Abstract:
We developed a tip-tilt system to compensate the turbulence induced image motion for the 1.3 m
telescope at Vainu Bappu Observatory, at Kavalur. The instrument is designed to operate at the visible
wavelength band (480−700 nm) with a field of view of 1 ′×1′. The tilt corrected images have demonstrated
up to ≈ 57% improvement in image resolution and a corresponding peak intensity increase by a factor of
≈ 2.8. A closed-loop correction bandwidth of ≈ 26 Hz has been achieved with on-sky tests and the root
mean square motion of the star image has been reduced by a factor of ∼ 14. These results are consistent
with theoretical and numerical predictions of wave-front aberrations caused by atmospheric turbulence and
image quality improvement expected from a real-time control system. In this paper, we present details of
the instrument design, laboratory calibration studies and quantify its performance on the telescope.
