Ideal platform for widefield imaging!The WF1000 f2.5 telescope is the ideal platform for wide field imaging and all-sky surveys. The WF1000 f2.5 features a 5-lens corrector and motorized focusing with absolute encoders. UWF1000 f2.5 Optical LayoutThe UWF1000 uses a prime focus configuration. The main mirror is a high order asphere and in the prime focus we use a 5 Lens corrector to correct any field aberrations in a wavelength range from 400nm to 700nm. This prime focus telescope achieves the large field through a larger possible field diameter, enabling the usage of the largest available CCD/CMOS cameras with up to 95x95mm2 sensor size. ==> See full UWF1000 F2.5 Report!
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Main Facts |
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Optical design
Wide Field, prime corrector Focal length
2500mm Clear Aperture / Focal Ratio Primary Mirror
1000mm (39.3 inch) / f2.5 Mirror material
Fused silica Surface quality
>80 strehl Coating
Al+SiO2 >96% Weight tube
1950kg (4300lbs) (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
42% Focal ratio system
f2.5 Image field
130mm (2.98 degrees) Image Quality FWHM
<8um RMS Microroughness
1.3nm RMS / <0.7nm Ra Back Focus from flange
100.88mm 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 |