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Puntino - Wavefront sensor based on the Shack-Hartmann principle that can be used to test a single focal ratio telescope or optical element.
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 Technical Specifications of Puntino Wavefront Sensor 
Feature Specification
Type of element that can be measured Astronomical telescopes (at Cassegrain, Prime and Newtonian focus). Telescopes in the laboratory. Lenses in external illumination
Focal ratios covered f/1.8 to f/300 standard. Faster focal ratios can be tested with special setup
Diameter of optical element that can be tested Practically any diameter
Diameter of lenslets 0.3 mm
Focal length of lenslets 41 mm
Standard sampling on the pupil About 26 x 26 spots
Maximum sampling Up to 70 x 70 spots can be used (camera dependent)
Analysis Software Sensoft
Precision of Zernike polynomials coefficients (laboratory) λ/300
Precision of Zernike polynomials coefficients (telescope) 0.01 "
Precision with which the wavefront is computed λ/150 rms
Wavelength range With standard camera from 0.375 μ up to 1.1 μ. With IR camera up to 2 μ
Reference source LED with cooled camera. Remotely controlled
Distance from flange to instrument focus 54.8 mm
Height of optical axis from base 61.5 mm
Camera for SH 16-bit cooled CCD
Camera for finder 10-bit uncooled CMOS, 1280 x 1024 pixels, 7.5 μ pixel size or 14 or 16-bit cooled CCD
Dimensions (depends from focal ratios tested) 9 (Height) x 22 (Length) x 9 (Width) cm
Power requirement (stepper motor) 12V, 500 mA
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