Altitude 4,205m · Atacama Desert · −24.6° S
Beyond the visible horizon
A next-generation deep space observatory unlocking the faintest signals from the earliest epochs of the universe.
Deep Field Catalogue
Active targets under observation. Each object resolved with sub-arcsecond precision.
Rosette Nebula
Monoceros
Distance
5,200 ly
Magnitude
9.0
Andromeda Galaxy
Andromeda
Distance
2.537M ly
Magnitude
3.4
Pillars of Creation
Serpens
Distance
7,000 ly
Magnitude
6.0
Crab Nebula
Taurus
Distance
6,500 ly
Magnitude
8.4
The Array
Four precision instruments engineered to interrogate the universe at every wavelength.
The Aperture
Primary Optical Array
A 12-meter segmented mirror with adaptive optics, correcting atmospheric turbulence in real-time. Resolves objects 100,000 times fainter than the naked eye.
Spectral Forge
High-Resolution Spectrograph
Decomposes starlight into 350,000 individual wavelength channels. Reveals chemical composition, temperature, and radial velocity of distant objects.
Temporal Eye
Time-Domain Photometry Engine
Captures 10,000 frames per second to detect transient events — supernovae, gamma-ray bursts, exoplanet transits — the blink-and-you-miss-it universe.
Deep Field Array
Radio Interferometer Network
64 synchronized dish antennas spanning 12 kilometers. Synthesizes a virtual telescope capable of imaging the cosmic microwave background with sub-arcminute resolution.
Observatory Index
Light-Years Observed
Deepest survey
Exoplanets Catalogued
Since commissioning
Uptime
3 years continuous
Primary Mirror
Segmented adaptive
Mission Log
First light captured from exoplanet TOI-700 d atmosphere. Preliminary spectra suggest water vapor signatures at 1.4μm band.
Deep Field Array calibration complete. Baseline sensitivity improved 340% over previous configuration. Ready for CMB observation window.
Gravitational wave event GW260228 correlated with optical counterpart in NGC 4993. Multi-messenger astronomy milestone achieved.
Commissioned Temporal Eye upgrade. New CMOS sensor array reduces read noise to 0.7e⁻ RMS. Dark current: 0.001 e⁻/pixel/sec at -100°C.
The universe doesn't wait for you. But we'll help you catch up.
Join the next generation of discovery. Apply for observation time, access our public data archive, or sponsor a mission.
