Ideal platform for wide field imaging!The UWF1000 f1.3 telescope is the ideal platform for wide field imaging and all-sky surveys. The UWF1000 f1.3 features a highly aspheric 5-lens corrector and motorized focusing with absolute encoders. The main mirror and the corrector can be collimated fully electronic to allow an easy and fast remote collimation. UWF1000 f1.3 Optical LayoutThe UWF1000 uses a prime focus configuration. The main mirror is a high order asphere and in the prime focus we use a highly aspheric 5 Lens corrector to correct any field aberrations in a wavelength range from 400nm to 700nm. Only with these latest technological advances in optical design (aspherical surfaces, ED glasses), we could combine such a wide field with this short focal ratio. ==> See full UWF1000 F1.3 Report!
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Main Facts |
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Optical design
Ultra Wide Field, prime corrector Focal length
1300mm Clear Aperture / Focal Ratio Primary Mirror
1000mm (39.3 inch) / f1.3 Mirror material
Fused silica Surface quality
>80 strehl Coating
Al+SiO2 >96% Weight tube
1900kg (4189lbs) (no camera or filter) Latitude Range
20 to 80 degrees views Max. slew speeds
Up to 50 degrees per second Tracking Accuracy (20° to 85°)
<0,25” RMS within 5 minutes tracking time over 5 min 0,05” RMS/min |
Linear central obstruction
48% Focal ratio system
f1.3 Image field
84mm (3.70 degrees) Image Quality FWHM
<4um RMS Microroughness
1.3nm RMS / <0.7nm Ra Back Focus from flange
81mm Motor
ASA Direct Drive Software
ASA API (application programming interface) available autumn 2023 ASA Software(Autoslew, Sequence-windows based, ACC) with ASCOM-Alpaca Pointing Accuracy (20° to 85°)
<8” RMS with pointing model and ASA telescope System Natural Frequency
10 Hz or greater |
ASA Accessories |
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Remote package pro | Weather station sensor package | All Sky Cam 0201171A |