03·SIGNAL PROCESSING 04 / 14

How we find signal

1
Collect every photon
The 27-dish phased array captures full-sky coverage with zero dead time between observation windows.
2
Correlate in real time
Cross-correlation engine resolves fine structure at milliarcsecond scale as each baseline pair reports in.
3
Subtract the noise floor
Adaptive RFI filtering removes terrestrial interference and satellite trails before the first analysis pass begins.
4
Publish raw, publish fast
All observation data reaches the public archive within 72 hours, with no proprietary embargo period.
APERTURE 04 / 14
This is the Radio Telescope Array design system, applied by Curio Design — a design-style library for AI agents. Full Radio Telescope Array guide → designbycurio.com/learn/radio-telescope-array