth would be seen to block the Sun’s light once a year), and from targets that we follow-up from other studies that claim interesting astrobiological results.
Animation of a tidal disruption event. Credit: NASA, ESA, STScI, Ralf Crawford (STScI).
But, as a world-class radio telescope, the ATA can also be used to advance other frontiers in radio astronomy. The ATA has collected data to help us understand high-energy events like supernovae—where a high-mass star explodes at the end of its life—and tidal disruption events—where a star is ripped apart by a supermassive black hole. By combining data from the ATA and other telescopes around the world, we can better understand the physics in these extreme events that cannot be replicated in labs on Earth.
In addition, we use the ATA to study a range of fascinating astrophysical objects. The ATA has observed pulsars (the whirling cores of dead stars) and used them as a backlight to understand more about the gas and dust in our galaxy. We have detected flares from active stars in the Milky Way, and Fast Radio Bursts (FRBs) from far beyond the Milky Way, using the ATA to learn about objects and regions of space far more extreme than our own Solar System.
The ATA is a world-class telescope because of its clever technical design. A field with 42 radio dishes may not look like a telescope, but the ATA can be used to study the sky in much the same way as a traditional visible-light telescope where you can look through an eyepiece.
One reason that the ATA is so valuable for science is its “large number of small dishes” design. These dishes are small compared to other facilities—“only” 20 feet across— but they are mighty when they work together! When combined by the computers in the signal processing room, the dishes provide as many pixels on the sky as a dish that is 1000 feet across!
Another reason that the ATA is such a powerhouse is its custom wide-bandwidth feeds: the part of the telescope that actually receives the radio waves. The feeds are located at the focus point of the dish, collecting all of the radio waves that are reflected down to a single point. The ATA’s original Welch Feeds were a groundbreaking log-periodic pyramid design, which were eventually trimmed down and streamlined into the current Antonio Feeds. These feeds are special because they can capture radio waves over a huge range of frequencies at once, speeding up our search for potential alien signals. The feeds are very sensitive to very faint signals—even one feed alone could detect a cellphone if it was transmitting from the Moon! We are continuing our tradition of pioneering engineering at the Hat Creek Radio Observatory by working on a completely new feed design, the Quad-Ridge Feed Horn, which will amplify the existing benefits of the Antonio Feeds.
To support such a sophisticated and complex telescope, we need the world’s most sophisticated and complex computers. We use the most cutting-edge GPUs and other compute hardware to capture the immense amounts of data coming out of the telescope: our data-taking computers record the equivalent of 6 4k movies of data every second!
Learn More and Get Involved
Visit the ATA
Want to learn more about the ATA? Visit the telescope itself by going to the Hat Creek Radio Observatory!
SETI Science
Want to know more about the techniques that let us do the SETI science that we do? Check out our SETI 101 pages.
Technical
Want to know more of the technical nitty-gritty about how the telescope works? Check out the Hat Creek Radio Observatory website.
Student Programs
Want to get involved in a college student program? Check out ARISE and the SETI Institute REU.
Follow Us
Want to keep up with our latest results? Sign up for the SETI Institute mailing list or follow us on Social Media!
How SETI Designed A Telescope To Look For Extraterrestrial Civilizations
In 2025, we invited Scott Manley for a tour of the Allen Telescope Array in Hat Creek, CA. Take an in-depth look of the facilities and research happening at the Hat Creek Radio Observatory!