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Next level high-end telescope system with 1.2m aperture. This complete solution represents a fully integrated alt-az observatory system. The AZ1200 1.2m is equipped with fused silica optics from ASA. This guarantees diffraction-limited performance and best micro-roughness values even under the most perfect Earth-based astronomical seeing conditions. With fast focal ratio, the design results in less obstruction, higher contrast, and a more compact system. The size and cost of your dome infrastructure is reduced. Main Facts
Optical design
Ritchey-Chrétien RC
Linear central obstruction
39%
Focus position
Nasmyth 2 as standard, 4 as option
Focal ratio system
f7.1
Clear Aperture / Focal Ratio Primary Mirror
1200mm (47,2 inch) / f2
Image field
150 mm (1.02 degrees)
Mirror material
Fused silica (option Zerodur)
Surface quality
>94 strehl
Microroughness
1nm RMS / <0.7nm Ra
Coating
Al+SiO2 >91%
Back Focus from flange
412mm
Total weight
4000kg (8819lbs)
Software
ASA Software package with a platform-independent Ascom Alpaca API (via TCP/IP), compatibility with numerous programs, and many additional API features for: • Creating and optimizing pointing files • MLPT (e.g., usable with a N.I.N.A plugin) • Uploading and tracking TLE and CPF satellite orbits • Orbit corrections when satellite tracking (autoguiding with external CCD cameras) • Focus control also via Ascom Alpaca API • Covers (if installed) via Ascom Alpaca API • Full API control over rotator, Nasmyth port
Pointing Accuracy (20° to 85°)
<8” RMS with pointing model
Tracking Accuracy (20° to 85° – unguided, with current pointingfile)
<0,25” RMS within 5 minutes
System Natural Frequency
10 Hz or greater |