Design, implementation, and on-sky performance of an advanced apochromatic triplet atmospheric dispersion corrector for the Magellan adaptive optics system and VisAO camera
Derek Kopon, Laird M. Close, Jared R. Males, and Victor Gasho

TL;DR
This paper details the design, laboratory testing, and on-sky performance of an advanced triplet atmospheric dispersion corrector for the Magellan adaptive optics system, significantly improving correction accuracy over conventional designs for visible wavelength astronomy.
Contribution
It introduces a novel triplet ADC design that enhances atmospheric dispersion correction, with laboratory verification and successful on-sky implementation in the MagAO system.
Findings
57% improvement in geometric rms spot size at 2 airmasses
33% improvement in encircled energy at 20 arcsec radius
62% improvement in Strehl ratio compared to doublet ADC
Abstract
We present the novel design, laboratory verification, and on-sky performance of our advanced triplet atmospheric dispersion corrector (ADC), an important component of the Magellan Adaptive Optics system (MagAO), which recently achieved first light in December 2012. High-precision broadband (0.5-1.0 microns) atmospheric dispersion correction at visible wavelengths is essential both for wavefront sensing (WFS) on fainter guide stars, and for performing visible AO science using our VisAO science camera. At 2 airmasses (60 degrees from zenith) and over the waveband 500-1000 nm, our triplet design produces a 57% improvement in geometric rms spot size, a 33% improvement in encircled energy at 20 arcsec radius, and a 62% improvement in Strehl ratio when compared to a conventional doublet design. This triplet design has been fabricated, tested in the lab, and integrated into the MagAO WFS and…
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