At a Glance: Allen Telescope Array (ATA)

  • The ATA is the first radio telescope designed specifically for SETI (search for extraterrestrial intelligence) research.
  • Located at Hat Creek Radio Observatory in northern California (about 300 miles north of San Francisco and just north of Lassen Peak).
  • Consists of 42 antennas (each 6 m in diameter) in current form, capable of simultaneous use for both SETI and advanced radio-astronomy research. 
  • Operates over a wide frequency range (~1–14 GHz), allowing observation of large swaths of sky and enabling dedicated SETI time rather than being secondary to other astronomy projects. 
  • Past observing programs include:
    • Targeting star systems identified by Kepler Space Telescope (especially those in habitable-zone candidate planets).
    • Surveying a region near the Milky Way’s Galactic Center (where stellar density is highest) for potential signals/beacons.
    • Focusing on nearby “habitable” stars (within ~1,000 light-years) as part of a legacy extending from Project Phoenix (1995–2004).
    • Investigating signals from the interstellar object ‘Oumuamua and from the direction of the famous 1977 “Wow! signal.”
  • The ATA recently underwent an upgrade with more sensitive receivers and expanded capabilities, enabling new SETI observing programs leveraging improved hardware. 
  • While not the world’s largest radio array, its design emphasizes wide field-of-view, dedicated SETI time, and flexibility—key strengths that distinguish it from other instruments. 

Science

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.

Illustration of a pulsar. Credit: NASA/JPL-Caltech.

Technical

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.

 

Antonio Feed inside an ATA Dish. Credit: SETI Institute

Quad-Ridge Feed Horn installation inside an ATA Dish. Credit: Jay Frothingham, SETI Institute

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!

Image Credit: Alex Pollak

Image Credit: Alex Pollak

Learn More and Get Involved

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Visit the ATA

Want to learn more about the ATA? Visit the telescope itself by going to the Hat Creek Radio Observatory! 

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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.

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Technical

Want to know more of the technical nitty-gritty about how the telescope works? Check out the Hat Creek Radio Observatory website.

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Student Programs

Want to get involved in a college student program? Check out ARISE and the SETI Institute REU.

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Follow Us

Want to keep up with our latest results? Sign up for the SETI Institute mailing list or follow us on Social Media!

News & Events

ATA News

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Jul 20, 2026
SETI Institute In the News: June Roundup 2026
Throughout June 2026, SETI Institute scientists, affiliates, and collaborators contributed to discussions spanning interstellar visitors, planetary science, technosignature searches, animal cognition, and the scientific process guiding the search for life beyond Earth. #SETI Institute in the News #SETI Institute #Community #Eduardo Bendek #Optical SETI #SETI #3I/ATLAS #ATA #Comets, Meteors, and Asteroids #Solar System #Franck Marchis #Ariel Graykowski #Jill Tarter #Vishal Gajjar #Radio Astronomy #Bill Diamond #Lori Marino
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Jun 3, 2026
SETI Institute Looks for Signs of Technology in Interstellar Visitor 3I/ATLAS
Observations with the Allen Telescope Array set new limits on possible signals from extraterrestrial transmitters. #Press Releases #ATA #3I/ATLAS #Hat Creek Radio Observatory #Radio Astronomy #SETI
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Apr 30, 2026
Narrowing the Search: The 45 Best Targets for Alien Life
#Blog #Astronomy #JWST #NASA Missions and Observatories #Trappist-1 #LaserSETI #ATA #Franck Marchis

 

 

Video

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!