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Optical measurement equipment Wavefront aberration measurement equipment SH sensor for astronomical telescopes PUNTINO-PUNTINO
Optical measurement equipment Wavefront aberration measurement equipment SH sensor for astronomical telescopes PUNTINO-Asahiko Trading Co., Ltd.

Optical measurement equipment Wavefront aberration measurement equipment SH sensor for astronomical telescopes PUNTINO
Asahiko Trading Co., Ltd.

Asahiko Trading Co., Ltd.'s Response Status

Response Rate

100.0%

Response Time

21.8hours

Relatively Fast Response


About This Product

■Summary

The PUNTINO SH sensor for astronomical telescopes provided by Spot Optics is used for evaluating the optical system of astronomical telescopes, alignment, and Strehl ratio evaluation.

■Features

・High dynamic range ・Wavefront analysis compatible with all optical aberrations ・The correction direction and size (mm) can be determined by the diagnostic program. ・Able to align optical components of astronomical telescopes ・Dedicated software for image acquisition and analysis Sensoft ・Discovering the correct focal plane from the analyzed spherical aberration ・Identification of air fluctuations by remaining spot analysis ・Online monitoring of how aberrations change at night ・Checking the correlation of aberration fluctuations due to temperature changes

■Accessories

The wavefront sensor is supplied with accessories useful for measurements. ・External calibration unit Cal25 ・External electric calibration unit ECM25 ・External calibration pinhole light source PH50 ・Beam expander/beam compressor BE25, BE60 and BE120 ・Standard light source with mounting ・Flat mirror with mounting ・Objective lens ・Optical element mounting mount ・Electric stage

■Application

astronomical telescope

■Optimize telescope performance with powerful tools

A finely tuned telescope is the key to obtaining deep, high-quality astronomical images. Developed specifically for telescopes, the Shack-Hartmann wavefront sensor Puntino is based on extensive experience in use in observatories around the world. Complete analysis of optics, mechanics, mirror supports, mirrors, and dome seeing. Based on the analysis results, the software recommends corrective actions to be taken, greatly simplifying maintenance tasks and completing normally time-consuming tasks in a matter of hours. Based on our philosophy of providing a complete set of tools, we also offer CCD-based systems for alignment telescopes and autocollimators.

  • Product

    Optical measurement equipment Wavefront aberration measurement equipment SH sensor for astronomical telescopes PUNTINO

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1 Models of Optical measurement equipment Wavefront aberration measurement equipment SH sensor for astronomical telescopes PUNTINO

Image Part Number Price (excluding tax) Analysis software Standard sampling of pupils Wavefront calculation accuracy Wavelength range Maximum sampling Power requirements (stepping motor) Target focal ratio Dimensions (depending on focal ratio) Reference light source Lenslet focal length Optical axis height from base Distance from flange to device focus Finder camera Types of elements that can be tested Accuracy of Zernike polynomial coefficients (telescope) Accuracy of Zernike polynomial coefficients (laboratory) Camera for SH
Optical measurement equipment Wavefront aberration measurement equipment SH sensor for astronomical telescopes PUNTINO-Part Number-PUNTINO

PUNTINO

Available upon quote

SenSoft

Approximately 40×40

Λ/150rms

From 0.375 to 1.1μ with standard camera

Maximum 65 x 65 spots (depending on camera)

12V, 1,000mA

F/1.8 to f/300 is standard. Faster focal ratios can be tested with special setups.

9 (height) × 22 (length) × 9 (width) cm

LED. Remote control possible

41mm

51.5mm

54.8mm

10-bit uncooled CMOS, 1,280 x 1,024 pixels, 5.4μ pixels
size or 14 or 16 bit cooled CCD

Astronomical telescope (Cassegrain type, prime focus type, Newtonian focus type).
Laboratory telescope, lens

0.01

Λ/300

16-bit cooled CCD

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About Company Handling This Product

Response Rate

100.0%


Response Time

21.8hrs

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