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 | 
                                    
            





					
                        
					
                        
					
                        
					
                        
					
                        
					
                        