Skip to main content

HartSCI ClearStar Adaptive Optics

Price:

Compare

Call for price

HartSCI’s ClearStar AO™ system represents a paradigm shift in high-resolution imaging. For the first time, high-performance image sharpening is available as an off-the-shelf product for small to mid-size professional telescopes. ClearStar AO™ overcomes atmospheric blurring to deliver diffraction-limited image quality to science instruments operating in the 750 – 1000 nm wavebands. Built-in hardware and software tools support full and automatic internal calibration. The system connects to the outside world through a simple ethernet port and comes with a full-featured browser-based graphical user interface that can be run on any computer.  ClearStarAO™ can also be controlled through an Application Programmers’ Interface (API), enabling fully automatic operation and seamless integration into the observatory environment.

Download our flyer

Specifications

Specifications

Correction speed 

Up to 1000 updates per second

Wavefront sensor

8×8 Shack-Hartmann

Actuator count 

45

Full-stroke tip-tilt control

±2 arcmin

Output focal ratio

f/12

External connectivity

Ethernet

Telescope mounting

Nasmyth port

Power draw

80 W

Weight

40 kg

Features

Features

  • Correction to the diffraction limit in 750 – 1000 nm waveband
  • Mates natively to PlaneWave CDK700, RC700, and PW1000 telescopes
  • Supports PlaneWave IRF90 instrument rotator/focuser
  • Customizable interface to other PlaneWave Instruments telescopes available
  • Diffraction-limited output beam delivers Nyquist-sampled images with common cameras
  • Built-in scoring/acquisition camera and calibration source
  • Customizable wavelength split between science and wavefront sensor channels
  • Automated target acquisition on wavefront sensor
  • Automated tracking error offload to telescope mount
  • Fiber coupling unit available (Q3 2022)

Benefits

Benefits

  • Breaks historical high-cost paradigm for high-order AO
  • Dollar for dollar the highest resolution and contrast for imaging and spectroscopy for meter-class telescopes
  • Eyes on sky within hours of delivery

Software

Software

  • Full-featured browser-based graphical user interface runs on any remote computer
  • Simple HTTP-based API offers full automation and seamless integration into observatory control systems (Q4 2022)
  • Built-in automated calibration functions
  • User-selectable recording of multiple full-speed telemetry streams to common HDF5 file format
X