Altair Deep Space Array is an automated synthetic aperture radio interferometer and photometric survey station. Operating in direct synchronization with our optical sister station, Starlight Observatory (UPUP6).
Continuous monitoring of galactic neutral hydrogen and high-energy astrophysical events.
Mapping the rotation curve and spiral structure of the Milky Way galaxy by measuring Doppler shift in the 1420.405 MHz emission line.
Read Survey Findings →Sub-millisecond real-time digital beamforming buffer searching for millisecond-duration extragalactic radio pulses.
View Transient Catalog →Precision Doppler tracking and signal decoding for interplanetary scientific probes and cubesat constellations.
Inspect Array Specs →