Fast Facts

The Argus Array forms an 8m-class array of 1200 telescopes providing 1.0 arcsec resolution across an 8,000 square degree field of view in every exposure. Taking images every 1 to 60 seconds, and stacking them to depths comparable to those of the deepest sky surveys, Argus will capture a continuous two-color, 120-gigapixel movie of the night sky. Argus's data will be shared with the world in real-time through public transient alerts, images, and light curves with millions of epochs for tens of millions of stars. Argus is under construction at a Northern Hemisphere site and planned to be completed in 2027.

System Parameters

Instrument
Field of View 8000 sq. deg
Nightly Coverage 21,000 sq. deg
Effective Aperture Diameter 8 meters
Single Telescope Aperture 0.28 meters
Detectors 1,200 Sony IMX461ALR
Image Size 120 GPix
Pixel Scale 1.0 arcsec / pixel
Read noise 1.4e-
Duty Cycle 94% (<1 ms dead time between exposures)
Bandpasses TBD, but likely dual band, b: 365-525 nm, r: 560-700 nm
Tracking 15 minute intervals, followed by 50 second reset
Survey & Data
Survey Length 5 year survey planned; 20 year design lifetime
Observing Cadence 1 minute (gray and dark time), 1 second (bright time)
Epochs ~20,000,000 (1s cadence, all Northern sky regions), ~300,000 (1-minute cadence, all Northern sky regions)
Delivered Image Quality 2 arcsec FWHM
Data Pipeline
Analysis Real-time image subtraction and transient detection with compression for offline analysis
Storage 107 targets and transient stamps at full cadence, full resolution coadds at 15-minute cadence and slower
Public Release All imaging and photometric data public, with real-time alerts from all cadences
Limiting Magnitudes (g-band, 5σ, dark time)
Cadence Design Goal Science Requirement Sky Area / epoch
1 second 17.1 16.8 8000 sq. deg
1 minute 20.5 20.0 8000 sq. deg
15 minute 22.1 21.5 8000 sq. deg
1 hour 22.9 22.3 9600 sq. deg
1 night 23.9 23.2 21000 sq. deg
7 nights 24.7 24.1 22500 sq. deg
6 months 26.5 29650 sq. deg